^ortl|£ôc0tcnt PntàersHg '^íbrarg ^ôanston, ^limota FROM THE LIBRARY OF DANIEL BONBRIGHT PROFESSOR OF LATIN IN NORTHWESTERN UNIVERSITY 1856-1912 ^ GREAT OUTLINE OF FOR HIGH SCHOOLS AND FAMILIES BY THEODORE S. FAY WITH -A.IT -A. T L-A. S. "Worship him that made heaven, and earth, and the sea, and the fountains of waters." Rev. XIV. 7 BERLIN STILKE & VAN MUYDEN 21. U. d. LINDEN. PARIS & PETERSBURG EMILE MELLIEK. NEW-YORK S. p. PUTNAM it SON. LONDON TRÜBNER & COMP. FLORENCE & TURIN H. LOE8CHER. JíO PREFACE. We have numerous, excellent School-Geographies. Why another? A few lessons, given or received, with the present work, will be a sufficient answer. It is because a large and simple enough circle of geographical knowledge is not generally taught. What countries does the traveler pass through, from Hammerfest to Hobarton — from London to the most populous city of the globe, Han-kow; or from the Baltic to the Adriatic? Why is the arctic circle, or tropic of Cancer, drawn just where it is? Explain the phenomena of the seasons; the condition of day and night, climate, etc., at the different points of the globe's surface. Why has one point of the earth, six months uninterrupted day or night, and another, never more than 12 hours? Why is the winter colder, and the summer hotter, in the S. Hem., than in the northern? Ask these, and similar questions, of young students, who have completed their geographical course; and IV / PREFACE. we shall often perceive that there is room for another geographical School-Book — that there is need of another, wider reaching, and which does its work more thoroughly. Consider, moreover, that the science of Geography itself has recently made striking advances—from geographical discoveries — from the concentration of knowledge in geographical societies — from the perfection to which map-drawing has been brought; and, also, that new political events, in many parts of the globe, have changed territorial limits. Our country has just passed through a great crisis. It is, at last, seated upon the foundations of Law, Liberty and Christianity. It has taken a higher place among the nations, and is beginning to exer¬ cise weightier influence in the councils of mankind. The uttermost corners of the earth are being ex¬ plored. Remote, until now unknown, civilisations are being opened; and steam and electricity are bringing them more within our observation, and in nearer relations with us. The entire Eastern Con¬ tinent is threatened with immense changes. It is pecessary that the American people should follow them with intelligent attention; and the rising gen¬ eration, particularly, require a clearer knowledge, not only of their own, but other countries. They must know the divisions of the whole earth, as they know the States of the Union or the rooms of their houses. Yet more. They must become better acquainted with the planet they inhabit, and with its immense and various populations — fellow- tenants of their wonderful abode. To give this \ \ PREFACE. \ V instruction completely, in a little volume, like the present, is impossible. A part, only, can be first given. What part? That is the question. We bave attempted to discover and separate this part. We present a School - Geography, upon an entirely new principle — a Great Outline, intended equally for the use of persons who have never studied Geography (these will find it a foundation), and for persons who have completed their studies (these will find it a résumé). It includes the main points — the essential parts of the science — that part which all persons will find it most advantageous, as well as most easy, to fix in their minds, and to carry with them through life. If you do not know this Outline, you can have no real knowledge of Geography. If you know it — all other geographical knowledge, which your circumstances may require, will come to you far more easily, indeed almost naturally. How to frame this Outline? What to select and reject? How to introduce it, when framed, into the mind? How to engrave it there permanently? How to give it a power of self-development, so that it will remain in the mind — not a mass of dead facts unconnected with each other — but a living seed, to bring forth fruit in its season? This is the task undertaken by the writer. The friends of education, the teacher, the student are respectfully invited to examine, whether, or not, it is accomplished. It has been said: there is "no royal road to Mathe¬ matics". The author cannot wholly repress the hope that he has cut a shorter and pleasanter pathway to Geography. VI / PREFACE. / Among the advantages oí this method the following may be stated. 1. The teacher reads all lessons from the book. The pupil follows every word upon the plates. He thus studies, at the same time, with his ear and eye. The effect will soon become apparent. 2. No formal demand is made on his memory; yet he cannot help learning by heart, understand¬ ing, and retaining what he has learned; because the book itself teaches him how it must be studied. 3. By an arrangement, equally simple and useful, the confusion of crowded names, on the maps, is avoided. 4. The text is constructed so that the more advanced pupils may easily become competent teachers of other classes. 5. The work will be equally usefiil to mothers, governesses, elder sisters, and brothers, who, even when not prepared by previous study, will find no difficulty, by its aid, in taking the younger mem¬ bers of the family through the whole course. 6. No study at home is necessary. The reci¬ tation is study enough. Thus the trouble of carry¬ ing books backward and forward is avoided. 7. The text is broken apart into 500 or 600 sections, each one carefully arranged after, or rather above the other, so that the ascent is as easy as the steps of a flight of stairs. 8. If any thing is left out, which other School- Geographies give, it is done intentionally, to supply the place with more important matter, which PREFACE. VII others omit. Such remarks, therefore, as "this river''', "that town!', etc., are not given, will, we think, be withdrawn, upon a better understanding of the plan. A man, passing around the globe, does not carry every thing in his knapsack. A correct opinion of the work cannot be formed by turning over the leaves. It is not a book of reference or reading. It is a teaching — a studying book. The text without the plates, or the plates without the text, might be deemed imperfect and unintelligible. They are parts of a machine; and must be used together, like the blades of a pair of scissors. While Parts I. II. and III. give a uniform bird's- eye view of the entire, globe's surface — not by dis¬ jointed maps, on different scales, but by planispheres, presenting whole views of the earth — Parts IV. and V. present outline views of Europe and the United States of America, on a larger scale, applying to them the same principles, which have been previously applied to the entire globe. The writer has not attempted to teach the whole science. Some may object that he has not taught enough. The answer is: learn this first; then it will be time to ask for more. Such as are prepared for more, are referred to Text-book, sections 6 and 98. Lastly, the work is not intended to reflect upon, far less, to displace,any other good School-Geography. We have several which execute, with conscientious¬ ness and success, the task they have undertaken. But that task differs from ours in this. We have blended, into their natural union, astronomical and VIH PREFACE. physical Geography. We have boldly rejected all the usual mass of details, irreconcilable with the simplicity and symmetry of a great, uniform out¬ line— an outline comprehending the entire Earth, and which cannot be properly got into the mind unless it be taken, apart from those details. It is hoped, therefore, that the "Great Outline" will be regarded, by other School-Geographies in the field — not as ati enemy, but as a re-enforcement. PREFACE TO SECOND EDITION. As the best mode of ascertaining imperfections of the first edition, the writer spent some months, teaching a private class selected for that purpose. The result is this second, corrected edition; in which several new names are supplied — the counting is more carefully adjusted — errors and discrepancies are removed — explanations given, in large outlines, of trade winds — tides — ocean- currents, etc., and the lists of names, more freely interspersed with brief, striking descriptions; intended to avoid monotony, awaken curiosity and impart a more living interest to the subject. Berlin, 8. May, 1868. TEXT-BOOK OF GEOGRAPHY. INTRODUCTION. (1.) Geography is a description of the surface of the earth, as the residence of man. " It is generally divided into Ancient and Modern Geography; the first embraces the period of man's residence on the earth, from the beginning of human history till the fall of the Roman Empire; the latter extends from the fall of the R. Empire (sec. 459) to our day.' Geography is subdivided into four departments — Astronomical or Mathematical, Physical, Political, and Historical. Remark to the teacher. Where another section is referred to (as four lines above), it is not intended to be read to the class, on going over this work for the first time, except where it is perceived to be indispensable. The notes, also, at the bottom of the page, may be omitted till the second reading. (2.) Astronomical Geography describes the earth as one of the heavenly bodies — its form, magnitude and place in our solar system — its motions and relations to other celestial bodies, particularly to the sun — the way in which it holds itself as it moves around that central orb, etc. It explains seasons— climates — currents — tides — winds — lines drawn on maps and artificial globes, as arctic circle, tropic of Capricorn, equator, ecliptic, etc. By it we ascertain the true position of places on the earth's surface. 1 2 INTRODUCTION. (ö.) Physical Geography — sometimes termed Natural Geography — describes striking natural features of the earth's surface — configuration of land — phe¬ nomena of the ocean — the soil — modifications of cli¬ mates—of tides—currents—winds, etc., and their physical causes. It also gives a general idea of great land and water divisions — continents — oceans — lakes — islands — peninsulas — capes — mountain-chains — mountain- peaks — rivers — plains — valleys, etc. 4 (4.) Ordinary, Political or Descriptive Ge¬ ography describes the divisions of the earth's surface into countries — empires — republics — kingdoms — states —towns, etc.; and gives some account of their inhabitants — governments — religions— languages — civilisation — natural productions — manufactures — commerce, etc. (5.) Historical Geography treats of the origin of countries — of what, for the sake of convenience, we call the different races and families of man — the great events, changes and revolutions through which they have passed — the enterprises and expeditions, by which we have gradually explored remote continents, islands and oceans; thus obtaining an exact knowledge of the real shape and dimensions of our planet and a tolerable acquaintance with nearly every part of its surface (see sec. 454.). (6.) Purpose of this work. — It is obvious that no mere school-hook can give a complete knowledge of these subjects. All that we can conscientiously promise to teach the young student, is an outline, to he more or less filled up, according to the opportunities and requirements of future life. The want of such a fun¬ damental work has long been felt by every intelligent teacher. We have endeavored to supply it by giving, within the smallest possible compass, and, consequently! by the premeditated sacrifice of many details, such aii outline of perfectly selected, philosophically arranged| INTRODUCTION. 3 and scientifically analyzed geographical facts, as is most necessary, not only for the student of every school, but for all persons in every class of life. And, as it is much more desirable to learn an elemental, definite part of a science thoroughly, than to obtain a larger amount of general knowledge superficially, we have limited our treatment of Astronomical, Physical and Political Geography to an epitome'^, constructed so as to — (we venture here to use this word) force itself into every mind; and to form a solid and permanent foun¬ dation. Whatever may be reasonably desired to complete the circle of Ordinary Geography, will he subsequently supplied by a second Text-book: Outline of Descriptive Geography, nearly ready for publication, containing articles on countries, prominent rivers, mountains, etc. The second Text-book is not necessarily to be taken as a part of this work. The student, after having mastered the latter, will be thoroughly prepared, un¬ aided by any teacher, to pursue his study merely hy reading, with attention, any good Treatise within his reach. The purpose of the second Text-book, is to furnish such a Treatise, framed to suit the knowledge thus acquired, corresponding with the Atlas in his possession, and presenting a clear, panoramic view of the nations now occupying the globe — their degree of christian civilization — the very striking peculiarities of their present position and condition, etc. * EPITOME (e-pit'-o-me) — from a greek word, to cut off, to shorten — a condensed statement containing the substance or essential matter of a subject, disengaged from all such details and digressions as would distract the attention and make it difficult to comprehend the whole and retain it in the memory. 1* PART 1. ASTRONOMICAL GEOGRAPHY. {7.) Starry heavens. — On a cloudless evening, the heavens appear scattered with stars set like gems in the interior of a vast concave. Our eye is not conscious of their unequal distances. Some seem larger than others and sparkle with far more brilliancy. (8.) Number of stars. — A person in the lati¬ tude of the United States can count, with the naked eye, 2 or 3,000. On the equator, where, in 24 hours, the spectator can get a view of the whole heavens without changing his place, he could distinguish about 5,000. The telescope discloses hundreds and thousands of millions — in fact, a number without limit*. \0iV.j ♦ The young student, somewhat advanced in Astron¬ omy, will understand (at least on the second reading of this volume), by the aid of PI. I. B and C, that, if we stood on the North pole, we should never see any part of the heavens except the northern half — on the South pole, except the southern half. But, if we stood on the equator, at midnight of 23. Dec., we should see one half the starry heavens; at midnight of 23. June, the diametrically opposite half (PI. I. C.). On those two nights, we should thus behold all the starry universe within the vision of human beings. On the equator, in consequence of the earth' i daily rotation on its axis, it is true, we should have a view of both sides of the entire heavens in 24: hours; but, during; 12 of those hours, it would be daylight. A8TROKOMICAL GEOGRAPHY. 5 (9.) Fixed Stars. — Except the planets, of which six (in their turns) are visible, all the stars are called Fixed Stars. They are blazing suns, many far ex¬ ceeding our sun in magnitude and brilliancy, but so immeasurably — so unimaginably distant, that the tele¬ scope discovers no disks — no dimensions at all — only inappreciable points of intense light. (10.) Constellations. — Now examine Pl.VIII. A. You there see two groups of fixed stars—that is, two constellations—very conspicuous in our winter night-sky, namely, Orion (O-ri'-on) and Taurus (the Bull). Such groups, from time immemorial, have been named after persons, animals or other objects, and are drawn on maps as in the diagram. You perceive these groups bear little resemblance to the figures after which they are called. Century after century, they appear in the same position with regard to each other. The three stars of Orion's belt thus always remain in a straight line with Sirius. The cluster, Hyades (hy'-a-dez), for thousands of years, has thus represented the letter V, with the red star Aldebaran (al-de-ba'-ran) at one of its extremities; although this letter V, as is the case with other groups and constellations, seems to be con¬ tinually moving through the heavens (around the earth), and consequently always changes its position relative to the person looking at it. You will see the same constellations in the picture of the heavens (PI. I. A). Point out, there, Pleiades (plê-'-ya-dêz), Hyades, Alde¬ baran (in the Bull's eye), the two stars in the tip of the Bull's horn, Orion's belt, Sirius. You would do well, on the first 'clear winter night, to seek out and recognize these constellations and stars in the natural heavens, of which they form the most brilliant ornaments. We shall presently explain why PI. I. A. is entitled: "Imaginary view from Neptune." (Sirius—in Great Dog). (11.) Milky Way. — As the night grows darker, we become more aware of a wonderful, luminous belt 6 ASTRONOMICAL GEOGRAPHY. I or ring, irregolar in outline, breadth and density, extending across the entire heavens, like a zone of indistinct clouds, or a river rolling in soft waves of light. During many ages, the world was unable to account for this. The telescope shows it to consist of masses upon masses of stars (PI. I. A) (594). (12.) Planets. — A slight study of the heavens enables the eye to detect, among the other stars, several, distinguished by the peculiarity that they do not generally sparkle like the fixed stars (although they sometimes do), hut shine with a soft, steady light, like that reflected from the moon*. These are called planets (wanderers), because, while the fixed stars remain thousands of years in the same position relative to each other, the planets, on the contrary, move or wander about, among the fixed stars, backward and forward — so that, in a few nights, or weeks, we can observe that they have changed their positions with regard to the fixed stars, and to each other. When we say, however, that they wander among the fixed stars, we do not mean that they are as far oif as the fixed stars. They are very, very much nearer. They belong to our solar system — heavenly bodies wheeling, at different distances, in the same di¬ rection, and nearly in the same plane, around the sun. While wheeling around the sun they, at the same time, and in the same direction, revolve on their axes. These planets do not, like the fixed stars, shine with their own light,- but are dark, opaque bodies like our earth. They appear bright, only because they reflect back the light received from the sun, as a wall, or a house, or a distant mountain, would. Our earth would appear just as much like a star and just as bright, if we could stand on one of them and look at it. Among the fixed stars (PI. I. A) you will easily distinguish two planets. * It is true, several planets occasionally sparkle, but they may be distinguished from the fixed stars, by a little habitual attention. They often appear ßrst in the evening sky. ASTRONOMICAL GEOGRAPHY. 7 (13.) Solar System — eight principal planets re¬ volving around the sun (PI. VIII. B): Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus (U'-ra-nus) and Neptune (with asteroids, moons, comets and meteors). (14.) Remark. The discovery of a new planet, Vulcan, about half way between the orbit of Mercury and the sun, has been announced. (15.) Asteroids. — an unknown number (100 in 1868) of little worlds — revolving around the sun be¬ tween orbits of Mars and Jupiter (PI. VIII. B) — largest about the size of Long Island — the diameter of one, 14 miles (a journey around his equator, half an hour by railroad, only a pleasant day's walk). Humboldt called them "pocket planets." One, Vesta, sometimes visible, to naked eye. (16.) Planet Neptune — is the most remote from us and from the sun, nearly 3,000 million miles. It is not easy to conceive this distance. Were it pos¬ sible to construct a railroad to Neptune, and the train travel at the rate of 40 miles an hour, day and night, without stopping a single moment, it would reach him in about 8,000 years; a cannon ball, in 456 years; a rapid pedestrian, without stopping to eat or sleep, in about 80,000 years. To walk along the entire path (PI. VIII. B) which Neptune describes around the sun, would require 480,000 years. A ray of light comes from Neptune to the earth in 51/2 hours. (17.) light-Years. — The distance of Neptune is very wonderful, compared with any we can measure on our earth; but the fixed stars are so prodigiously remote that, in proportion, the space, between us and Neptune, diminishes to almost nothing. It would be useless to speak of pedestrians, railroads or even flying cannon-balls,with reference to fixed stars. Astronomers have sought a different standard, namely, light. Light passes 200,000 miles in a second. It could go 8 times 8 ASTRON.OMICAL GEOGRAPHY. around our earth while you count one. It comes frora the sun (PI. VIII. B) to the earth in 8 minutes 18 seconds. It traverses the whole breadth of the solar system (B) in 11 hours. Who then can imagine the distance it travels in a year? Between 6 and 7,000,000,000,000 (seven billion) miles. This distance is called a light-year. A billion is a million times a million. It would take 30,000 years, night and day without stopping, to count one billion. Yet the nearest fixed star, alpha Centauri (Fl. VIII. C), is so remote, 20 billion miles, that it takes a ray of its light 3'/a years to reach our earth. Thus that distance is called 31/2 light-years. It would take, therefore, more than 600,000 years to count the distance, in miles, of the very nearest fixed star. Now what is a light-year? The distance which a ray of light traverses in one year. And what is that distance? Between 6 and 7 billion miles. And what is a billion? A million millions. (18.) Remark. 1. The teacher, according to his dis¬ cretion, will put similar questions. 2. Among the French, a billion is a thousand millions. (19.) Distances of other Fixed Stars. — PI. VIII. C will help you to conceive the amazing distance of even the nearest fixed star. Our entire solar system, (whose dimensions are described in sec. 16) is, in PI. VIII. C, only about as large as the head of a pin. This is the reason why the fixed stars would appear materially in the same form and groups, and at about the same distance, whether seen from Neptune or from our earth. It would make almost as little difference which one of the planets we view the Fixed-Star World from — as which house of a city, or which story of a house. What is the reason? Because the distance is so great that, m comparison*, the whole size of the solar (ly A.J • As, however, the distance between the earth's posi¬ tions, at any two opposite points of its orbit, has alone enabled ASTRONOMICAL GEOGRAPHY. 9 system would scarcely be greater than the head of a pin. PL VIII. C gives the distance of the principal stars which have been measured. The star called alpha Centauri, S'/j light-years — that numbered 61 in Cygnus, 91/2—Vega, IS'/î — Arcturus, 26 — Sirius, 22 — Iota, in Great Bear, 25—Polar Star, 31 — Capella, 72. These stars are tfw very nearest to our solar system. The others are too distant for measurement; the Milky Way, thousands of light-years; other starry systems, called nebulae (outside of—far, far beyond the Milky Way), probably millions of light-years distant. In PI. VIII. C the solar system is given as a point. The fixed stars, alpha Centauri, etc., are at different distances from it. The dotted lines give the relative distances of those fixed stars, compared one with the other-, for instance, Capella is nearly three times farther, from the solar system, than Iota, in the Great Bear, is; but these lines are not intended to show the distance of any star, compared with the size of the solar system. ( 19 B') Remark to teacher. — If any pupil here inquire what man knows as to the origin, dimensions and duration of the physical universe, it wonld not be proper to leave such a (juestion without reply. Modern atheists declare the world infinite in extent and duration — without beginning and without end. This assertion rests on no proof. According to Scripture, it had a beginning. It has limits. The stars are numbered. Each one has a name (98 B). The hints of the Bible on these, and other similar points, are among the eternal evidences of its divine origin ; not only from their superhuman sublimity, and their wonderful correspond¬ ence with each other, during all the centuries from Job and Moses to Paul and John; but from their correspondence with the discoveries of modern science. As to the duration of the universe, the sacred page represents it as destined to undergo the most amazing trans¬ formations in its progress to a state of far higher, eternal perfection. (20.) Imaginary view of the heavens from Neptune — Our earth a star. — We cannot see Neptune, from our earth, with the naked eye; scarcely with a telescope. Indeed his existence was unknown astronomers to measure a few of the fixed stars, it is pretty certain that more could be measured from Neptune-, because the diameter of his orbit is so much greater than that of the earth (595). 10 ASTRONOMICAL GEOGRAPHY. till 1846. He is far larger than the earth, his diame¬ ter being more than 4 times greater. Suppose we had a Car, propelled by light, in which we could visit the heavenly bodies. Imagine yourself (PI. I. A) thus arrived upon that dark, cold, remote planet. The starry heavens are drawn as they appear from our earth on a winter night. You easily recognize Orion and his belt; Taurus, with the two clusters, Hyades and Pleiades; two stars in the tip of the Bull's horn; the brilliant star Aldebaran; Sirius, etc. The sun, although, from our earth, too dazzling to be looked at, seen from Neptune, would dwindle to a compara¬ tively insignificant luminary 1,300 times weaker than he appears to us. We may well imagine an occasional winter day of that planet so nearly resembling in darkness some of the nights of our earth, as to afford a view of the starry heavens. Although, from Neptune, we should see the same fixed stars, as from our earth, several of the planets, which ornament our sky, would not be visible, at least to the naked eye. A glance at PI. VIII. B will show the reason why Mercury, Venus, Mars, Jupiter and Saturn are visible to us inhabitants of the earth; Uranus, scarcely; Neptune, not at all, with the unassisted eye. From Neptune, on the con¬ trary, we should easily distinguish those nearest him — Uranus, Saturn and Jupiter. Two of these will be found in the picture (PI. I. A). If really on Neptune, we should naturally cast our eyes over the heavens in search of the little planet on which we had lived. Its distance, perhaps its proximity to the sun, would bide it from our view. If we had a sufficiently powerful telescope, however, we might detect, very near the sun, a small star — a distant point of light — an atom of gold dust floating in free space among the millions of other worlds. That is our Earth (star nearest the .sun, PI. I. A) (596). (21.) Nearer view of the Earth. — Let us now leave Neptune in our Light-Car, and, instead of visiting ASTRONOMICAL GEOGRAPHY. 11 any other heavenly body, let us choose a point, in free space, so near, that the earth would appear somewhat as it does in PI. I. B. We here arrest our Car in full sight of the earth, to explain the meaning of several terms connected with Astronomical or Mathematical Geography. Take PI. VIII. and PI. I. (22.) The Earth an oblate spheroid (PI.I. B). You there see the earth — a round body — an orb — a sphere — a globe. A globe is a round, spherical body whose surface is, in every part, equally distant from the center. What is a globe? The earth is so nearly a perfect sphere that it would not be possible to rep¬ resent it correctly in a picture, except by an absolute¬ ly spherical figure. Its stupendous mass, however, has been measured with wonderful accuracy and the discovery made that it is not a perfect sphere. It was once, and perhaps still is, a flexible body—that is, yielding and capable of being bent without breaking. By its diurnal rotation, the equatorial mass has been thrown a little out, and the parts about the poles, in a corresponding degree, drawn in. Its circumference, at the equator, is 24,899 english statute miles; its polar circumference, less. Its diameter is, therefore, greater at the equator than at the poles, the former 7,907Ys miles; the latter 7,880 miles. The différence therefore is 27 Vs miles, very little, compared with the dimensions of the whole planet; each pole being only about 13 miles nearer the center, than the equator is*. Its real figure is called an ohlate spheroid, that is, a figure not absolutely a sphere. PI. VIII. M gives the real figure of the earth but, of course, in an exagger¬ ated form. The same Plate (D) gives the earth with notes of its dimensions. (22 A.) * "We have reason to believe the equator to be not strictly circular, but in some degree, elliptic; the proportion of its greatest and least diameters not being yet precisely known, though very much nearer to equality than that of the equatorial and polar diameters." (Sir John Herschel.) 12 ASTRONOMICAL GEOGRAPHY. (23.) Axis — Pole — Bevoliition — Bota- tion. — PI. VIII. E represents a wooden globe, with an iron rod passing through its center and projecting at each extremity. One end of the rod rests on the floor, the other is held by my hand. Now suppose this globe to turn over and over, on the rod, from the direction of the word west, to that of the word east. It would revolve, or rotate, on the rod, from west to east. The rod would be its axis-, the points of the two extremities, where they reach the circumference, would be the two -poles of the globe. The two poles then are the only two points of the globe which do not revolve; and, remember, the N. Pole of the earth, during its whole annual revolution around the sun, always points to the N. Star. Now look at PI. I. B. The earth revolves in this way, on its axis, from "W. to E., and in the same oblique position relative to the ecliptic, as the wooden globe in the diagram, with its N. Pole pointing to the N. Star. Only it has no rod. The earth and other plan¬ ets revolve on their axes, in the void of space, un¬ supported by any rod, floor or hand, except that of the Creator. "He hangeth the earth upon nothing". The axis of the earth in B. is represented by a line drawn through the earth's center. Those two points, where the axis reaches the circumference of the earth, are called its poles. A man standing in the picture B, where the word west is written, would be carried completely around by the rotation of the earth, and would thus, in 24 hours, get a view of every portion of the celestial sphere (see sec. 8). But a man standing at the N. Pole, immediately beneath the N. Star, would not he carried away from that position at all. The N. Star would he in his zenith (33) directly above his head, and would remain so during the whole rotation; although the rest of the heavens, above his horizon, would seem to revolve around him, without ever descend¬ ing beneath his horizon. What is the earth's axis? ASTRONOMICAL GEOGRAPHY. 13 An imaginary straight line, on which the earth revolves from west to east, once in every 24 hours. (24). Remark. Speaking with astronomical accuracy, the earth revolves once every 23 hours, 56 minutes, 4 seconds and nine one-hundredths of a second. This daily rotation is performed with a punctuality which has no parallel within human knowledge. It has not varied the one-hundredth of a second in 2000 years. (25.) North Star and Great Bear. — The earth is surrounded on every side by stars (PI. I. A and B). Wherever we travel over its surface, we find the night heavens scattered with thousands, and, when observed through a telescope, thousands of millions of stars. One of these, the North Star or Polar Star is always to be found in our heavens, over the back of the con¬ stellation, the Great Bear. Its position may be seen in PI. VIII. F. You will easily recognize* the Great Bear on any clear night, and the two stars called the pointers, point¬ ing to the N. Star. In the course of 24 hours the Great Bear and all the stars of the heavens seem to revolve around the N. Star. The diagram represents the Great Bear at 4 different periods of the 24 hours — 6 o'clock in the evening, 12 at night, 6 in the morning, 12 the next day (noon)—at the latter hour, of course, invisible on account of the daylight. (26.) Remark. He does not always stand with his feet toward your horizon at 6 o'clock in the evening. He stands with his feet toward your horizon once every 24 hours; but is seen in that position, at 6 o'clock in the evening, only once during the year. (27.) North Star stationary. — The N. Star is thus the only star which does not seem to revolve every 24 hours; the reason has been seen (PI. I. B and PI. VIII. E). As the earth revolves from W. to E., the whole heavens appear to revolve from E. to 14 ASTRONOMICAL GEOGRAPHY. W. As the N. Pole of the earth points to the N. Star, and the poles are the only points of the earth which do not revolve, so the N. Star is the only point of our heavens which does not seem to revolve. (28.) North — South — East — West. — (PI. I. B) North, toward the North Pole; South, toward the opposite Pole. When you stand on the globe's surface with your face toward the North Pole, your right hand is toward the East; your left toward the West. (29.) Equator of the earth — hemisphere.— The equator is a large circle, supposed to be drawn around the earth, equi-distant from the poles. It is marked upon the earth in PI. I. B. It divides the globe into two equal parts. Northern hemisphere and Southern hemisphere (half sphere). We often hear also the terms Eastern, Western, Land and Water hemispheres. Each half of the globe is a hemisphere. (30.) Sensible Horizon.—Wherever we are — on a plain, at sea, on a desert, on a mountain—we have a circular view. A circle appears drawn around us, beyond which we can see no more of the earth's surface and no more of the etherial concave. At the center of this circle we stand; at the circumference of it, the earth and sky seem to meet. This circle — when applied to our earth — is called our sensible horizon (from a greek word, I terminate). It contracts or enlarges of course according to the elevation of the spectator. Upon the ocean, supposing our eye to be elevated 5 or 6 feet, the diameter of the sensible horizon would be only about 3 miles. The summits of lofty objects, as a mountain, or the masts of a ship, can be seen at a greater distance — in favorable weather, the Peak of Teneriffe, at the distance of a hundred miles. Now what is the sensible horizon? It is a small circle, bounding our view of the earth's surface, in the center of which, we stand, and at the circumference of which, the earth and sky seem to meet. ASTRONOMICAL GEOGRAPHY. 15 (31.) national Horizon.—If we were suspended (in our Light-Car) in free space, the earth not existing at all, how would the heavens appear? A vast, hollow sphere, of which we should see the whole interior. The Milky Way would present itself a continuous ring, one half over our head, the other, beneath our feet. There would thus be no horizon, either sensible or rational. As, however, we stand, not in free space, but upon the stupendous, convex globe, our view is quite different; and, wherever we stand upon its surface, we can see, never the whole, but always exactly one half of tl\e Celestial Sphere. The other half is, of course, hidden by the globe itself; and our view is limited by a great circle, of which our eye forms the central point. This great circle is called our rational horizon. Thus the rational or true horizon divides the heavens into two equal parts, the one visible, the other invisible. These two horizons are, in one sense, the same. While the term sensible horizon is applied to the small circle which terminates our very contracted view of the earth's sur¬ face, the term rational horizon is applied to that great circle which terminates our view of the immense celestial concave, cutting off the lower half of it from our sight. Now what is the rational horizon? You will not perhaps, immediately understand what is meant by the further explanation that, the rational horizon is also an imaginary plane extending, through the center of the earth, on every side, to the starry heavens, thus cutting into two halves, both the heavens and the earth. The sun, moon and stars become visible to us, when they rise above this plane. (32.) Axis of the heavens — apparent daily revolution of the Celestial Sphere npon it. — PI. I. B shows a line reaching, through the earth's center, across the heavens, to the N. Star, and to a corresponding point in the southern heavens. The axis of the heavens is an imaginary line 16 ASTRONOMICAL GEOGRAPHY. identical* with the axis of the earth, — a prolongation of it. The entire hollow sphere of the starry heavens appears to revolve upon it from E. to W., and the northern extremity of it passes through, or very near the N. Star. As the earth, with its N. Pole always pointing to the N. Star, revolves, once every day, on its imaginary axis, from W. to E. —, that motion makes the great starry concave, called the Celestial Sphere, seem to revolve, once every day, from E. to W., on the imaginary line, called the axis of the heavens. The atmosphere, forming an envelope around the earth about 500 miles high, accompanies the planet in all its movements, with no other consequent disturbance than the trade- winds and the storms connected with them. Thus — the clouds — the birds — man — the atmosphere itself—are borne softly around, with the earth, in its annual and diurnal rotation. Kther, which is believed, to fill all space, is too rare and delicate to offer any perceptible resistance; so that we are unconscious of the earth's motion, and have no means of discovering it, except by watching disconnected objects, quite apart from it, and not moving with it, snch as the sun, moon and stars. These, of course, seem to revolve in a contrary direction, on an axis exactly corresponding to the earth's axis, that is the axis of the heavens. The two points of the heavenly sphere (at the extrem¬ ities of its axis) which do not seem to revolve, are called its poles. The N. pole of the heavens is at the North Star — the S. pole, opposite the S. pole of the earth, is, of course, as far heneath our southern horizon, as the N. pole of the heavens is above it. (Please here read 597.) — (for trade-winds, 603). (33.) Zenith (zee'-nith) — is that point of the visible celestial sphere vertical to the spectator, that * IDENTICAL; the same; not different; from the Latin, idem, the same. ASTRONOMICAL GEOGRAPHY. 17 is, directly over the place where he stands. A man standing on the N. pole (PI. I. B) would have the North Star in his zenith. (34.) Nadir (nä-dir) — that point of the heavens directly opposite the zenith — directly under the observer's feet. A perpendicular line drawn from the zenith, through the spectator, and through the center of the earth, to the opposite point of the lower celestial hemisphere, would extent to the nadir. At noon, 23. of June (PI. I. B), a person, on the tropic of Cancer, would have the sun in his zenith. The center of the sun would be vertical, that is, exactly over his head. Zenith and nadir are arabic terms. (35.) Right line or straight line — shortest line between two points. (36.) Curve line — a line which departs con¬ tinually from a direct course. Remark. 1. The diagrams referred to, in sections 35 to 55, will easily be found in PI. VIII. 2. Our plan requires that the pupil should not be instructed, at this stage of his studies, on any other points than those presented in the text. The subjects explained have reference to future lessons. As much care has been taken to exclude explanations not yet needed, as to furnish those necessary. The object is to teach, not Geometry nor Astronomy, but Geography ; and that, only ascending step by step. (37.) Parallel lines — lines extended in the same direction and equally distant from each other throughout the whole length. (38.) Oblique lines. — Oblique means slanting. Oblique lines are such as are inclined toward each other from a direct line, whether horizontal or perpendicular. 2 18 astronomical geography. (39.) Horizontal line — a level line par¬ allel to the horizon. (40.) Perpendicular line. — When one straight line stands upon another, so as to make the angles, on each side, equal to each other — that is, neither leaning to one side, nor to the other — the lines are said to be perpendicular to each other — as in the diagram entitled "right angle". (41.) Angle — the space comprised between two straight lines that meet in a point. (42.) Bight angle — formed when one right line intersects another right line perpendicularly. (43.) Acute angle — less than a right angle. (44.) Obtuse angle — greater than a right angle. (45.) Circle — Center. — A circle is a single curve line, every part of which is equi-distant from a point called its center. The six following sections describe parts of a circle (PI. Vm. Q): (46.) Circumference. — The curve line that encompasses a circle — about three times the diameter. (47.) Arc (P) — any portion of the circumference of a circle. In the figure there are three arcs and three chords. (48.) Chord (P) — a right line joining the extremities of an arc. (49.) Diameter (Q) — a straight line from any point of the circumference passing through the ASTRONOMICAL GEOGRAPHY. n center to the opposite point. It divides the circlet into two equal parts. (50.) Eadius (ra-di-us) (Q) — a straight line drawn from the center to the circumference. All radii of the same circle are equal to each other and each is half the diameter. Radii, the plural of radius. (51.) Quadrant (Q) — one quarter of a circle or 90 0 (the circle being divided into 360®). The circumference of the globe, from the equator to the pole, is 90®—that is a quadrant. (52.) Remark. The terras drcumferenee B,Tidi diameter are equally applied to a globe and other solid bodies. (53.) Concentric Circles (P) — circles drawn within each other which, although of different dimen¬ sions, have a common center. (54.) Great Circle — Small Circle. — A circle drawn around the earth may be either great or small. A great circle passes around its greatest circumference and divides its surface into two equal parts or hemispheres. The equator, therefore, is a great circle. The meridians are great circles. The ecliptic, sometimes drawn upon maps and globes (E), is also a great circle. All other circles drawn around the earth are small circles. In PI. VIII. S. you see the equator drawn completely around the globe as a great circle, while the two tropics and the two polar circles appear as small ones. Examine the great and small circles upon all the figures of the earth in PI. I. (55.) Ellipse — Focus (P). — An ellipse is an oblong figure, such as a circle would appear if held obliquely (as the cart-wheel i in PI. VIII. L). The figure of an ellipse is described around two points, called its foci (the plural of focus). 2* ■20 ASTRONOMICAL GEOGRAPHY. (56.) Latitude (R) — upon the earth, is distance from the equator, north or south, reckoned, toward the poles, in degrees, minutes and seconds. In plani- globes (PI. II for instance), it is marked on the entire circumference; in other maps (Pis. IV. VI. etc.), on the right and left margins. In PL VIII. R. you see the equator and four parallels drawn at 20® N. lat., at 40®, 60® and 80®. There is also in diagr. R. the same number of south parallels. The pole is of course at the 90® of latitude. No place can be farther from the equator than the pole; so no place can have a higher latitude than 90®. When, in your journey N. or S. from the equator, you pass the point called thé pole, in what direction must you go? Answer: In passing the North pole, we must go south-, of course, we then approach the equator on the opposite side of the globe; in passing the .South pole, of course, we go north, toward the equator. (57.) Parallels of Latitude (R) — shortly called Parallels — are small circles supposed to be drawn around the earth parallel to, and at different distances from, the equator. (58.) Longitude (R) — distance of a place, E. or W., from any given meridian, and, like latitude, measured in degrees, minutes and seconds. In plani- globes (PI. II), it is marked, by the arabic figures, on the equator and on the two parallels, nearest the poles; in other maps (PI. IV, VI. VII, etc.), on the top and bottom margins. (59.) Meridians (R) — great circles supposed to be drawn around the globe and to pass through the poles of the earth, intersecting the equator at right angles. Each of them divides the sphere into two hemispheres. For parallels and meridians see also all figures of the earth in PI. I. Point out there the par¬ allels; the meridians. ASTRONOMICAL GEOGRAPHY. 21 (60.) Degrees — Minutes — Seconds. — A circle is supposed to be divided into 360 equal parts. Each part is called a degree, expressed by a small sign, thus (®). Take PI. VIII. T. Each degree is subdivided into 60 equal parts, called minutes, marked by a comma, thus ('); and each minute is subdivided into 60 equal parts, called seconds, marked by two commas, thus ("). We write 10 degrees, 5 minutes, and 4 seconds (as in T)—10» 5' 4". (61.) How an angle is measured. —An angle is measured (PI. VIH. T.) by making its sides radii of a circle and taking the length of the arc in degrees, minutes, and seconds. Diagram T. (fig. o) shows a circle divided into 360®. You, must imagine each degree to be subdivided into 60', and each minute, into 60". Fig. h shows a right angle measured on the arc of the circle, the arc here, being exactly a quarter of the circle, meas¬ ures 90". In fig. c the two lines e. f. form an acute angle of 23" 27' 26" (twenty-three degrees, twenty- seven minutes, twenty-six seconds). The two lines g. h. form the same angle of 23" 27' 26". Fig. T. c- is drawn in the same position as that in which the earth holds itself, in its annual journey around the sun. The line g represents the equator ; the line h, the ecliptic, or the plane of the ecliptic, or the plane of the earth's annual orbit or path around the sun. Hence we say the equator is inclined to the ecliptic 23" 27' 26". (62.) Remarle. Young people, who cannot com¬ prehend what is meant by such phrases as "inclination of the equator to the ecliptic" — "plane of the ecliptic" — "plane of the earth's orMt" — "earth's axis leans 23^ 27' 26" toward the ecliptic", etc. — must not be dis¬ couraged. Let them mark these phrases well, whether they understand them or not; and the meaning will, we trust, become gradually clear. It is scarcely possible for an inexperienced student to grasp these ideas by 22 ASTRONOMICAL GEOGRAPHY. any single explanation. He must, by a series of ex¬ planations, following each other in a carefully arranged succession, slowly ascend to a point, where the earth's true position, with its axis inclined toward the plane of its orbit, and thus holding itself, obliquely^ as it annually moves around the sun, will at last break upon him, like the effect of a stereoscope. Hence our readers will find several apparent repetitions, which however are not accidental, but premeditated. (63.) Plane. — When a ball rolls on a level meadow or floor, it rolls on a plain. The solar system consists principally of the sun with eight planets, revolving around him in nearly the same level or plane, as if they were rolling on a floor. The word ^lain means smooth — even — level — flat — without elevations or de¬ pressions. But when astronomers describe the planets revolving around the sun, áll of them in about the same level, just as if they were rolling on a great level or plain in space, they use the word plane. (63 A.) PI. Vni. G. will aid in giving an idea of the plane of an orbit and how planes may be inclined or perpendicular to each other. It represents the inte¬ rior of a room. At A, the planets revolve on the plane of the floor; at C, on an inclined part of the ceil¬ ing; at B and Z), on two walls perpendicular to each other and to the floor. We here see that the expres¬ sion, the "earth's orbif, and the "plane of the earth's orbit", are not to be confounded with each other. The line, marked "earth's orbit", describes the path which the earth pursues around the sun. It is therefore a line—a curve line. The plane of the earth's orbit is the level or plane in which this line or orbit lies, that is, in which the earth revolves. In PI. VHI. G. it is the floor, or the walls, or the ceiling. In the solar system itself, there is no floor; but the earth and planets revolve in about the same plane, as if there were a floor. That imaginary floor, extended out in every di¬ rection, is the plane of their orbits. ASTRONOMICAL GEOGRAPHY. 23 (6 3 B.) PL Vni. L. will help you to understand this. A cart-wheel is held up to your eye in different positions. At a, it is a circle. You have only to suppose the sun in the center, and then the circum¬ ference or tire of the wheel to be the orbit of the earth. You can hold it up before you so that the tire will appear a circle. If you were directly above the orbit of the earth, ii, also, would be a circle, as at a. If you were to take another stand-point, half on one side, the earth's orbit would appear as in h. But, if you were to go quite on one side of the earth's orbit, it could then be represented as a straight line, as in c. Your eye would then be said to be in the plone of the earth's orbit. The earth's orbit thus (PI. VIII. L. c) is given as a line; and the plane of the earth's orbit is repre¬ sented as a line. A figure of the earth is drawn in the wheel c to show the inclination of the axis and the equator, to the plane of the orbit. The equator, as we have seen, forms an angle of 23® 27' 26"; and the axis leans, from a perpendicular, 23® 27' 26". In B and C, Plate I, the earth is drawn in this position; the orbit, and the plane of the orbit, are each represented by a line instead of a circle. In D, the orbit is drawn as the wheel at h. In PI. VIII. B. the orbits of the planets are seen from the same stand¬ point as the wheel at a. (64.) Ecliptic — plane of the ecliptic — angle formed by equator and ecliptic (or by their planes). — If we suppose ourselves standing outside of the solar system and looking upon the circle which the earth describes around the sun (PI. VIII. G. a), we call that the orUt of the earth. But, as we stand upon the earth, we are not conscious that the earth moves annually around the sun. It seems to us that the sun moves annually around the earth. The circle, in which he seems to move, is called the ecliptic. Thus the ecliptic must be defined by a double definition. 24 ASTRONOMICAL GE06RAFHT. First, it is the orbit in which the sun seems to move, once every year, around the earth. Secondly, it is the orbit in which the earth really does move once every year around the sun. In PI. VIII. G. you have several views of the earth's orbit; in one. Mercury, Venus and the Earth revolve on the floor. The line in which the earth there revolves around the sun, is the earth's orbit^ the floor is the plane of the earth's orbit. But, remember, to the people upon the earth, the earth seems to stand still; and the sun seems to go around the earth in a circle just like that in which the earth goes around the sun. The orbit of the earth, therefore, is the ecliptic, and the ecliptic, although it does not so appear to us, is, in reality, the orbit of the earth. They are quite the same. The floor is, at the same time, the plane of the earth's orbit and the plane of the ecliptic. Now when we describe the position, in which the earth holds itself, as it goes around the sun, it is usual to represent the plane of the ecliptic as a line, and the plane of the equator as a line; and thus to show what angle they form together. PI. I. B. shows it clearly. The earth holds its axis with regard to the ecliptic so that the equator forms an angle of 23® 27' 26". Astronomers, in describing the earth's position, therefore, say "the obliquity of the equator is 23" 27' 26"". The earth's position may be described however in an¬ other way. The axis is inclined 23" 27' 26" toward the ecliptic, i. e. away from a perpendicular line. In PI. I. B. the line of the shadow forms the perpendic¬ ular; and the distance of the N. Pole from that line is 23® 27' 26"—exactly the same as that from the ecliptic to the equator. Remark. We have now commenced to acquire some idea of various terms generally used in explain¬ ing the four seasons, climates, and the inequalities of day and night. SEASONS. 25 SEASONS. (65.) Succession of Seasons. — For thousands of years, mankind Tainly endeavored to account for the phenomena of the seasons. At one period, we are conscious of oppressive light and heat; at another, we pass into a gloomy shadow, and suffer from darkness and cold. Spring and autumn bring days and nights equal all over the globe. In our midsummer, the sun remains 12 hours above the horizon at the equator; 24 hours at the arctic circle; and 6 months at the N. Pole. In our midwinter, the sun remains iemath our horizon 24 hours, at the arctic circle, and 6 months at the N. Pole. As man became better acquainted with the shape and surface of our planet, it was discovered that the S. hemisphere underwent the same ever varying revolutions of heat and cold, winter and summer, as the N. hemisphere, with a perfectly mathematical corre¬ spondence, except at diametrically opposite periods. These changes follow each other annually with extra¬ ordinary regularity. The true explanation was given, about 300 years ago, by Copernicus, who demonstrated that the earth was not a fixed point, with the sun and heavens revolving around it, once every day, and then, again, once every year, (as, to its inhabitants, seems to be the case; and as Ptolemy and other learned men had taught), but that it daily rotates, on its axis, and, at the same time, moves annually around the sun. The causes of the seasons are as simple as the reason why the sunny side of a house is warmer than the shady side; or why one side of a house may be shady in the morning and sunshiny in the afternoon. (66.) Earth at midsummer. — In PI. J. B. we have the earth, 21 — 23 June. You see the equator drawn equally distant from either pole. N. of equator are two parallel circles — tropic of Cancer and arctic circle; S. of equator—tropic of Capricorn and ant-» arctic circle. 26 ASTRONOMICAL GEOGRAPHY. Remark ten phenomena (fig. F): Summer and longest day in N. hemisphere. Winter and shortest day in S. hemisphere. Greatest inequality in length of day and night everywhere except on equator. This inequality in¬ creases as you approach either pole — i. e., the day is longer, the farther you go N., till you come to a re¬ gion where there is no night at all; and the day is shorter, the farther you go S., till you come to a re¬ gion where there is no day at all. Sun's center as far N. as tropic of Cancer. Within arctic circle no night. Within antarctic circle no day. At point of N. Pole, noon of a day which lasts six months. At point of S. Pole, midnight of a night which lasts six months. Between arctic circle and N. Pole (that is every¬ where within arctic circle), a day varying in length from 6 months to 24 hours (with a night the same in the antarctic circle). Between arctic circle and equator, a day varying from 24 hours to 12 hours, and between the antarctic circle and equator, a night varying from 24 hours to 12 hours. Every season, in one hemisphere, exactly the reverse of that in the other. This is the state of our earth on 21—23 June. (67.) Suppose earth stationary 23. June. — If the earth did not move in its annual orbit around the sun, this condition would be permanent. The daily revolution would never bring any point, lying within the arctic circle, away from the sun's rays, nor any part, within the antarctic circle, out of the earth's shadow. At one pole, it would be uninterrupted sum¬ mer and day; at the other, uninterrupted winter and night. The condition of the countries, lying on or near the equator, would scarcely be changed from that SEASONS. 27 which they actually always enjoy; except that those, lying on tropic of Cancer, would have the central point of the sun in their zenith permanently; while those, on tropic of Capricorn, would see him far to the North, We, in the United States, should have an unchanging summer, always long days and short nights, as on the 21—23. of June. The length of the day and night, at any given latitude, would never vary. (68.) Earth at midwinter. — PI. I. C. is an illustration of the four seasons. The earth is visible at 3 points of its orbit. A figure of the earth is supposed to be also at the point opposite 2 (of course on the other side of the sun and thus hidden from our eye). At 1, we have the earth as already given in B; 3 represents the earth on the 23. of December. Point out these figures; name the 5 principal circles. The ten phenomena, marking the 23 of June, are here exactly reversed (fig. 3). Winter and shortest day in N. hemisphere. Summer and longest day in S. hemisphere. Greatest inequality in length of day and night everywhere except on equator, but in an inverted order; and in a ratio always increasing as you approach either pole. Sun's center as far S. as tropic of Capricorn. Within arctic circle no day. Within antarctic circle no night. At the point called S. Pole, noon of a day which lasts six months. At the point called N. Pole, midnight of a night which lasts six months. . Between antarctic circle and S. Pole (that is everywhere within antarctic circle), a day varying in length from 6 months to 24 hours (with a night the same in the arctic circle). Between antarctic circle and equator, a day varying in length from 24 hours to 12 hours (night the same from arctic circle to equator). 28 ASTRONOMICAL GEOGRAPHY. Condition of equatorial regions little changed. Only difference—the central point of the sun is per¬ pendicular over tropic of Capricorn instead of tropic of Cancer, The people on the equator have him on the S., -whereas on the 23. of June, they have him on the N. (in fig. 1.). (69.) Solstices and Eqninoxes. — Let us now (C) follow the earth in its annual movement around the sun and watch the coming on and passing away of the summer, autumn, winter and spring. We are supposed to be in a position, where the orhit of the earth is turned toward us, like the edge of the wheel in PI. VIII. L. fig. c—that is, where our eye is in the plane of the earth's orhit. Thus we see the orhit, not as a circle, hut as a line. Now take PI. I. C. again. The earth is represented in 4 points of its orhit — 1. summer solstice (N. hem.); 2. autumnal equinox; 3. winter solstice; 4. spring equinox (at the point exactly opposite to, and behind the sun). (70.) Summer solstice. — Fig. 1 represents the earth as having reached the point of midsummer, the 21 of June. It is here at its summer solstice (from two latin words, meaning the sun and to stand), because, at this part of the year, from the shape of the earth's orhit, and the inclination of its axis, the increase and decrease in the length of day and night are, for some days, less than usual. The earth thus seems to stand still. The sun thus seems to stand still. (71.) Autumnal equinox. — We behold the globe move slowly around in the direction of the arrow. In three months, it reaches the position of fig. 2. It is then the 21. of September — our autumnal equinox. Which pole is there turned the most toward the sun? (For all these sections, PI. I. both C and D.) Neither (nee-ther) one nor the other. Each pole is turned equally toward him. The earth is turned sideways SEA.80NS. 29 toward him. The sun's center is directly over the equator. He is said here to cross the equator, because he is just now in the zenith of the people on the equator. In fig. 1, our midsummer day,^ he was in the zenith of the people on tropic of Cancer ; in fig. 3, our midwinter day, he will be in the zenith of, that is vertical to — the people on tropic of Capricorn. At fig. 2, our autumnal equinox (21. of Sept.), he is vertical to the people on equator who see him exactly over their heads (only for one day), because he is passing on his way from tropic of Cancer to tropic of Cap¬ ricorn. At fig. 4, he will cross the equator again on his way back to tropic.of Cancer. He is thus said to cross the equator, or to cross the line, at our autumnal and spring equinoxes. In fig. 2, the whole of the E. hemisphere is turned toward the sun's light; the whole of the W. hemisphere is turned away from it. It is therefore, at this moment, midnight in America and noon in Asia; and the days and nights are equal on every part of the earth's surface —12 hours night and 12 hours day at the equator — also 12 hours night and 12 hours day at each of the two poles. This, and the corresponding opposite point of the year, are called equinoxes (from two latin words signifying equal and night.') It is called our autumnal' equinox, because it is autumn. We are just half way on our journey from the point where we had the longest summer day, to the point where we shall have the longest winter night. What is the condition of the two poles at fig. 2? The N. Pole has its autumnal equinox. Day and night are equal. It is just bidding adieu to its long Summer and entering upon its long winter. The sun, which has been visible for six months, now sinks be¬ neath the horizon, to remain invisible for the next six months. He will reappear, at that pole, about the 21. of March, when the earth shall have completely passed on to the other side of the sun. At the S. Pole, the condition is reversed. The sun is, there, just rising above the horizon, to remain 30 ASTRONOMICAL OROGRAPHY. till the 21. of March. Summer begins to break over the S. hemisphere. The days grow longer, the nights shorter. (72.) Winter solstice (fig. 3). — Watch the progress of our planet three months more. It slowly advances to the point 3, where we have winter in the N. hemisphere with the longest night and the shortest day. This is called, in the N. hemisphere, the winter solstice; of course it is the summer solstice in the 8. hemisphere. (73.) Spring or vernal equinox. — In three months more, the earth moves to the point opposite that occupied by the central fig. 2; being covered by fig. 2. and also by the sun, it is of course invisible in Pi. I. C. It is now our spring or vernal equinox. Instead of bidding farewell to the summer, we are now advancing to meet that season. The phenomena of the autumnal equinox are here exactly repeated — the two poles turned neither toward the sun, nor away from him; the sun's burning orb exactly over the heads of the nations on the equator (of course at their noon) so that each pole receives «n equal portion of his light; day and night are equal; exactly 12 hours each, on every part of the earth's surface—even at the poles. This entire equality of day and night (or of light and darkness) which at the equator is perpet¬ ual, extends over the whole earth twice a year, and lasts only 24 hours. (74.) Unequal length of seasons. (PI. VIII. K) — The seasons are not of the same length. In the N. hemisphere the winter is the shortest, the summer the longest. The autumn is shorter than the spring. The exact duration is given in the following table. Winter 88 days 19 hours 29 minutes. Autumn 89 „ 17 „ 24 „ Spring. 92 „ 21 „ 11 „ Summer 93 „ 13 „ 56 , SEASONS. 31 The summer is thus 16 hours 48 minutes longer than the spring, and 4 days 18 hours and 27 minutes longer than the winter. The spring is 3 days 3 hours 47 minutes longer than the autumn. (598.) (74 A.) Remark. "We may well here pause to observe the exactness with which that divine creation, called the solar system, performs its operations. It has been seen that the time of the earth's daily revolution, for thousands of years, has not varied the hundredth part of a second; and here, the relative length of each returning season is found to be always precisely the same. It is true that, on looking deeper, there appear certain irreg¬ ularities. But, on looking still deeper, these supposed irregularities are discovered to be limited by precise periods and to be in conformity to regular, eternal laws. May we not infer that the.moral world, also, is guided by the same supreme, omnipotent Intelligence — that its seeming irregularities, also, are measured by periods, and subject to laws, and that they will finally disappear altogether, or appear only as necessary parts of one harmonious whole (98 — 98 A). (74 B.) Another phenomenon connected with the seasons is the symmetrical correspondence in the S. hemi¬ sphere, where the above given inequalities of duration in the N. hemisphere, are diametrically reversed. The winter of the S. hemisphere is not only longer, hut colder in proportion; and the summer, not only shorter but warmer in proportion. This would not be the case, if the earth's orbit were a circle. The seasons, in that case, would be of equal length. The sun would be in the center of the circle. The distance traversed by the earth, during each of the four seasons, would then be absolutely equal, and the earth would move, during these four seasons, and over every portion of her orbit, with the same invariable velocity. This equality is disturbed by the real form of the earth's orbit, which is not a perfect circle with the sun in its center. It is an ellipse, with the sun, not in its center, but in one of the foci. 32 ASTRONOMICAL GEOGRAPHY. (74 C.) In Pl.VIII. K. the elliptical shape of the earth's orbit is given in an exaggerated form, in order to make more apparent the way in which the unequal duration of the seasons results from it. (74 D.) Remark, in this diagram : First, the two points of the earth's orbit, the most distant from each other, are, not the summer and winter solstitial points, B and E, but the greatest length of the ellipse is between the points A and D (sec. 599). Secondly, the earth, at our (N. hem.) winter solstice, is much nearer the sun than at our (N. hem.) summer solstice. Thirdly, the two lines, B E and C F, drawn through the sun's center and the solstitial points, and through the sun's center and the equinoctial points, divide the earth's elliptical orbit into four unequal parts. The earth, during our northern winter, passes from B to F-, during the spring, from F to Fduring the summer, from F to C; and during the autumn, from G to B again. It is plain therefore that it must traverse a greater distance, during the spring, and par¬ ticularly during the summer, than during the autumn, and the still shorter winter. (74 E.) The inequality In the duration of seasons is augmented by another circumstance. The earth moves, with increased velocity, along those parts of the orbit which are nearest the sun (because it is there more exposed to the sun's attracting power), and relaxes its speed in proportion to its greater distance. Hence, during the spring and summer of N. hemisphere, its velocity is less than during the autumn and winter. The long spring and summer are thus made longer by the diminished velocity of our planet, while the increasing speed with which it passes through the rest of the ellipse, makes the short autumn and winter still shorter. This cause and effect are reversed in the S. hemisphere, where, as we have already seen, the seasons are reversed. Instead of having a long spring and a SEASONS. 33 still longer summer — a short autumn, and a still shorter winter, it has a long winter, which corresponds in length to our summer; and a short summer which corresponds to our winter — an autumn corresponding in length to our spring; and a spring, to our autumn. (74 F.) The diagram shows the earth to be nearer the sun in winter than in summer. Our winter is never¬ theless cold from the fact that the N. hemisphere is so far turned away from the sun as to receive its rays obliquely; but the S. hemisphere has its summer just at the point where the earth is nearest the sun; so that the intensity of the heat, in summer, is greater than in winter, from two causes: 1. It receives the sun's rays more vertically. 2. It is nearer the sun than at any other period*. (74 G.) The same causes, reversed, increase the intensity of the S. hem. winter, which takes place at our ■summer solstice, when the earth is farthest from the sun. The S. hem., then, receives the sun's rays, not only obliquely, but from a greater distance. And, as the earth, at that period, moves more slowly, the S. hem. winter is so much the longer. The intensity of the winter, however, is counterbalanced by that of the summer. The same, inversely, in the N. hem.; so that the mean annual temperature is equal N. and S. of equator. (600.) (74 H.) * The earth is about 3 million miles nearer the sun, in our (N. hem.) winter, than in our summer. The former season ought, consequently, to he the hotter. But, remark, two circum¬ stances neutralize the effect of this proximity. 1. It occurs at the period when the N. hem. leans the farthest away from the sun. 2. Much heat is lost by the greater velocity with which our planet moves through that part of its orbit. In the S. hem., just the contrary. There, it is hotter, the nearer the earth is to the sun. In other words, the whole earth is hotter at the period of our midwinter, than it would be, if the sun were in the center of a circle. The summer of the S. hem. is hotter than it would then be; and the winter of the N. hem. is hotter than it would then be. 3 34 ASTRONOMICAL GEOGRAPHY. (74 K.) Remark. In reading sec. 74, and, indeed, all the astronomical sections, the student of N. America, Europe, etc., must be careful continually to remember that he inhabits the northern hemisphere. (75.) Earth and its orbit seen partly from above. — Let us now pass to D. We are here supposed- to stand, neither at a point directly above the plane of the ecliptic, where the earth's orbit would appear a circle, nor in the plane of the ecliptic, where the orbit must appear a line; but about hcdf way between those two points, where the orbit appears, neither a line, nor a circle, but an oval, because the circle is fore-shortened* (as in the cart-wheel PI. VIII. L. Fig. b). We will now reconsider (PI. I. D) the earth's annual movement, beginning at the summer solstice. The ten phenomena are here, in the N. hem., still more visible. As we have taken a position somewhat over the N. hem., the S. Pole is, of course, invisible. Read again the ten phenomena of 23. June (66). By examining the earth (PI. I. D. fig. 1) you will better understand the causes of these phenomena. You see how the N. hem. here leans toward the sun; why, within the arctic circle, there can he no night; why the N. hem. has now its summer and its longest day, etc. The whole arctic circle here lies in the sunshine 24 h., that is, during the whole diurnal revolution; because the whole arctic circle is turned toward the sun. It takes the earth three months to come round to the autumnal equinox (fig. 2), where just one half of the arctic circle lies in the shadow. Day and night must, consequently, be there equal. Three months later, at the winter solstice (fig. 3), the whole arctic circle, for 24 h., lies in the shadow. The daily revolution brings no part of this space into the sun's light. At the vernal equinox (fig. 4), one half the arctic circle * FORE-SHORTENED ¡ — represented as it would appear to the eye when seen obliquely. SEASONS. 35 is again in the light, and one half is in the shadow; giving thus, at the pole, and everywhere else, on that day, perfect equality of day and night. As the earth passes, from the vernal equinox, to the summer solstice again, equality of day and night begins immediately to disappear. With every revolution, the day, in our N. hem., becomes longer, the night shorter, the season more advanced, till we reach that point again (fig. 1), where the N. Pole is turned as far toward the sun as the earth's position will ever permit. We no sooner reach the longest day (fig. 1), than the movement of the ever advancing earth begins to change our condi¬ tion again. The days begin to shorten. Remark, how¬ ever, the next section. (76.) Sun stands still. — At two points of the year—midsummer and midwinter — the sun is said to stand still, because, for a short period, the days have scarcely any perceptible increase or decrease. You have already learned, first, that the sun is stationary in the center of the solar system, and that the planets roll around him; secondly, that, to the inhabitants of the earth, our planet does not seem to move at all, but to be a fixed point, while the entire heavens seem to move around it, once every 24 hours. In addition, the sun, and the whole starry sphere, seem to float slowly around the earth once in about 365 days. When astronomers say the sun stands still, they, of course, speak only of this last apparent annual movement around the earth, which is nothing more than a reflection of the earth's annual movement around the sun. Thus the term "the sun stands still" means only "the earth stands still". But does the earth stand still? Certainly not. Yet, at the two solstitial points (keep your eyes on fig. 1 D), the days remain, during several diurnal revolutions, almost exactly of the same length. This results from the fact that the inclination of the earth's axis, and the elliptical form of its orbit, are such, that the path of the sun, instead of being, as usual, N. or 3* 36 ASTRONOMICAL GEOGRAPHY. S., appears parallel to the equator, E. and W. He ^oes, for a time, neither N. nor S., hut lingers (C) in •tropic of Cancer. The days remain, therefore, of about the same length. Hence has arisen the -word solstice; and the term, the "sun stands still". (7 6 A.) JRemark. I, We abstain from many expla¬ nations indispensable to more advanced students—par- ticulary students of astronomy — hut which would be out of place in these lessons. When we say, for instance, the sun is stationary in the center of the solar system, we mean relatively. He is not, strictly speaking, in the center; neither is he stationary. He not only revolves on his axis, hut he moves, in a kind of orbit, around his central point. In addition, like the rest of the fixed stars, he and his family of worlds, are sweeping forward, probably in an unimaginable circle or ellipse, around an unknown center. (^76B.) 2. The ellipticity of the earth's orbit, in PI. I. D, is not intended to show the real form of the orbit. It results merely from the circle being held up to the eye obliquely. The real ellipticity (22) is too slight to be represented on any sheet, as other than a circle. But, although exaggerated, the elliptical form in D, illustrates correctly one of the reasons why, at this point of the orbit, the sun, for several days, scarcely changes his direction. (77.) Four circles. — Eemark. In the 8 pictures (PL I), from E to M, the earth is drawn at its summer solstice (23. June). In E, F, G, H, your eye is sup¬ posed to he in the plane of its orbit and you see four different points of the diurnal revolution, by which New York passes through the 24 hours. In I, you are exactly over the N. Pole. You see the six months day of the arctic circle (midsummer of N. hem.). In K, you are exactly over the S. Pole, with the N. Star CIRCLES. 3i7 on the opposite side of the earth. You there see the six months night of the antarctic circle (midwinter of S. hem.). Figs. B, C, D, will enable you to understand' the four circles are drawn where they are. If the axis of the earth were perpendicular to the ecliptic, there would be no change of seasons; and the length of day and night would be always equal. There would be no regularly defined zones and no reason for the arctic or tropical circles. It is the inclination of the axis which brings the earth into the different positions seen in PI. I figures C and D. Remark. Most of the figures on PI. I ought to be consulted during the examination of the circles, hut particularly B, C, D. (78.) Arctic Circle. — In this position (B), the shadow has receded from the N. Pole as far as it ever can. There is thus, around the pole, a circular space, out of the earth's shadow and in the sun's light during one diurnal rotation. The arctic circle describes the limits of this space. Its entire circumference can be seen on D, I, and L. (79.) Antarctic Circle. — A similar space around^ the S. Pole (B), is described by the antarctic circle; and the same conditions are, at the same moment, repeated there, except inversely. While the arctic circle remains in the sunshine, independent of the earth's revolution, the antarctic circle remains in the shadow. (C. fig. 1 K and M.) The regions within the arctic and antarctic circles are the only parts of the globe's surface where the sun ever remains 24 hours either above or below the horizon. And, remember, that, while, on the circle itself, the day, or the night, is never longer than 24 hours, it lengthens, as we advance from the circle to the pole, until, at the point of the pole itself, it has a duration of six months. Now what is the distinguishing feature of the arctic and 38 ASTRONOMICAL GEOGRAPHY. antarctic circles? And what are the conditions, there, of day and night*? (80.) Tropic of Cancer. — If the earth's axis were perpendicular to the ecliptic, the sun's center would always be vertical over the equator; but, as the axis leans 23® 27' 26", from a perpendicular, toward the ecliptic — that depresses the equator 23® 27' 26" below the ecliptic and brings a corresponding point of the earth 23® 27' 26" N. of the equator (21. June), under the perpendicular rays of the sun. A circle, supposed to be drawn at this point around the earth, is called the tropic of Cancer. This can best be seen in C. The sun is never vertical over any point of the earth N. of this tropic-, and that is why the circle is drawn just there. When the N. hem. turns so far toward the sun that his center is vertical over this point, he seems to turn and go back again. Hence the word tropic (from a Greek word, to twni). What is the distinguishing feature of the tropic of Cancer? (81.) Tropic of Capricorn. — The tropic of Capricorn marks (PI. I. C. fig. I) in the S. hem., the same phenomena, at the opposite period of the year. Fig. 3. shows the earth at our northern winter solstice. Instead of the N. hem., the S. hem. is turned, toward the sun, as far as it ever can be — far enough to bring the sun vertical over the tropic of Capricorn. His ray& are never vertical over any point S. of this tropic. Hence the space, between these two tropics, is the only space on the surface of the globe which ever receives the vertical rays of the sun. Name the distin¬ guishing feature of tropic of Capricorn. (82.) Sun's apparent semi-annual movement N. and S. between the tropics. — Look at the * The teacher is here again reminded to put such questions, where not found in the text. CIRCLES. 39 summer solstice (PL I. C). There the sun is in the zenith of the people on tropic of Cancer. In our autumnal equinox (fig. 2), his center is vertical* over the equator. At our winter solstice (fig. 3), his center is vertical over the tropic of Capricorn. At our vernal equinox (fig. 4) it is over the equator once more. At our summer solstice, it is directly over the tropic of Cancer again. Thus, to the people of the earth, the sun seems to come into the northern heavens as far as tropic of Cancer, then to pass S. as far as tropic of Capricorn, and thus to be, continually and forever, passing vertically over their heads, north and south, between those two circles or tropics, crossing the equator twice a year. (83.) Fonr'seasons at equator. — Take PI. I. C. Suppose yourself on the equator, in that figure of the earth, marked 1 (our summer solstice). We have here one of the equatorial winters. For, in this zone, there are two winters and two summers every year. The sun's center is as far away from the equator, on the N., as it ever can he. The tropic of Cancer marks the limit. The sun will now begin to turn back toward the equator. In three months, his center will be exactly over the equator (2). That is one of the equatorial midsummers. From figs. 2 to 3, he will, after having crossed the equator, be passing S. of it. At 3, his center will be vertical, as far S. as it ever can be, on tropic of Capricorn. The equator, now, has its second annual winter. At 4, invisible in the Plate (supposed to be on the opposite side of the sun), the equator has its second midsummer. At fig. 1, the sun has withdrawn as far N. again as tropic of Cancer. The equator has once more its winter. During the successive seasons, as will easily be understood by examining that * VERTICAL — : in the zenith — placed perpendicularly over the head. The sun is vertical to the inhabitants within the tropics at certain times every year. (Webster's Diet.) 40 ASTRONOMICAL GEOGRAPHY. point of the equator intersected by the shadow (fig. 1), day and night are of equal length. Remark, also, the two midsummers, at equator, correspond to our two equinoctial points — while one midwinter corresponds to the northern midsummer; and the other midwinter to the southern midsummer. The seasons of this equatorial region are marked by rain and drought instead of by heat and cold (600 A). (84.) Four seasons at tropic of Cancer. — Suppose yourself (PI. I. C. fig. 1) on tropic of Cancer, in Mexico for instance. It is midsummer, about 23. June. You have, on that day, the burning sun directly over your head. He does not, however, seem to move farther N. He seems to stand still a few days (except, of course, the apparent motion arising from the daily rotation of the earth). He then turns toward the S., rising every morning on a more southern paral¬ lel. The day and night cannot here he equal, as on the equator. The day is about 14 hours; the night, about 10. As the earth moves around to fig. 2, the day and night are equal again; because the sun has moved 8. as far as the equator. At fig. 3, the sun rises as far S., as tropic of Capricorn. Your night is now 14 hours long, your day, only 10. (85.) Four seasons at arctic circle. — Place yourself at Behring Strait, on the arctic circle (PI. I. D. fig. 1). Here, about 23. June, you can see the sun all night — that is during the whole diurnal rotation. You have a circle which does not turn away from the sun, at this point of the year, during 24 hours. Each day, however, that circle contracts. You have less sunshine every 24 hours. Thus your days shorten and your nights lengthen. At fig. 2, your day and night are equal. At fig. 3, the season of fig. 1 is exactly reversed. During one diurnal revolution of the globe, you have, here, no view of the sun at all; but the circle of darkness begins to contract, just as the circle ZONES. 41 of light did at 1. Your day lengthens again till, at fig. 4, it is 12 hours, and it continues to lengthen, till, at fig. 1, your night, during a single revolution of the globe, ceases altogether. (86.) Four seasons at North Pole. — Take your stand at the point called the N. Pole (D. 1). You have, here, the sun as high in the heavens as he ever can be. He wheels, or rather seems to wheel, without disappearing at all, in small circles around the N. Star; because the region of the earth, on which you stand, wheels in small circles around the pole, without being withdrawn from his rays. He has been shining, with¬ out interruption, since you left the point 4. He con¬ tinues to shine, till you reach fig. 2 (that is six months) ; but wheels lower and lower toward the horizon till, at 2 (our autumnal equinox), his fiery globe disappears altogether, and you will not see him again for six months. He has passed S. of the equator. He has crossed the equator, and thus sunk beneath your line of vision. He has descended beneath your rational horizon (32). At 3, he is at farthest S. point — the tropic of Capricorn. The night circle around the N. Pole has reached its greatest circumference, because the sun is as far beneath your horizon as he ever can be. We call this circumference the arctíc circle. The day after you leave 3, the shadow begins to contract. It grows smaller and smaller, till, at 4, it recedes from the point of the pole. You then catch, once more, a glimpse of the sun and do not lose sight of him again for six months. (86 A). Remark. The rising of the sun, after his pro¬ longed absence, is a great event to the poor tribes of these dreary regions. The first sign of his gradual reap¬ pearance is hailed with extravagant joy, and his slow approach watched with extraordinary interèst. We may imagine also with what emotions they behold him (PI. I. D. fig. 2) slowly descend, and at last entirely 42 ASTRONOMICAI, GEOGRAPHY. disappear beneath their horizon, for days, weeks, or months (according to their latitude). (87.) Five Zones. — The four circles thus divide the surface of the globe into five regions or zones — the north frigid zone, the north temperate zone, the torrid zone, the south temperate zone and the south frigid zone (PI. VIII. N). Name these 5 zones and describe their limits. (88.) North Frigid Z one. — The phenomena of this zone are (PI. I. D) — : 1. It is a circle, every part of which, at the summer solstice, has the sun above its horizon during one entire revolution of the earth on its axis. 2. At its central point (the pole), the sun does not set for six months. 3. At the intervening points, between the center and the circumference of the circle, the sun remains above the horizon from 6 months to 24 hours, accord¬ ing to the different parallels of latitude. 4. At the winter solstice, the conditions of day and night are (fig. 3) reversed. The whole of its area has the sun beneath its horizon, during one entire revolution of the earth on its axis, and the length of the night increases from 24 hours to 6 months, as you approach from the circumference of the circle to the central point — the pole. Of course the seasons correspond to the conditions of day and night. 5. While the sun's rays are thus withdrawn in the winter, they fall so obliquely on this region, even in the summer, that, except for a very brief period, the heat and vegetation are feeble, and the frigid zone is thus, from intense cold, scarcely inhabitable by human beings. Name distinguishing features of the N. frigid zone. (89.) South Frigid Zone. — The conditions of the N. frigid zone are exactly reproduced, except at opposite points of the year. LENGTH OF DAY AND NIGHT. 43 (90.) Torrid Zone. — 1. Some part of it always has the sun in its zenith (PI. I. C.) 2. Every part of it receives the sun's perpendicular rays twice a year. He seems to come N., till (our summer solstice) his center is in the zenith of places on the tropic of Cancer. île then turns and moves S., (that is, he rises every day at a more southerly point than on the preceding day), until (our winter solstice) his center is in the zenith of places on the tropic of Capricorn, when he turns and begins to go back toward the N. 3. On the equator, and in a zone about 6® on each side of it, the day and the night are always of equal length, namely 12 hours. The winter cold, as in the four other zones, is unknown. 4. The sun never remains above, nor below, the horizon an entire revolution of the earth on its axis. Name distinguishing features of torrid zone. (91.) North Temperate Zone. — 1. It has (unlike the frigid zones), never the sun above, nor below, the horizon during a revolution of the earth. 2. It has (unlike the torrid zone), never the sun's rays vertical over any part. 3. The length of day and night (except at equinoxes) is never equal (as on the equator); but far less unequal tban witbin the polar circles. Name distinguishing features of N. temperate zone. (92.) South Temperate Zone. — The same peculiarities, but at opposite period of the year. June, July, August, are the winter months, while December, January and February are the summer. (93.) Different length of day and night in different zones. — A glance at the figures of the earth on PL I. will show that, on 21. June, the relative length of day and night must be different at every parallel of latitude, from arctic circle to antarctic circle (fig. F). The arctic circle will have the longest day, 44 ASTRONOMICAL GKOGRAPHY. namely 24 hours. The day will be shorter, and the night longer, on places in proportion as they are nearer to the antarctic circle. This condition of coui-se will be exactly reversed at C. 3. Half way between 1 and 3, (that is, at the equinoctial points), the day and the night will be equal in length. At the different points of the earth's orbit, between the summer and winter solstices again, these'conditions will be reversed: and the relative length of day and night will change pre¬ cisely as the earth moves forward from one of these points to the other. From the circumference of the arctic and antarctic circles to their centers (i. e. the poles), the length of the day, according to the parallel of latitude, will vary, from 24 hours to 6 months, with the earth's annual revolution, the phenomena being exactly reversed every six months (601). (94.) Table of different length of day and night — on the 23. June, at different parallels of latitude. On equator, and 6 degrees each side of it, day and night always . . . . 12 hours. On parallel 16® 44' the longest day 13 - 30» 48' 14 - 41® 24' - - - 15 - 49® 2' - - - 16 - 54® 31' . - - 17 - 58® 27' ... 18 - 61® 19' ... 19 - 63® 23' . 20 - 64® 50' . 21 - 65® 48' . 22 - 66® 21' ... 23 - 67® 23' . 1 month 69® 51' ... 2 - 73® 40' ... 3 - 78® 11' . 4 . 84® 5' . 5 . 90® 0' ... 6 LENGTH OF DAY AND NIGHT. 45 You will understand this better by PI, I. fig. F. There the six months day at thé N. Pole, in our mid¬ summer, and the six months night and winter at the S. Pole, in our midsummer, may be comprehended at a glance, with the diíFerent lengths of day, on the different intervening parallels (also W. hem. PI. II.) (95.) Morning —Noon —Afternon —Night, at New York. — By the 8 figures of the earth (PI. I), particularly from E to H, you see how the continents, oceans, etc., are situated, with regard to zones and climates; and how differently they are affected by the motions of the earth, as to the length of day and night, etc. Bear in mind that, in all these figures, the earth is represented at our summer solstice. Describe condition of N. hem. Midsummer and longest day. Describe S. hem. Midwinter and shortest day. At the point called N. Pole. Six months day. At the point called S. Pole. Six months night. "Where is the sun's center? Vertical over tropic of Cancer. Describe condi¬ tion of arctic circle. It has the sun above the horizon 24 hours. Antarctic circle? Sun beneath the horizon 24 hours. As the globe revolves from west to east (E), the point, marked New York, has moved from the shadow into the light. At New York, therefore, in E, it is morning or forenoon. At F, it is noon. In G, New York is on the opposite side of the globe, and moving toward the shadow; it is therefore afternoon. In H, New York has passed into the shadow and nearly out of it again; it is therefore night, but not long before sunrise. When the diurnal movement shall carry New York to the limit of the shadow, the sun will rise. You see here, in H, that the sun rises earlier, at mid¬ summer, to places on the same meridian, in proportion as they lie nearer the N. Pole, till the point of the arctic circle, after which the sun remains above the horizon the whole 24 hours. The sun, in H, is just rising over Hudson Str. which is on the same meridian 46 ASTRONOMICAL GEOGRAPHY. as the Republic of Ecuador (S. America). But the sun will not rise, in the latter place, till 4 hours later. By the table of the different length of day and night (F), we perceive that New York has the sun about 15 hours above the horizon, on our longest summer day; of course, 15 hours beneath our horizon, on the longest winter night. (96.) Why does the N. Pole always point to the North Star? — The attentive student may desire a more particular answer to one question. The earth moves annually in an immense ellipse around the sun and, at midsummer and midwinter (PI. I. C.), occupies two positions about 200 million miles distant from each other. Its axis, at the same time, retains its parallelism — that is (consult PI. VIII. H.) at every point of its orbit, remains parallel to itself at every other point of its orbit. How then can the N. Pole always point to the North Star, during its whole annual revolution around the sun? This phe¬ nomenon results from the stupendous distance of the North Star, which is so amazing that the whole solar system, in comparison, dwindles to a mere needle-point We have already (17 and 19) touched on the subject. In PI. I. B., you observe a small circle, little more than a dot, called orbit of Neptune, drawn in the line between the N. Pole and the North Star. That is in¬ tended to represent the comparatively insignificant space occupied by our solar system among the fixed stars. You must suppose the earth, revolving around the sun, within that little circle; you will not require any farther explanation, why the N. Pole always points to the North Star. RECAPITULATORY QUESTIONS. 47 QUESTIONS UPON THE SEASONS. (97.) There are, as we have seen, four causes which co-operate to produce the seasons actually existing on our planet: 1. The inclination of the earth's axis to the plane of its orbit. 2. The annual movement of the earth around the sun. 3. While moving annually around the sun, the earth remains always in the same plane. 4. The axis retains its parallelism. (97 A.) Repeat the first of these causes. The inclina¬ tion of the earth's axis to the plane of its orbit. How does that cause the seasons? Would there be no seasons, if the earth's axis were not inclined? Would the sun not be there and shine? Would there not be heat and coldt There would he seasons. What would be the condition of the globe, if the earth's axis were not inclined, — that is, if it were, we will say, perpendicular to the plane of its orbit? Take PI. I. C. fig. 1. How would the axis then be situated with regard to the line of the shadow? It would he identical with it. How would the equator lie with regard to the earth's orbit or ecliptic? It would he identical with it. What season would it be in the torrid zone? Midsummer. In the two temperate zones? Neither midsummer nor midwinter, hut between the two — about the same temperature as our spring or autumn. What in the frigid zone? Would it be midwinter or midsummer there? It would he there also a season between the two. We see, therefore, that there would be seasons, but different from our present seasons. As the axis would form a perpetual right angle with the ecliptic, the N. Pole would, of 48 ASTRONOMICAL GEOGRAPHY. course, never be turned toward the sun, as in fig. 1., nor away from it, as in fig. 3. Midsummer and mid¬ winter, therefore, would never exist in the frigid and temperate zones, as they now do; hut there would he an everlasting midsummer in the torrid zone. What would he the condition of the earth with regard to day and night? Day and night would be always equal every¬ where upon the earth's surface. What is it then which causes our actual midsummer and midwinter N. and S. of the tropics? The inclination of the earths axis to the plane of its orbit. We have observed that the prin¬ cipal result of the inclination of the earth's axis, is our present midwinter and midsummer N. and S. of the tropics. What effect does this inclination have upon the torrid zone? At present, the inclination of the axis causes the sun to pass from the tropic of Cancer to the tropic of Capricorn, and then from the tropic of Capricorn to the tropic of Cancer again, once every year; whereas if the axis were perpendicular, the sun would be always in the zenith of the people on the equator. To what extent is the axis inclined? Twenty-three degrees, twenty-seven minutes, twenty-six seconds. What angle (PI. VIII. T. fig. c.) does the axis form with the perpendicular line of shadow? Twenty-three degrees, twenty-seven minutes, twenty-six seconds. What angle does the equator form with the ecliptic? Twenty-three degrees, twenty-seven minutes, twenty-six seconds. You say the axis leans 23" 27' 26", Irom a perpendicular, toward the ecliptic — what angle does that perpendicular form with the ecliptic? An angle of 90'> or a quadrant (see PI. VIII. T. fig. h). Now if the perpendicular line of shadow form an angle of 90® with the ecliptic, state again, what angle the axis forms with the perpendicular? Twenty-three degrees, twenty-seven minutes, twenty-six seconds. Now state, what angle the axis forms with the ecliptic. Of course it will he 90®, less 23® 27' 26"; and as it is a somewhat slow process to deduct 23® 27' 26" from 90®, we will give you the answer—66® 32' 34", Now state what is the angle formed by the axis with the RECAPITULATORY QUESTIONS. 49 ecliptic? Sixty-six degrees, thirty-two minutes, thirty-four seconds. If the axis were itself perpendicular to the ecliptic, it would form a right angle — that is, an angle of 90®. As it leans 23® 27' 26", from a perpendicular, toward the ecliptic, of course its angle with the ecliptic will be 23® 27' 26" less than 90®*. Now supposing the axis to be always perpendicular to the ecliptic, how would the seasons be influenced by the annual revo¬ lution of the earth around the sun? Not at all. There would be no succession of seasons. There would he no variety. But would there not be one slight change of temperature? (see note, 74H). There would, as the earth is, at one point of the year, 3 million miles nearer the sun than at the opposite point, the temperature would slightly rise everywhere on the earth's surface at one period of the year. The inclination of the earth's axis, there¬ fore, explains why, in fig. 1. of C., it is summer in the N. hem. and winter in the S. hem. (97 B.) But another cause is required to explain the succession of the seasons. For if the earth remain stationary, as at fig. 1, the seasons would remain stationary also. If the sun revolved around the earth, in the plane of the ecliptic, as Ptolemy taught, there would, indeed, he a succession of seasons. But the evidences of the fixity of the sun, as the center of the solar system, are too overwhelming to he doubted; the annual movement of the earth is de¬ monstrated by unanswerable arguments. We may, therefore, take the earth's annual movement as a second cause. (9.7C.) Suppose the earth, while moving annually around the sun, were frequently to rise above the plane of its orbit; and, again, to sink beneath it, without * The teacher will perceive that these are premeditated repetitions. 4 50 ASTRONOMICAL GEOGRAPHY. keeping in an unchanged level — what would be the effect of that on our seasons? A proportionate irregu¬ larity of the seasons. Yes, if our planet were to sink below the sun, we should have the sun of course above the N. Pole — tropical heat in the arctic circle — ice and snow on the equator—in the antarctic circle, an increased intensity of cold and darkness. What, there¬ fore, is the third cause of the regularity with which the seasons follow each other? The earth always moves in the same plane. Yes, the earth's center never rises above, nor falls below, that line (PI. I. C) representing the ecliptic. (97 D.) Lastly. Suppose the earth's axis should sway backward and forward, like the masts of a rolling ship at sea — what would be the effect of that on our seasons? The effect would be, an irregularity, similar to that which would result, if the planet were to pass above or beneath the plane of the ecliptic. The seasons would fluctuate in proportion to the vacillation of the axis. The N. Pole would sometimes hend down toward the ecliptic, presenting the N. hem. more broadly to the sun; sometimes it would turn away from the sun, into far more intense cold and darkness than our polar re¬ gions have ever experienced. Equatorial heat and polar cold would suddenly displace each other, according as the huge globe reeled to and fro. God has ordained it otherwise. He who "hath meted out heaven with the span", hath said: "While the earth remaineth, seed¬ time and harvest, and cold and heat, and summer and winter, and day and night, shall not cease'\ Not only the axis is inclined so many degrees, mirrutes and seconds, to the plane of the orbit, but, during its entire annual journey around the sun, it keeps invariably its axis at the same angle with that plane. How do you describe this circumstance, in other words. The earth's axis always retains its parallelism (as in PI. VHI. H). What do you mean by the axis retaining its parallelism? I CONCLUDING REMARKS. 51 mean that the axis, at every point of its orbit, remains parallel to itself, at every other point of its orbit. Now name the four circumstances which explain the seasons, and the regularity with which they succeed each other (section 97). (98.) Parallelism of the earth's axis. — This term, like many others, must not be taken without a reserve. There is, in fact, a perpetual departure from absolute parallelism, although too inconceivably minute to be perceptible to us, and therefore (at least for thousands of years) not affecting any thing said with regard to our seasons. As the earth revolves, it continually performs a gyratory motion, in the manner of a spinning top, or te-to-tum, so that, like the extremity of the axes of those two toys, the N. pole is always describing a circle. The circle, which the N. pole of the earth thus describes, in the heavens, reaches from our present N. star to the star Vega (in Lyra) (PI. I. B). But a period of 25,868 years is required for each one of these gyra¬ tory movements (which the te-to-tum makes in a second). Thus, in 12,000 years, our N. pole will point to Vega; in about twice that time, it will come back to our present N. star again. The S. pole, of course, describes a corresponding circle in the southern heavens. This period is called the platonic or great yeat*. (98 A.) Remark. To the questions, how this "swaying backward and forward of the earth's axis" (97 D), during the platonic year, would affect our existing seasons; and how a change in the latter could be reconciled with the scripture-passages quoted in 97D, we answer: first, this sketch is confined to points required by the student of Geography. For such as desire to study Astronomy, the writer has prepared a * It has been suggested that the platonic year may be re¬ ferred to, in some Bible-passages, which man has generally interpreted Ao mean our solar year. 4* 52 ASTRONOMICAL GEOGRAPHY. third volume (6), entitled: Great Outline of Astronomy, treating that science, in a simple form, intelligible to all who read in connection with its accompanying plates. Some remarks will there be found upon the platonic year, the precession of the equinoxes, and the we- period (138). Secondly, the fair-minded, christian student may continue his studies, with the perfect assurance (whatever a certain class of philosophers declare to the contrary) that, the more clearly the outline oj Nature and Science is understood; and the more clearly the outline of Scripture-Revelation is understood, the more they will be found in harmony with each other.* (98B.) Fixed stars not fixed. — The constel¬ lations, from time immemorial, have remained in the same relative positions, so that the orbs composing them may well be called "fixed stars". But they are fixed only in appearance. There is reason to believe that, with oar sun (76 A), they are all pursuing their eternid courses, around a mysterious center, with a velocity which, however great, is imperceptible from the fact that their remoteness is too amazing for the human intellect. During the next, let us say, million years, the groups, called constellations, will be dissolved. The seven stars in the Great Bear, for instance — those in Taurus, with Hyades and Pleiades — Aldebaran, Al¬ cyone, Sirius, Arcturus, Betelgeux, and the rest, will recede from their present places, and move far off into distant and opposite points of. space. The sky will then present new combinations of stars — the "bands of Orion" will be "loosened", by the same Almighty hand which brought the orbs of those clusters into their present juxta-position. But they will, doubtless, during subsequent centuries, re-appear in their former stations; for the universe is obviously » machine (as much so as a clock), framed by a Supreme Intelligence, outside of, and above it; and performing * Frederick de Rougemont of Neufchatel. » CONCLUDING REMARKS. 53 its movements on a scale so stupendous, that the time, since the human race first appeared on the earth, is too short to afford more than some faint indications. It is the work of a divine artist. "Thus the heavens and the earth were finished and all the host of them". They may be likened to a wonderful temple, whose godlike beauty, by the researches of science, is, in some degree, slowly breaking upon the human mind. "We may reasonably conclude that this resplendent and majestic structure is not without a beneficent, eternal purpose; corresponding to the stupendousness of its dimensions — to the harmonious grandeur of its archi¬ tectural form — to the prodigious scale of its periods — to tke series of ascending changes by which the earth has reached its present state — to the nature of man, capable of happiness and able to discriminate between right and wrong — to the exultant representations of the prophets — to the hints of the new heaven and the new earth, so frequent in the Bible — and to the revealed character of that infinite, omnipotent, incomprehensible Being who, in creating the universe, conceived, and is still executing, a plan of love, worthy of Himself. "The heavens declare the glory of God; and the firmament sheweth his handy- work. Day unto day uttereth speech, and night unto night sheweth knowledge". — "Lift up your eyes on high, and behold who hath created these things, that bringeth out their host by number: he calleth thèm all by names by the greatness of his might, for that he is strong in power; not one faileth". (98 C.) To the teacher. — Many intelligent pupils will fail to acquire a clear knowledge, from one reading of the previous pages. The - lessons are prepared to be best understood during a second reading. The brevity of the text-book, and the circumstance that no study is required, except the recitation, render it quite practicable to give it several complete readings, without devoting as much time as is usually accorded to other text-books. PART IL PHYSICAL OR NATURAL GEOGRAPHY. NINETEEN LAND AND WATER DIVISIONS OP THE GLOBE. (99.) Prefatory Observations. — By the aid of figures A, B, C, D (PI. I), we have endeavored to acquire some idea of astronomical geography. The rest of the pictures bring us nearer to the earth, and enable us to examine several striking objects upon its surface. We here commence the study of physical or natural geography. The 8 circular views of the earth are called Planispheres, because each one represents a sphere upon a flat surface or a plane. They are also called Hemispheres. western hemisphere. fig. E. — N. Pole is at top; S. Pole, at bottom; equator, equi-distant between them. Your eye is here supposed to be in the plane of the equator. eastern hemisphere. fig. G. — Poles and equa¬ tor seen from same stand-point, as in previous fig. (E), but the earth has here made a half revolution. northern hemisphere. fig. I. — Here wc haVC changed our position. We are over the N. Pole. Hence we look down on that half of our planet N. of equator. NINETEEN LAND AND W ATER Dl VISION S. 55 The equator, therefore, forms the circumference of our circular view — N. Pole, its center. As the earth re¬ volves, the point, called N. Pole, will remain stationary and the objects of N. hem. will move around in circles, without disappearing. SOUTHERN HEMISPHERE. FIS. K. — Same Con¬ ditions as in fig. I, except that, instead of being over North Pole, we have moved around to a point exactly over South Pole. We are looking down upon that half of the globe, south of equator. The equator is the cir¬ cumference of our circular view — S. Pole, its center. With earth's revolution, the objects will move in circles around the point called S. Pole. Remark, we were supposed to look down upon the earth, in fig. I. But, opposite South Pole (K), should we not look up at the earth? How can we look doum upon it? Because, when we break away from our childish ideas of up and doim, we discover that, in reality, there is no such thing except relatively. Down is toward the center of the earth; up, away from the center. We look equally down, toward the earth, when our Light-Car is over N. Pole — over S. Pole—over equator—over either tropic — or over any other point of the globe's surface. LAND HEMISPHERE. FIG. L. — That side of globe which contains greatest mass of land. WATER HEMISPHERE. FIG. M. — Greatest mass of water. PACIFIC HEMISPHERE. FIG. F. — Best general view of Pacific. ATLANTIC HEMISPHERE. FIG. H. — Complete vicw of Atlantic. Now consider these figures more particularly. (100.) Western—Eastern Hemispheres. — Let us suppose ourselves in our Light-Car, sailing through free space, and sufficiently near the earth to distinguish oceans, continents, etc.; with power to go where we like — to stop and remain stationary when we like — to pass above, around, below the earth, in every 56 physical geography. direction, and to view it on all sides. We move to that point of space where we behold the earth, as in fig. E (PI. I). It presents the western hemisphere. Now we move to another side of the globe (G), exactly opposite Western Hemisphere. There, we view eastern hemisphere. These two hemispheres, together, show every part of the earth's surface. (101.) Three Continents and Antarctic Re> gion (often called a continent). — Many geographers count four continents, viz. in W. hemisphere (E), the immense broken fragment, extending nearly from N. pole to S. pole: america, western continent or new world; in E. hemisphere (G), the principal land- mass: eastern continent or old world; the small¬ er portion of land, S. E. of E. Continent (sometimes called an island, but, compared with islands, having more the proportions of a continent): Australia. The unexplored land and ice around S. pole (K), although little known, is usually termed antarctic continent. Point out and name four continents. What is a con¬ tinent? (Read 121.) (101 A.) Eemark. Region called Antarctic Continent. — It has been supposed that the area (ay'-re-ah) within antarctic circle is occupied by a continent, nearly 3000 m. long and 2000 m. broad — without the least vegetation — buried under everlasting snows — untrod¬ den by human feet — gigantic volcanoes, one of which, Erebus, 12,367 f. high, when first discovered, was in full eruption and is believed to be in constant activity — land, in the interior, seemed to reach an elevation of 3000 f. — broken coasts, consisting of ice-precipices, sometimes 200 f. high. From the remarkable shallow¬ ness of the waters near the shore, some infer a land- mass— climate 10 degrees colder than in correspond¬ ing northern latitudes (74 G.) — wind and seas more boisterous — limit of drifting ice (PI. II.) extends al¬ most to Cape Horn, La Plata Bay, and C. of Good nineteen land and water divisions. 57 Hope; many degrees nearer the equator than is the case in northern hem. For supposed form of the coasts, consult PI. II. and PI. I. K and M. (101B.) Remark. Until its incorrectness be demon¬ strated (de-mon'-strat-ed), we retain the name continent, to indicate this mass of land and ice, yet (the student must carefully bear in mind) there is no proof that it really is (any more than that it really is noí) one solid body of land, or even large islands, or island-chains, or groups. A continuous coast has not been discovered; and no exploration of the interior effected. Some of the land, reported by "Wilkes (A. D. 1839), has since been freely traversed by Ross, in the ships Erebus and Terror. Several eminent authorities incline to the idea of a few islands, locked together by a frozen ocean. (102.) Subdivisions of Continents. — The w. continent (E) is Subdivided into north America and south america; e. continent (G), intO europe, asia and africa. (103.) Remark. The ural mountains form part of the boundary between Europe and Asia. (103 A.) Geographers sometimes consider the world in eight divisions: — n. america —s. america-europe— asia — africa — australia—antarctic continent or region—oceania — the latter subdivided (PI. I. G and F) into three island-groups: — Malaysia—Austral¬ asia (including Australia)—Polynesia. (104.) Oceania — the great island-world (F and G) — consists of an immense number of islands extending north, east and south of Australia, between W. and E. Continents, over nearly whole Pacific. PI. II. gives a view of Oceania, on a larger scale, with its three subdivisions. You may here also consult PI. IV. (105.) Six Oceans. — Seen from some points (PI. I. K. M), the planet we inhabit appears a vast 58 PHYSICAL GEOGRAPHY. water-globe. One universal ocean covers about two- thirds of its surface. Several large, broken landmasses, and a great number of islands, are distributed in it and divide it into diiferent parts, bearing different names, as if different oceans, namely: pacific ocean (fig. F) ATLANTIC OCEAN (fig. H)—INDIAN OCEAN (fig. G) — GREAT SOUTHERN OCEAN (fig. K) — ARCTIC OCEAN (fig. L) — ANTARCTIC OCEAN (fig. K). Point out Pacific on all the planispheres. Now Atlantic. Indian Ocean. Great Southern Ocean. Arctic Ocean. Ant¬ arctic Ocean. How many oceans are there? Six. Name them. What is an ocean? (Read 153). (106.) Great Sonthern Ocean. — Point out Southern Ocean on figures of PI. I. — Some geogra¬ phers have considered the Pacific, Atlantic and Indian Oceans to extend down to antarctic circle (F, G, H, K), and given the names. Southern Pacific, Southern Atlantic, etc., to those portions reaching below C. Horn (S. America), C. of Good Hope (Africa) and Australia. Others have made the Antarctic Ocean reach up to C. Horn, C. of Good Hope and the whole S. coast of Australia. Point out these? In 1845, the Geographical Society of London recommended that the southern limits of the Pacific, Atlantic and Indian Oceans, should be the antarctic circle (E, F, G, K, M). This recommendation has not been generally adopted. The navigator, in the neighborhood of the antarctic circle, does not enter upon his log-book (sea-journal) what ocean he is in, but only his latitude and longitude; for what ocean is he in, on the meridian of C. Horn and antarctic coast? In order more clearly to define an area of the great universal ocean, distinguished from the rest by a peculiarity, as striking as any marking the different zones, we shall, as some others have done, give the name of Great Southern Ocean to all that water which (K) lies N. of antarctic circle, and S. of a line drawn from C. Horn to C. of Good Hope, thence to S. point of Australia round to G. Horn again. In N. NINETEEN LAND AND WATER DIVISIONS. 59 hem. (I), it is not possible for a ship to sail in one continued circle, due E. or W., around the earth; be¬ cause its course would be interrupted by land, (except, possibly, a small, unexplored area encircling the N. Pole (I. L), supposed by many to be blocked up with eternal ice); but, in the Southern Ocean (K), a ship might sail, due E. or W., in a circle, around the globe, and come back, without interruption from land, to the point whence it started. Remark. The words, "Great Southern Ocean", on the planispheres of the earth (PI. I), have the appear¬ ance of being placed on the map negligently. The shape of the ocean, however, requires that they should be so inscribed, in order to show the very irregular northern limits: for instance (fig. H), from C. Horn to C. of Good Hope (also PI. IV). (107.) Continents and Oceans in one unbroken outline. — Take PI. IV. — a different kind of map, called Mercator's Projection (Mer-ca'-tor) — more partic¬ ularly explained hereafter (442). The advantage of it is that we have, at a glance, all the different continents and oceans — an unbroken view of Great Southern Ocean, bounded on the N. (106) by a line reaching from C. Horn to C. of Good Hope, thence, touching southern point of Australia, to C. Horn again — and the entire limits of Oceania. The antarctic circle, forming the southern limit of the map, cuts off the Antarctic Ocean and part of the so called Antarctic Continent. How many objects have we indicated on the surface of the earth? Nineteen. How many continents? Four. How many subdivisions of continents? Five. What others? Oceania (with its three subdivisions) and six oceans. Name, and point out, on Plates I and IV, each of these 19 objects. (108.) Nineteen chief objects on the globe's surface. — 1. AMERICA, WESTERN CONTINENT Or NEW WORLD; 60 physical geography. — 2. EASTERN CONTINENT Or OLD WORLD; 3, AUSTRALIA; — 4. ANTARCTIC CONTINENT OR REGION; 5. NORTH AMERICA;— 6. SOUTH AMERICA;— 7. EUROPE;—8. ASIA; 9. AFRICA; 10. oceania, divided into—11. Malaysia, 12. australasia (including Australia), and 13. Poly¬ nesia; — 14. PACIFIC OCEAN;—15. ATLANTIC OCEAN; — 16. INDIAN OCEAN; 17. SOUTHERN OCEAN; 18. ARCTIC OCEAN; —19. ANTARCTIC OCEAN. (108 A.) Remark. You will more easily repeat and retain these 19 objects, by always dividing them (in your own mind) as follows ; — four continents — five subdivisions of continents (that makes nine) — Oceania, with its three chief subdivisions (make thirteen) and six oceans (make nineteen). These to be repeated several times. (109.) Light -Car in plane of equator, over W. Hemisphere. — Let us now, in our imaginary Light-Car (100), move around the earth, in every direction, as we have seen a swallow fly over and around a great church; only with this difference^our Light-Car will take us, so to speak, under, as well as over. We bring our Car to a stop, and remain station¬ ary, opposite fig. E, over that point where equator is intersected by the middle meridian. What hemisphere? AMERICA, WESTERN CONTINENT OR NEW WORLD. Name nineteen chief objects (108). Which objects are here visible, partly or wholly? — America, western con¬ tinent or new world — n. america — s. america — SMALL POINT OF ASIA ATLANTIC PACIFIC, WITH OCEANIA — ARCTIC AND ANTARCTIC OCEANS. Which part of Oceania (F)? Polynesia and Australasia. Name those of the nineteen objects not visible in E. Where are they? Opposite side of the globe. In which figure? In ßg. G. nineteen land and water divisions. 61 Remark. There are three oceans and one continent, namely: Arctic, Antarctic and Southern Oceans, and Antarctic Continent: which, encircling the North or South Pole, extend quite around the globe. We will not name those four objects in replying to the follow¬ ing questions of sect. 109. What lies E. of America? Atlantic. E. of Atlantic. europe and africa. E. of Europc and Africa? asia and indian ocean. E. of Asia and Indian Ocean? pacific with Oceania, divided into Malaysia, australasia (including Australia), and Polynesia. E. of Pacific? america. Now go eastward around the earth, from America, and name those objects. Now go westward around the earth, from America, and name those same objects. America — pacific with etc. —ASIA AND INDIAN OCEAN EUROPE— AFRICA — atlantic — america again. Repeat these backward and forward, a number of times. Point out circles on fig. E. Which of the nineteen objects lie within arctic circle? — Between arctic circle and tropic of Cancer? — Between two tropics? — Between tropic of Capricorn and antarctic circle?—Within antarctic circle? (110.) Light-C ar over Pacific Hemisphere (F). — Remember, we keep our Light-Car stationary, at the point selected (109), over fig. E. We remain stationary, but tbe earth slowly revolves, from W. to E.; so that, in a few hours, we should have, beneath ns, fig. F, and we should be in the zenith of that point, where the equator intersects the middle meridian. What hemisphere? Why so called? Name again nineteen ob¬ jects. Which are here visible, wholly or in part? AMERICA, W. CONTINENT Or NEW WORLD — EASTERN continent or old world — australia antarctic continent — n. america — s. america — asia — oceania, divided into Malaysia, Australasia (in¬ cluding australia), and Polynesia — pacific — atlantic (a very small part) — southern ocean — antarctic — arctic. Name those of the nineteen ob- 62 physical geography. jects not visible here. Point out circles. What objects lie within antarctic circle? — Between arctic circle and tropic of Cancer? — Within the tropics? — Between tropic of Capricorn and antarctic circle? — Within ant¬ arctic circle? (111.) Light-Car over Eastern Hemisphere (G). — Name nineteen objects. Name those visible, wholly or in part, in E. hemisphere, eastern con¬ tinent or old world — australia — antarctic continent— europe— asia — africa — oceania, divided into Malaysia, Australasia (includingAustralia), and polynesia — pacific — atlantic indian ocean great southern ocean — arctic and antarctic oceans. Which of the nineteen objects are wholly, or in part, on opposite side of G? Describe their positions with regard to the circles. (112.) Light-Car over Atlantic Hemisphere (H). — Name nineteen objects. Name those visible in H. america, w. continent or new world — e. continent or old world — antarctic conti¬ nent — n. america — s. america — europe — asia — africa —pacific — atlantic — indian ocean — southern ocean — arctic and antarctic oceans. Describe positions of these objects with regard to the circles. (113.) ^ Light-Car over Northern Hemisphere. (fig. I). — If we remain in the position thus selected (109) — that is in plane of equator — the earth would continue to revolve beneath us, and the four hemispheres E, F, G, H, would follow each other in a perpetual succession; but we should never, at one glance, obtain a complete view, either bf N. or S. hem¬ isphere. In order to do this — (we will first seek to obtain a complete view of tbe N. hemisphere)—we must move our Light-Car to a quite different point of nineteen land and water divisions. 63 spacp, and greatly change our position with regard to the earth. We must quit plane of equator, where it appears a line, go N., and arrest our Car at a point, just one quarter way around the globe, where we shall have the arctic circle fully in front of us — and where the equator will, of course, appear a circle. We will direct our Light-Car, first, to a point above the N. Pole. Over which figure are we now? Fig. I. Where is the N. Star? In our zenith. The S. Pole? Beneath our feet., on opposite side of globe. Where must our Light-Car stand, in B, to afiord the view of the earth in fig. I? It must stand at the point marked by the letter W, on the line between N. Pole and N. Star. Name objects, visible wholly or in part in fig. 1. Begin at America and go eastward, america — Atlantic — europe — africa-asia — indian ocean - pacific 0 c K A NIA. What parts of Oceania (F)? parts of malaysia and polynesia. Name Same objects going westward. Point out N. Pole — arctic circle — tropic of Cancer — equator — tropic of Capricorn. Where is tropic of Capricorn? On the other side of the globe, exactly opposite tropic of Cancer. Where is antarctic circle? What other objects lie on opposite side of globe (K)? What four objects in fig. I. appear entirely? What part of the earth, in fig. E, is visible in I? All that part N. of equator. Point out the objects visible, both in E and I? What part of the earth, in each of the other figures, is visible in I? All those parts N. of equator. Point out the objects, in F, also visible in I? The objects in G? in H? in M? in L? in K? Why are none of the objects, in K, visible in I? Because 1 presents only the objects North of equator and K presents only the objects South of equator. Point out those objects, in E, which are also visible in K. Now those objects, in F; in 6; in H; in M; in L. Say what parts, of each of the other figures, are visible in K? Only those parts south of equator. Why are none of the objects in K visible in I? Because K presents only that portion of the earth, south of equator. Which €4 physical geography. ■way does the earth revolve? From W. to E. In what direction would America move in fig. I? Toward top or bottom of the map? Toward top of the map and so around. Yes, it would go in a direction contrary to that in which the hands of a clock move. All the objects would move, in that direction, around the N. Pole, in circles, more or less large, according to their distance. If our Light-Car remain always stationary, in its present point, should we see any other hemi¬ sphere? No. Suppose we desire to examine the S. hem., as we have now examined the N. hem., where must we go? We must move just half way around the globe, to a point of space, on the other side of S. hem. —exactly corresponding to that which, in fig. I, we occupy over N. hemisphere. (114.) Light-Car over Southern Hemisphere (K). — Where is N. Star in K? — On opposite side of heavens, over N. Pole. Where should we stand, in B, in order to see the earth as in K? At point marked by letter Z. Point out S. Pole and circles. Name ob¬ jects visible, wholly or in part. Begin with America and go east. —s. america — Atlantic — afeica — indian ocean — pacific with oceania. Which subdivisions of Oceania (F)? australasia (including Australia) — parts of Malaysia and Polynesia.— Which way do objects move, when we stand opposite S. Pole? In the direction of the hands of a clock. (115.) The terms East and West, in free space. — We have seen (113) that, to an eye above N. hem. (fig. I), objects, moving, with the earth's daily rotation, eastward, move in a direction contrary to that of the hands of a clock; whereas, to an eye above S. hem. (fig. K), objects move with the hands of a clock — that is, in the same direction. Yet, as the earth's daily motion is always from West to East, the objects on it can never change their direction. This is to he NINETEEN LAND AND WATER DIVISIONS. 65 explained as follows. There is no such thing as East or West in infinite space. If the N. Star and solar system did not exist, how would you describe North, South, East and West? The terms are relative — invented by the inhabitants of the earth. That part of oar horizon in which the sun rises, we call the East — the opposite point, the West. As the sun's apparent daily motion is from E. to W., and as this apparent motion results from a real, contrary, daily motion of the earth, on its axis, we say the earth revolves on its axis from TFcst to East We know that the sun and all the planets revolve on their axes, in the same direction as the earth does; we say therefore the sun and the planets revolve on their axes from W. to E. The earth revolves around the sun in the same direction as that in which it revolves on its axis; we say therefore the earth revolves around the sun from W. to E. All other planets revolve around the sun, in the same direction with the earth; we say therefore all the planets revolve around the sun from W. to E. In order to understand North, South, East and West on the earth, we must suppose our face to the N. pole and our back to the S. pole (28). But for persons not on the earth, this definition must be enlarged. Let us leave our planet in our Light-Car and choose a point directly opposite the S. pole, so that our globe is presented to us as in PI. I. K. We now know the earth moves from W. to E., and when we stand opposite the S. hem., we stand with our face toward the N. Star. Thus we can still speak of North, South, East and West, as when we stood upon the earth. Here we perceive also another circumstance, that not only all the planetary movements are from W. to E., but, standing as we do with our face toward the S. pole (and also of course toward the N. Star), the earth's movement on its axis is in the direction of the hands of a clock. If we recede far enough to obtain a view of the entire solar system (PI. VIII. B), we shall see that the planetary movements are uniform 5 66 PHYSICAL GEOGRAPHY. — from W. to E. — and (to ns standing on the south side) in the direction of the hands of a clock.* If we go to opposite side of solar system (i. e. the north side), the motions, of course, would be contrary to that of the hands of a clock. To a person standing behind a transparent clock, the movement of the hands would be reoersed. That is the reason why the direction of the revolving objects, in fig. I, is the reverse of those in K. Which way does the earth move in C? Neither with, nor contrary to, the hands of a clock, as we are neither over N. nor S. hemisphere. But in D, where we look down upon the northern hemisphere, we see a direction contrary to that of the hands of a clock. (116.) Light-Car over Land Hemisphere (L). — We now move to that point whence we behold, at a glance, the greatest mass of land. Name objects visible. Begin at America going eastward. Repeat them westward. Name objects not visible (M). Point out circles. Which way does the earth revolve in L? As the hands of a clock? or in a contrary direction? In a contrary direction. Why? Because, viewed from the north side of the globe, instead of the south side. Where is the N. Star, in L? Behind our head, but not exactly over it. (117.) Light-Car over Water Hemisphere (M). —-Name objects visible.— Objects not visible. Point out circles. Which way is the rotation, compared with the hands of a clock? In the same direction. Why? Because we are opposite S. hem. (117 A.) Bemark. London (L) lies almost exactly in the central point of the Land Hemisphere; while • In the diagram (PL. VDI. B), the planets are represented (by the small arrows) as moving contrary to the direction of the hands of a clock. Why? Because we are there supposed to be looking down on the northern hemispheres. You have only to turn the transparent sheet toward a window; you will then be opposite their southern hemispheres. Then their motions will he in the direction of the hands of a clock. NINETEEN LAND AND WATER DIVISIONS. 67 New Zealand (M), a British possession, lies nearly in the central point of the Water Hemisphere. (H7B.) We know very little of the arctic and still less of the antarctic region. They have resisted all man's efforts to penetrate into their awful solitudes. It is not probable that, any human being has ever visited those points of our globe's surface called the poles. . If the climate were not an insurmountable obstacle—if a mild, perpetual summer could displace those frozen winters with their eternal ice-masses, we should be surprised tO' .see how near, in reality, are British America, Siberia, etc. (L); how those coasts, now frequented only by the bear, the walruss, the seal, and legions of other animals and birds, would be crossed by lines of rapidly going steamers, or perhaps railroads — so that points of the globe, at present, for all purposes of intercom¬ munication, the most remote from each other — as, for instance, Behring Str. and London (L)—C. Horn and Australia, etc. (K) — would be brought together, as Italy and England — New York and Cuba. (118.) Boundaries of continents and oceans. — Examine these boundaries on each of the proper figures, as well as on the one indicated. Bound Western Continent (E). — N. by Arctic Ocean; E. by Atlantic; S. by Atlantic, Great Southern Ocean and Pacific; W. by Pacific, Behring Str., separating from Asia, and Arctic Ocean. Eastern Continent (G). — N. by Arctic Ocean; E. by Behring Str., N. America, Pacific, Malaysia, and Indian Ocean; S. by Pacific, Malaysia, Indian, Great Southern and Atlantic Oceans; W. by Atlantic and Arctic. Bemark. The whole E. Continent is not given on E. hemisphere; the N. E. part of Asia stretches over into W. hemisphere and nearly joins the N. W. part of N. America, from which it is separated by Behring Strait (E. F. I. L.). 5* 68 PHYSICAL GEOGRAPHY. Australia (G). — N. by Pacific and part of Oceania; E. by Pacific and part of Oceania; S. by Great South¬ ern Ocean; W. by Indian Ocean. Antarctic Continent (K). — N. E. and W. by Ant¬ arctic and Great Southern Oceans. It has properly speaking no southern boundaries — except S. Pole. For doubt, as to Antarctic Continent, (101B). Nctrth America (E). — N. by Arctic Ocean; E. by Arctic, Atlantic and part of S. America; S. by Atlantic and Pacific; W. by Pacific, Behring Str., separating from Asia, and by Arctic Ocean. South America (E). — N. and E. by Atlantic; S. by Atlantic, Great Southern Ocean and Pacific; W. by Pacific and a small part of N. America. Europe (G). — N. by Atlantic and Arctic; E. by Asia; S. by Asia and Africa; W. by Atlantic and Arctic (103). Asia (G). — N. by Arctic; E. by Behring Str., separating from N. America, and by Pacific; S. by Pacific, Malaysia, Indian Ocean and Africa; W. by Africa, Europe and Arctic. Africa (G. H). — N. by Atlantic, Europe and Asia; E. by Asia and Indian Ocean; S. by Indian, Great Southern and Atlantic Oceans; W. by Atlantic. Pacific (F). — N. by Asia, Behring Str. and America; E. by N. and S. America; S. by Great Southern Ocean and Australia; W, by Australia, part of Oceania, Indian Ocean and Asia. Atlantic (H). — N. by S. America, N. America, Arctic Ocean, Africa; E. by Europe and Africa; S. by Africa, Great Southern Ocean and S. America; W. by S. and N. America. Indian Ocean (G). — N. by Africa and Asia; E. by Pacific, Malaysia and Australasia; S. by Great Southern Ocean ; "W. by Africa and Asia. Great Southern Ocean (K). — It is bounded only on the North and South. N. by S. America, Atlantic, Africa, Indian Ocean, Australia and Pacific Ocean; S. by Antarctic Continent and Ocean. EARTH 8EEN FROM MOON. 69 Arctic Ocean (I). — The water within arctic circle is called Arctic Ocean. Whether the area be chiefly land, ice or water, we know not; how is it bounded? N. by N. Pole, which is also its center; S. by N. America, Atlantic, Europe, Asia and Pacific, to which it is united by Behring Str. Antarctic Ocean (K). — We can only say, it is bounded N. everywhere by Great Southern Ocean, and S. E. or W. by what is called Antarctic Continent. EARTH SEEN FROM MOON. (119.) Suppose we now make an imaginary journey to our nearest neighbor among the heavenly bodies — the moon; (although, probably, no human being could exist there). Distance, about 200,000 miles; — by rail¬ road {sec. 16), 8 months; — by Light-Car, one second. Fancy that, (an exception to all other mortals,) we have reached the moon. We anchor our Gar upon some broken plateau, surrounded by shattered cliffs. It is one of her long nights (two of our weeks). The most prominent object, in the starry concave above our heads, is an immense, magnificent moon, 14 times larger than the full moon appears to us. That is our earth. Con¬ trasted with the dark sky, its broad, illuminated disk offers a spectacle of unsurpassable interest and splendor. The continents and oceans are distinctly visible (when the dense vapor which loads our gross atmosphere, permits a clear view). The circles of snow and ice, under which the polar regions lie perpetually buried, shine with white, dazzling lustre. That around the S.Pole, is the larger (101A—740—600). The landmasses are brighter than the oceans, because land reflects, and water absorbs, light. The continents are spotted, here and there, with clouds — mountain-ranges and shadows — vallies — seas — deserts — table-lands — glaciers — pri¬ meval forests (those of N. America, Brazil etc.). With our telescope, we fancy we descry faint indications of 70 PHYSICAL GEOGRAPHY. the larger cities. While we gaze, one edge of the luminous orb darkens; a black, circular shadow moves, for some hours, across its disk, and gradually passes off at the opposite edge. That is the shadow of the moon itself. The countries of the earth, over which it passes, have an eclipse of the sun. Western Hemisphere. — Our first view is (let us say) the W. hem, (fig. E)*. As we contemplate it, with wonder and delight, we become aware that the spots are not stationary. They move, very slowly, along the disk, from W. to E. The mighty globe is majes¬ tically revolving on its axis. The Atlantic gradually disappears. America moves toward the eastern edge. S. America speedily passes beyond the edge and van¬ ishes (F). The Pacific (with Oceania) comes more and more into view; until, in about six hours, we have before us the: Pacific Hemisphere. — Here (F) the globe has turned one quarter around. We see part of W. hem. and part of E. hem. As the movement is scarcely perceptible, we have ample time" to study the objects. This side of the earth — the Pacific hemisphere — affords an unbroken view of that vast waste of water, in all its immensity, washing the coasts of Asia, Australia and America, and reaching nearly from pole to pole (for what we call the Great Southern Ocean, however properly designated by a name of its own, is still a continuation of Atlantic, Pacific, and Indian Oceans). While we gaze, the objects almost imperceptibly change their positions. N. America, in a few hours, and, after it, the principal part of the Pacific, advance beyond the eastern edge and disappear. Australia moves for¬ ward, on its way around to the other side of the sphere * The figures E, F, Gr, H, with their circles and names, are, of course, not intended to represent the supposed appearance of the earth, seen from the moon. But, as they are successive hemispheres brought into view hy four periods of one revolution, the pupil will find it agreeable to use them during the follow¬ ing description. EARTH SEEN FROM MOON. 71 ■(as in G). That subdivision of Oceania, called Ma¬ laysia, in 12 hours, passes from western to eastern edge. Behring Str. vanishes over north-eastern limit, till, in about six hours more, the retreating objects are succeeded by whole E. Continent and Indian Ocean*. They glide along with no greater celerity than the hour-hand of a clock. Eastern Hemisphere (G). — The stupendous globe has now made exactly a half revolution. It has turned W. hem. completely away and brought E. hem. into full view. Slowly advancing, by and by, Asia and Australia follow the remnant of Pacific out of sight. Europe and Africa creep forward toward the eastern rim (as in H); till yet other portions of the globe's surface come round and the: Atlantic Hemisphere (H) — now lies broadly be¬ fore us. The entire Atlantic, with its vast, broken coasts, has glided into the center of the disk, revealing its immense form, somewhat in the shape of the letter S. Slowly N. and S. America project forward their huge shattered angles, followed by the deeply indented gulfs of N. America; while the Pacific, which only an hour or two before, sank beneath the eastern edge, already re-appears on the western side. Remarks. Has the earth yet completed a revolu¬ tion? No. For that, it requires about six hours more. It would then present to us the W. hemisphere again (as in E), and so, forever and ever, it accomplishes its wonderful revolutions (24); every place returning to a given meridian in precisely 23 hours, 56 minutes, 4 seconds and nine one-hundredths of a second — counting from that hundredth part of a second on which it left it. To the inhabitants of the moon, if there were any, it would perform the office of a clock far better than any machine made by human hand. * The hemispheres F and G do not absolutely correspond to the period of six hours. The slight deviation was expedient in order to present unbroken outlines of the Pacific and Atlantic. 72 PHYSICAL GEOGRAPHY. We may, at our ease, contemplate this phenom- enon; for the glorious orb will never set, as the moon does to us. It reniains stationary in its place; becauso the moon itself revolves on its axis, only once a month, and, in such a way, as to keep the same side always: turned toward the earth. But, although the stupendous orb never sets, a person, in the moon, would see it pass through the same monthly phases, as the moon does to us. Sometimes, it would float in the heavens, a slender crescent; sometimes, a half moon ; and some- times, the mighty globe would turn broadly toward him its entire, illuminated hemisphere. These varying phases are caused by the monthly revolution of the moon around the earth, which brings her, sometimes, between the earth and the sun (when she has the earth as a full moon) — sometimes, to a point, where the earth is be¬ tween the sun and her (then she sees the earth, if at all, as a crescent). Remark, the earth, as a half moon (Ë to M), would not be all visible, as in the figures. The night-half would entirely disappear. Along the broken edge, would be, at times, distinguished the illu¬ minated peaks of the Andes, Alps etc. DEFINITIONS OF LAND DIVISIONS. (120.) Remark. — It is not expected that every younger student will here acquire a very exact idea of the objects treated in the following definitions. They are now merely to be read over as a preparatio-n; each pupil reading, aloud, one at a time. They will be referred to, hereafter, again and read over more under standingly, at the proper stages of the lessons, and in connection with examples. (121.) Continent. — A term applied to the three largest landmasses of the earth, and, doubtfully, to the frozen mass, whether of ice or islands, within antarctic circle. The word is often used by geographical writers, when speaking of smaller land divisions; as. Continent of N. America; Continent of S. America; Continent of Europe; Continent of Asia; Continent of Africa. DEFINITIONS OF LAN,D DIVISIONS. 73 ^122.) Island. — A portion of land, smaller than a continent, entirely surrounded by water. (123.) Island Chain. — Islands ranged in a line, whether straight or curved, are termed a chain. Such fre¬ quently connect a group with the mainland; or promonto¬ ries or peninsulas, with corresponding portions of the oppo¬ site coast; as, Aleutian or Fox Is., connecting N. America with Asia — the three chains, of which the West India Is. are principally composed (PI. III. fig. 3), namely: 1. Cuba, Jamaica, St. Domingo, and Porto Rico. 2. Bahama Is. (ba- hay'-ma). 3. Lesser Antilles-, also (PI. II.) Kurile Is. with Japan—Ladrona Is., etc. (124.) Peninsula. — Land almost surrounded by water as. Nova Scotia, Florida, Italy, Malacca. (125.) Key. — Sometimes Cay (from the Spanish cayo, an islet), a ledge or lay of rocks near the surface of the water; or a chain of low, sandy islands, reefs and sandbanks sometimes of coral formation, very dangerous to the navi¬ gator, as (PI. III. fig. 3) Florida Keys, southern extremity of Florida, constantly the scene of disastrous shipwrecks. The term is applied to many small islands in the West Indies; also to certain islands of Oceania, in the south west of the Moluccas. (126.) Isthmus. — A narrow neck of land joining landmasses. (127.) Coast or shore. — That part of land which borders on the sea. The shore or beach of the sea is sometimes called the strand-. "From Greenland's icy mountains; From India's coral strands." Bluff. A high bank, almost perpendicular, projecting into the sea or a river—an American term, used princi¬ pally to designate the abrupt banks and high clifis along the Mississippi. (128.) Cape. — The extreme point of a portion of land stretching into the sea. 74 PHYSICAL GEOGRAPHY. (129.) Promontory. .— A high point of land or rock projecting into the sea. It differs from a cape in denoting highland. Every promontory therefore is a cape, but every cape is not a promontory (prom'-on-to-ry). (130.) mountain—Knob — Dune—Down. — A mass of earth or rock greatly elevated above the surrounding country. Hill is a mass of earth rising above the common level of the surrounding land. A hill is less high than a mountain, but of no definite magnitude. The term is some¬ times applied to a mountain. Knob is a hill or low mount¬ ain with a round top. Dunes—low hills of blown or movable sand on low coasts; as, the dunes of England, France, etc. Down — an elevation or bank thrown up by the sea; in England, also a tract of poor, naked, hilly land, used only for pasturing sheep. Remark. A well known road for shipping, in the English Channel, near Goodwin Sands, is called the Downs. (162. 162 A.) (131.) Monntain-range—ridge or chain. — A term ap¬ plied to a number of mountains, more or less united at the base, and having the same direction; as, the Andes, Rocky Mts., Alleghanies, Ural Mts. (132.) mountain-system. — This term has two mean¬ ings; first, a mass of mountains elevated at the same geo¬ logical period; as, the Pacific Range, the Himalaya, the Ural Mountains. The Alps and Apallachian (or All^hany) Mountains, on the contrary, were each thrown up, by different plutonic actions, at different periods. Secondly, the term "mountain-system" is applied to mountain - chains grouped together without reference to geological age. (133.) Peak. — An elevated mountain, isolated, and of difficult access, the summit of which, seen from a distance, appears pointed. The term is also applied to the most elevated summits of a mountain-range. Crest is a general term for the highest part of a mountain. (134.) Volcano. — An opening in the surface of the earth, or in a mountain, which casts out fire, smoke, ashes, lava and other substances, (vol-cay'no). DEFINITIONS OF LAND DIVISIONS. 75 (^loO.j Uonntain-pasB. — A place, between peaks, or higher elevations, where a mountain-chain is passable. Mountain-passes are usually at the angle formed by one part of a chain with another, and consequently, being at the head of valleys, are also at the headwaters of rivers. A pass was sometimes, by the ancients, called a gate, as it is now by the Spaniards. (135 A.) Gap — Col—Port — Defile—Gorge — B a vine — Quebrada (kay-brah'-da) — Canon—Barancas. — In the United States and British America, mountain - passes are often called gaps; in the French Alps, cok (from the French word col, narrow) as. Col de Balme, Col de Tenda, etc.; in the Pyrenees, ports, as. Port de Roncevaux. Defile ^\s a narrow passage, between precipitous rocks, especially if long and winding; gorge is often near the summit of a mountain ; and ravine is a long, deep, narrow hollow, worn by a stream or torrent of water; hence, any long deep and narrow pass through mountains. Quebradas immense "breaks" or "valleys", frequently 2000 feet deep, with a stream running at the bottom. In some parts of S. America, • Mexico and adjacent territories, the term canon (kan-yown) is applied to a high, narrow defile through which flows a rapid stream; or to a deep ravine, worn in the mountains by torrents. Barancas are immense rents in the earth's surface by volcanic action. In Mexico they intersect parts of the country in a direction E. and W. The precipitous walls rise sometimes 1000 feet. (136.) Valley. — A tract of land between hills or mountains. Remark. The term "valley" may be applied to any depression on the surface of the globe; the beds of the oceans are only great valleys. Vale is the diminutive of valley, properly applied to undulating depressions between hills. (137.) Avalanche. — An immense mass of snow and ice, precipitated, with thundering roar, from mountain - heights, into the valleys, and sometimes bearing away, and burying travellers, huts and entire villages. The term is also applied to masses of earth and rock in Alpine regions which break away and slip down. 76 PHYSICAL GEOGBAPHY. (^Idö,^ Olacier (glay'-seer). — Vast fields or immense accumulations of ice, perpetnallj filling the more elevated parts of valleys in the higher mountain-chains, and always in slow motion. They sometimes descend considerably below the snowy mountain elevations and advance far into com¬ paratively low, fertile valleys. The Alps, Norway, Iceland, Spitzbergen, the shores of the Antarctic Continent, present extensive, remarkable examples. There are numerous snow peaks in the Andes, but few or no glaciers, except in Patagonia, where are found the most tremendous and astonishing of the globe. In the Alps, 400 have been counted, occupying a space of 14,000 sq. miles. These glaciers move slowly downward, "intruding themselves, like unwelcome guests, into the lower valleys". They bear with them immense blocks of stone, with masses of gravel and mud. One of these transported blocks measured 100 feet long by 40 broad. Some of the Swiss glaciers are 400 yards in length; others 20 miles long by ó broad. Sometimes the lifeless bodies of men, lost among the mountains, are discovered, years afterward, perfectly preserved in the ice, at places remote from the spot where they perished. Until recently it was supposed there were but few and small glaciers in the Himalaya Mountains; modem travellers have discovered them of extraordinary extent and stupendous height. (138 A.) Ice period. — Remark. The glacier theory, elaborated by Agassis, supposes that the frigid and temperate zones were, at some period or periods, covered with ice nearly to the tops of the highest mountains—that the temperature, from whatever cause (98), has gradually risen and melted the ice, the agency of which, during its formation and dissolution, accounts for several phenomena; the rounded forms of bowlders (592 A), the deep lines on certain rocks, the distribution of various stones and other loose materials over the earth's surface, etc. (602.) (138B.) Iceberg. — A hill or mountain of ice floating on the ocean, sometimes detached from the ice masses on the shore of the frigid zones, sometimes formed at a distance from the land, often carried toward the equator as low as the 40"» parallel, making the early summer passage between the United States and England dangerous. Fifty icebergs DEFINITIONS OF LAND DIVISIONS. 77 have been seen at one time floating on the coast of Pa¬ tagonia, one of which was 160 feet high—all loaded with blocks of granite and other rocks. Occasionally gla¬ ciers, descending by the slow motion mentioned in sec. 138, reach the sea and become icebergs. (101Á.) (139.) Watershed. —• An elevated part or ridge of a country which divides the sources of its streams or rivers — one set, flowing down one of its slopes, the other, down the opposite one. The entire mountain - range or region, in fact, may be called a watershed. Remark the Rocky Mts., for instance (PI. II.), with the rivers flowing down the eastern and western slopes. From the great Himalaya watershed, see what rivers flow to the N., to the E., to the S., and to the W. So of the Alpine system — also of the Alleghany system (PI. VII.), etc., etc. (140.) B asín*. — The entire tract of country drained by a river and its tributaries. The basin of a sea is the region watered by all the rivers which it receives. (141.) Table-land—High plain—Blatean. — A level, or nearly level, tract of land, at a considerable height above the sea. A very large portion of the dry land of the globe consists of extensive, more or less elevated districts. (142.) Terrace. — This term is applied to plateaux particularly when rising in succession one above another, as the terraces of Guiana. (143.) PI ain — Lowland. — An extensive tract of laud nearly flat, as the great northern plain of Europe and Asia, the plains of Lombardy (river Po) and Hungary (Danube). When at about the level of the sea it is often called Low¬ land or Lowlands. Hence the term as applied to Holland, {Pays Bas, Netherlands, Lowlands). The plain of Hol¬ land is so low that the whole country, but for the dikes, would be overflowed by the sea. The plain, around the Caspian and Aral seas, sinks considerably below the level * In some respects a hasin is synonymous with valley, ex¬ pressing the same idea; as, the basin or valley of the Amazon, of the Mississippi, of the Po. 78 PHYSICAL GEOGRAPHY. of the ocean, forming a vast cavity of 160,000 sq. miles. The surface of the Caspian Sea itself lies 348 feet below the sea level. The low plains and steppes of Europe and western Asia are occasionally crossed by hills swelling in long waves or undulations. (144). Frairie. — An extensive tract of land mostly level, destitute of trees, covered with tall, coarse grass; as, in the United States, W. of the Alleghany Mts., especially between the Ohio, Mississippi and the five great lakes. (145.) Savanna. — Indian name given to the large grassy plains in the southern part of Ñ. America; as, the Alachua Savanna (Florida). (146.) Llanos (lyanos). — Spanish word for great plains on the Orinoco — on the La Plata, pampas (PI. II). (147.) Karroos. — Extensive interior plains of southern Africa (Cape Colony), occupying most of the terraces be¬ tween the mountain-ranges. In the great karroo of Cape Colony, there is sometimes no rain for 2 or 3 years. The karroos, the hunting-grounds of the colonists, are wonder¬ fully crowded with various kinds of animals — the antilope, buffalo, elephant, river-horse, rhinoceros, wild ass, zebra, etc. (147 A.) Vlakten. — African plains in the Orange Kiver Territory, useless for agricultural and pastoral pur¬ poses; but, like the karroos, supporting incredible numbers of animals — herds of tens of thousands. (148.) Steppes — (from the Russian, step, harren). Vast level plains, destitute of trees, in .south-eastern Euro¬ pean and Asiatic Russia—marked by ifearful extremities of cold and heat — neither man nor animal can resist their storms — in the summer-drought, cattle perish by thousands. (148A.) Tnndra or Tundras a succession of level, desert tracts forming the northern part of the great plain of Siberia (582.), near Arctic Ocean (Kara Sea, Asiatic Polar Sea)—in the short summer, covered by lichens and other mosses, coarse grass, and dwarf willows — in the win¬ ter, one dreary extent of solid ice (PI. II). DEFINITIONS OF LAND DIVISIONS. 79 (149.) Silvas (Pl. II.) — Portuguese name for vast plains in valley of Amazon, covered with primeval forests. (150.) Desert. — A vast and barren tract of land; as, desert of Sahara, desert of Gobi or Shamo. (151.) Oasis, (ö'-ay-sis) — A fertile spot in a desert, watered by springs, as the oasis of Tuat, 100 miles long and 15 wide. It is generally a depression below the surface. (152.) Delta. — A term applied to low tracts of land sometimes found between the forks of a river (172), or at its mouths. These tracts are generally triangular, some¬ what in the form of the Greek letter delta A. whence the name; as, the delta of the Nile, Ganges, Niger (Ni'-jer). (152 A.) Swamp — marsh — morass — bog — quagmire (that is quake-mire)—everglade—quicksand —. Various terms applied, under somewhat different circumstances, to low, spongy ground saturated with water; for instance, the Great Dismal Swamp in Virginia and N. Carolina —40 m. long by 25 m. broad—consisting of black, soft, wet, vegetable matter — generally covered with stagnant pools. There is another swamp in N. Carolina, called the Little Dismal. These two once formed retreats for run-away negro, slaves. Persons have been born, have lived and died there, never seeing any thing else of the earth, and perhaps never knowing that the globe offered scenes of adifferent de¬ scription. The Runn of Cutch in Arabian Sea {sec. 230 and PI. II.) is another example. Everglade, a tract of land of large extent, more or less covered with water; the Ever¬ glades of Florida, for instance (PI. VII.) —160 m. long, 60 broad — studded with thousands of islands — might al¬ most be called a lake; the water, only from one to six feet deep, does not prevent a rank growth of tall grass — soil adapted to the banana* (bah-nah'-nah) and plantain * BANANA — a delicious fruit—size and form of the cu¬ cumber— growing almost spontaneously and abundantly, upon a tree 15 or 20 feet high — sometimes a hundred bananas are found on a single stock — leaves, from six to ten feet long.— "No other plant", says Appleton's Am. Cyclop., "produces the same amount of nutriment, from the same space of ground". The plantain is a variety of the species. 80 PHYSICAL GEOGRAPHY. (plan'-tin). Quicksand or Quicksands—tracts of loose, unsolid sand which have the appearance of land, and yet are yielding like water — formed on many sea-coasts, or at the mouths of rivers, as those of the NUe and Senegal. The horseman or other traveller, hastening on his way, suddenly disappears, in one of those places, and is never seen again. DEFINITIONS OF WATER DIVISIONS. (153.) Ocean. — A va.st body of salt water. (154.) Sargasso Sea or Fnons bank. — A large tract of the Atlantic, extending from Bermudas to Azores and C. Verde Is. — covered, at intervals, with vast quantities of a marine plant (sea-grass or gulfweed) called sargasso (fucus natans)—sometimes torn from its roots in the Mexican Gulf and collected in this part of the ocean by the vast whirling eddy of one of the branches of the Gulf Stream- sometimes growing up from the bottom of the sea, which Humboldt concludes to be, here, an immense submarine pla¬ teau. It occupies an area equal to six times that of Germany — but, at different seasons, its dimensions are changed by winds and currents. The appearance is that of an endless, ever green, inundated prairie, the grass swaying gently to and fro with the waves and winds — in some places, sufficiently thick to impede the advance of a ship during a light breeze— inhabited by innumerable marine animals. It was discovered by Columbus, and caused great alarm to his crew, who feared they would never escape from its entanglement. Similar tracts are found at south-east extremity of South America (neighborhood of Falkland Is.), in Southern Ocean (south of Indian Ocean), where it is called Long Kelp', and in Pacific (North of Sandwich Is.). Occasionally the stems are 800 feet long and nearly a foot in diameter. (155.) Sea. — As usually applied, is a body of salt water smaller than an ocean. DEFINITIONS OF WATER DIVISIONS. 81 (156.) Archipelago (ar-ke-pel'-a-go). — Â sea studded with groups of islands. The term was originally applied to the sea between Greece and Asia Minor, i. e. Aegean Sea (e-jee'-an), and is derived from the Greek, arc/ios, chief, and pelagos, sea, because that was the most important sea to the Greeks. A number of island groups is called an aréhipelûgo. (157.) Tide. — The alternate rising and falling of the waters of the ocean, with bays, rivers and waters connected therewith. The tide ebbs and flows twice in little mOre than 24 hours. The flow or rising of the water is called the Jiood-tidé, the descent of the water, the ebb-tide. The tide, higher than the common tide, which happens twioe a month, namely at. Or soon after, the new and full moon, is called the spring-tide. The tides which happen near the first and last quarters of the moon, when the difference between high and low water is less than at any period of the month, are Called neap-tides. They are the opposite to spring-tides. A tidal wave, following the moon in her revolution, flows around the earth, arriving at any partic¬ ular place about 50 minutes later every day (605). (157 A.) Bore—pororoca. — When the tidal wave, compressed within a narrow channel, rises rapidly with terrible force and noise, this is ëalled a bore (from a Hindoo word, signifying a flood); as, the bore of Bristol Channel, Bay of Fundy, the Hoogly, the Amazon (2ÓSA and 605 F). Nearly all similar situations, especially where exposed tö the direct action of the tidal wave, show more or lesS of this phenomenon. (158.) Ocean Current. — Constant and reprúlar move¬ ments of portions of the ocean, in certain directions — in their nature and origin, quite distinct from tides. They sweep forward, through the surrounding flood, like rivers flowing between their banks (604) ; ex. Japan Current, etc. (159.) Gnlf. — A portion of water almost surrounded by land. (160.) Bay. — An indentation of the ocean, lying more open than a gulf. 6 82 PHYSICAL GEOGRAPHY. (161.) Bight. — A bend between two points of land — synonymous with bay. (161 A.) Haff — lagoon. The first term is particu¬ larly applied to three large estuaries on S. shore of Baltic (PI. V.)—communicating with it by narrow passages. They are all in Prussia, at the mouths of the Oder, Vistula and Niemen; example: Stettiner Haff. Lagoon — an extens¬ ive body of shallow water, near the sea and connected with it; lagoons of Venice. (162.) Port—Haven—Harbor—Boad or Boadstead— Downs. — Any bay, cove, inlet or recess of the sea, or of a lake, or the mouth of a river, which ships or vessels can enter, and where they can lie safe from injury by storms. Ports may be natural or artificial-, sometimes works of art, as piers and moles, are added to the natural shores of a place, to render a harbor more safe. The word port, is generally applied to spacious harbors much resorted to by ships, as the Port of New York or Boston-, and not to small bays or coves which are entered occasionally, or in stress of weather only. Harbor includes all places of safety for shipping. Road or Roadstead — a part of the open sea or other water at some distance from the shore, where ships may ride at anchor in safety; for instance (PI. VI. B) Spithead, S. coast of England, near I. of Wight; also the Downs, S. E. extremity of England, near Str. of Dover, where valuable shelter for shipping is ensured by the Goodwin Sands which serve as a breakwater. (162 A.) Shoal or Shoals — shallow sandbanks, often dry at low water; for example, Goodwin Sands—a range of shoals in the Str. of Dover.- Their shifting and loose nature is in the highest degree dangerous to life and prop¬ erty. Sbakspeare alludes to them three times; Salanio. Now what news on the Rialto? Salarino. Why, yet it lives there unchecked, that Antonio hath a ship of rich Jading wrecked on the narrow seas; the Goodwim,, I think they call the place; a very dangerous flat, and fatal, where the carcasses of many a tall ship lie buried. (Merchant of Venice.) ^163.) Bank, — Shoals, shelves or shallows — also ele¬ vated ground at bottom of sea, as. Bank of Newfoundland-, one of the most extensive submarine plateaux of the globe DEFINITIONS OF WATER DIVISIONS. 83 — 600 m. long, 200 m. broad — 25 to 94 fathoms deep — bottom, in some places, solid rock—covered with dense fog from Gulf Stream — swarming with cod and almost every other variety of fish—yielding annually several million dollars—occupying 2 or 3000 vessels. Another example is that remarkable elevation of the bottom of the sea extend¬ ing between Ireland and Newfoundland, sometimes called Telegraphic Plateau, on which was laid great submarine telegraphic cable which unites Europe with America. (164.) Seef—bar—breaker. — Numerous low rocks lying at, or near, the surface of the water. Those stony habitations, constructed for themselves, in various parts of the tropical seas, by the little coral animals, the zoophytes (zö'-o-fites), are called coral reefs. The coral builds not only reefs, but regular islands. In the space of ocean, extending from the southern end of the Low Archipelago (Polynesia) to the northern end of Marshall Archipelago, every island, with one exception, is atoll-formed—atolls being circular islands of coral, with a very shallow salt¬ water lake within them. Some of these islands measure from fifty to eighty miles in length and nearly twenty miles in breadth. Bar—a bank of sand, gravel or earth forming a shoal at the mouth of a river or harbor, obstructing entrance or rendering it difficult. Breaket—waves forced by the tide, wind or currents, foaming and roaring over rocks and shoals. The term is sometimes applied to the rocks themselves. (165.) Strait. — A narrow passage of water separating two pieces of land and connecting, two bodies of water. A small strait, or the narrowest part of the strait, is some¬ times called a g\it. The term strait is often erroneously used in the plural. (166.) ch annel. — A passage connecting two seas or bodies of water, longer and broader than a strait. (167.) Sound. — Nearly the same as a strait, but distinguished from it in not, of necessity, having a double communication with the ocean; it is also in '^soundings", (eighty fathoms—a fathom, six feet). 6* 84 PHYSICAL GEOGRAPHY. (168.) Belt. — A term applied to narrow passages or straits in the Baltic. The Great Belt is. the passage between I. of Seeland and that of Funen, at the entrance of Baltic. The passage, separating I. of Funen from mainland (Danish Peninsula), is the Little Belt (PI. V). (169.) Lake. — A body of water surrounded by land, often, differing from a sea only as being fresh water. (170.) Biver—Creek—Brook —Bun. — A stream of fresh water flowing into another river, ocean, lake or ether body of water; the spring or fountain, from which it first proceeds, is its source or head; the part, where it empties into another body of water,, is its mouth; the cavity, in which a river flows, is called its channel; the bottom of the channel, its bed; the right and left sides, proceeding frem the source to the mouth, are its right and left banks. The banks may be sloping or steep, rocky or fertile. Some rivers, particularly in Africa, lose themselves in sand. The salt tide-water of the oceans enters into many rivers for some distance from the mouth. Greek—a narrow portion of water running into the land: in some of the American States a small river. Brook—a small natural stream of water, or a current flowing from a spring or fountain less than a river. In the Middle and Southern States of America, run is used in a like sense ; but it is also applied to streams larger than a brook. (171.) Estuary—Frith — Firth (furth) — a narrow passage of the sea. The term is occasionally used to des¬ ignate that part of a river opening into- the sea, as Frith of Forth — Swedish, Fiord. (172.) Tributary—affluent—fork—branch. — An¬ other smaller stream which flows into a river; for instance, the Ohio has many large tributary streams and is itself tributary to the Mississippi. The point, at which they unite, is called the conjiuence; as, the confluence of the Tigris and Euphrates, or of the Ohio and Mississippi. The term fork is applied to the part where a river divides, or rather where two rivers meet and unite into one stream. £ach branch is called a fork (15*2). DEFINITIONS OF WATER DIVISIONS. 85 (173.) Cataract — A large body of water falling over a precipice. The greatest of the world, believed to be Falls of Niagara. (174.) Cascade or waterialL^— A small body of wa¬ ter falling over a precipice. (175.) Kapid. — The part of a river where its bed is much inclined and the water rushes down rapidly. (176.) Xoch. — In Scotland a lake or an arm of the sea is sometimes called a loch, in Ireland lough (lock). (177.) Whirlpool—Eddy. .— When, by the force of the tide, or currents, pressing the water diagonally against the shore, or between rocks or banks, a circular direction is given to it; or where a similar effect is produced by the meeting of two currents; or by deep holes, causing a downward suction — this is termed an eddg. In the latter case, when very large and powerful, it is called a whirlpool-, as the Maelstrom (mahl'-strum) i. e. millstream — caused by the force of' currents and of the ebbing and flowing tides, among the Loflb'-den and other islands, on the coast of Norway (PI. II). It is not always dangerous. Twiçe every day it subsides to rest (at the two low tides — 605 C.) and is then safely traversed. At certain times—in the winter — during heavy storms—particularly at the full and new moon (605 F) and during equinoxes—it becomes violent and unnavi- gable. Ships must then keep at a distance of at least 10 or 15 miles. Many other whirlpools render this coast dangerous.— Charyhdis — (kah-rib'-dis)—celebrated point in Str. of Messina, between I. of Sicily and mainland, .where strong currents meet and make wild uproar — navigation has been, and still is dangerous — now called Galofaro (193). (178.) Wady, — (Wod'-y) an Arabian word — a river channel, dry, except in the rainy season; as, Wady Draa (southern boundary of Morocco, PI. II). A small valley, a river, even a town, sometimes take this name. (179.) Inle t—Cove. — A recess in the shore of a sea, or of a lake, or large river, or between islands — a kind of bay. Cove—a small inlet, creek, or bay. 86 PHYSICAL 6B06RAPHY. (180.) Remark. The terms, Sea, Gulf, Bay, Inlet, Bight, are very vaguely used. The Gulf of Mexico might be called a Bay; the Bay of Biscay, a Gulf. A gulf is said to differ from a bay only in extent. A bay is a "large or small recess of the sea;" a gulf is only "a large extent of ■water." But why do we say. Bay of Bengal and Arabian Sea ; or Hudson Bay and Gulf of Mexico ? Why not Chan¬ nel of Tartary instead of G. ofTartary? Why not Hudson Gvlf and Bay of Mexico? The student will often find the same piece of water called a gulf, by one geographer, and a bay, by another; as for instance, Mosquito Bay. WATER DIVISIONS. (PLATE II.) (181.) Remark to teacher. Make no demand upon the pupil's memory. Read, slowly, from text book, three names at a time; the pupil, as he finds each place on thé map, reads the name aloud. Thus certain that he is not expected to repeat from memory, his confidence becomes every moment greater; his task, as well as that of the teacher, more easy; and the lesson, as he constantly reads from, and contemplates the map, gradually photographs itself upon his mind and remains there permanently. No study is needed, except the recitation itself, which, for young persons, ought not to be extended over one short hour. (181 A.) How to connt the names. — The names should be repeated, by all the pupils, in the same order, and counted in the same way, by threes, (unless there appear some special reason for the contrary). (181 B.) One pupil must not say Gulf of California, and another, California Gulf, but the name is to be read always, and by everyone, exactly as it is on the map, California. Gulf. In this, as in other respects, the text and Atlas are intended to coincide. (18lC.) The starting-points, that is, Behring Str., Str. of Belle Isle, etc., are counted twice, because they serve as stations or land-marks to guide the pupil. WATER DIVISIONS. 87 (181D.) When an archipelago (156) is namedi and then, any group of islands composing it, count the archipelago-name as one, and each group-name as one-, because our object is, to get a clear idea of the number of names we have to remember; for instance (209), antarctic archipelago, consisting of south Georgia, SANDWICH GROUP, SOUTH ORKNEY, and SOUTH SHET¬ LAND IS., count five. (181E.) Names of river-mouths to be counted with the rest. (181E.) The teacher, ot course, may apply the principle of repetition according to his discretion and the wants of the class. (182.) (Western Continent). — North Coast of N. America, from Behring Strait to Strait of Belle Isle (bel-île). — Behring str., kotzebue sound (kot-se-bü), American polar sea with mouth of mackenzie river. (Read 4). — str. prince of wales, north-west passage, boothia gulf (Read 3. — Read from Behring Str.). — k a n e • s supposed open sea, kennedy channel, kane sea (Read 3. — Read from Behring Str.). — smith str., baffin bay, davis str. (Read 3.—Read from Behring Str.). — hudson bay with mouth of saskatchewan or nelson river, hudson str. (Read 3. — Read from Behring Str.). str. of belle isle. (How many from Behring Str.? Read 17). Remark. Kane's supposed open sea, i. e., supposed to be more free from ice than farther south. (183.) East and South Coast of N. America, from Str. of Belle Isle to Mosquito Bay. — str. of belle isle, G. of st. lawrence with mouth of river st. lawrence, b. of fundy (R. 4). — long island sound, delaware b., chesapeake b. with mouth of potomac r. (R. 4. — R. from Str. of Belle Isle). — florida str. and gulf stream, g. of mexico 88 PHYSICAL GEOGRAPHY. ■with moüth of mississippi r. (R. 4. — F. from Str. of Belle Isle). — campeachy b., hondorab b., mos¬ quito b. C^. 3. — How many from Sir. of Belle Islel B, 45. —Read from Behring Str.). (184.) Whole Coast of S. America, from Mosquito B., around Cape Horn, to B. of Panama. — mosquito b., Caribbean sea (kar-rib- bee'an), darien b. (day're-en). (R. 3.) — g. of mara- caybo (mah-rah-kï-bo), mouth of amazon r. (am'a- zod), all saints bay (R. 3.—R. from Mosquito Bay). — la plata river or bay, st. george gulf, str. OF magellan (mah-jel'laD) (R. 3.—R. from Mosquito B.) — guayaquil g. (gwi-ah-keel'—near equator),— b. OF panama (pahn-a-mab') (R. 2. — How many from Mos¬ quito B.? R. 11. — R. from Behring Str.). (185.) W. Coast of N. America, from B. of Panama to Behring Str. — b. of panama, te- huantepeo g. ((tay-wahn-tah-pek'), california g. with mouth of colorado R. (R. 4) — B. of san francisco with str. golden Gate, mouth of Columbia h. (R. 3. — R. from B. of Panama) — str. juan de fuca (foo'-ka), queen charlotte sound, cook inlet (R. 3. — R. from B. of Panama) — bristol bay, Beh¬ ring sea or sea of kamchatka (kahm-chaht'• ka^ norton sound with kwichpack r. (R. 4. — R. from B. of Panama) — Behring str. (How many from B. of Panama^ R. 15). (185 A.) Rule for teaching. At the end of the section, or as often as may be deemed proper, the pupils, silently examining the map, must answer, each one separately, to the question: how many, etc.? If any answer incorrectly, that one must be asked to prove the answer, by pointing out the objects on the map; the others may correct him, until the class be unanimously agreed. (185£>.) The class will now answer, as above, to the following question : how many waterdlvisions have we named water divisions. 89 altogether from Behring Str. to Behring Str.f (the teacher has alwajs the answer in his hand). Kead 58. (185 C.) Remark to the class. You say there are 58 naqies ftom Behring Str. to Behring Str. again. Have ^ou not counted some of them more than once? Examine what the actual number of names is. Answer: 54. What were the four starting-points? Answer; behring str.— str. belle isle —mosquito b.-b. of panama. How many times too often did you count each of those starting- points? Each one was counted twice. Suppose I say you have counted each starting-point three times; prove to me the contrary from the map? You have then learned 54 names instead of 58. ( R. 54 from PI. III. — then from PI. IV. — then, as far as they are to he fotmd, from PI. VII). (186.) (Eastern Continent). — E. Coast of Asia, from Behring Str. to Str. of Malacca. — behring str., anadir g. (ahn-ah-deer'), behring sea or sea of kamtchatka again (R. 3) — sea of okhotsk (o-kotsk'), g. of tartary with mouth of amoor r. (ah-moor') (R. 3 — B. from Behring Str.) — japan sea (jab-pan'), str. 9f corea (ko-ree'-a) (B. 2 — R. from Behring Str.) — yellow sea with mouths of hoang-ho and yang-tse-kiang rivers (yahng-tse- ke-ahng' — (R. 3 — R. from Behring Str.) — china sea with mouth of canton r., tonquin g. (ton-keen') (R. 3 — R. from Behring Str.) — siam g. (st-am'), str. of malacca (R. 2 — How many from Behring Str.f R. 16.) Remark. We select only a few great rivers. (187.) S. Coast of Asia, from Str. of Malacca to B.ed Sea. — str. of Malacca (mah-lak'-ka), b. of bengal (ben-gawl') with mouth of ganges r. (gàn'-jeez) (R. 3) — palk's str. (pawk), Arabian sba with mouth of indus r. (R. 3 — R. from Str. of Malacca) — g. of oman (o-mahn'), sttr. of or'mus (R. 2 — R. from Str. of Malacca) — Persian g. with mouth 90 physical geography. of the united rivers tigris (tî'-gris) and edphrates (u-frä-teez) (E. 3.—E. from Str. of Malacca — now out of Persian G., by Str. of Ormus and G. of Oman) g. of aden (ah'-den), str. of bab-el-man'deb, red sea (i2. 3.—E. from Str. of Malacca — now in Eed Sea, consult also fig. 5.) g. of a'kabah, g. of suez (soo'-ez) (E. 2. — How many from Str. of Malacca"? E. 16.—Eead from Behring Str.). (187 A.) Gulf of Suez—200 m. long, 30 m. broad.— It is supposed that the Israelites, pursued by Pharaoh and his hosts, crossed Red Sea (1491 B. C.), two miles from head of this gulf. Between Gulfs of Akabah and Suez, is mt. sinai, or jebel-hoosa ("Mouut of Moscs") — One of a cluster of mountains—where the ten commandments were given. Opinions differ as to which peak was the original Sinai (fig. 5.). (187B.) Str. of Bab-el-Man'deb O'gate of tear^') so called from the number of vessels, formerly wrecked in passing through it—distance between Asia and Africa, at this point, about 20 miles. (188.) Coast of Africa, around C. of Good Hope, from Red Sea to St. of Gibraltar (je-brawP- ter). — red sea, (out of Eed Sea again by Str. of Bab- el-Mandeb and G. of Aden) Mozambique channel (mo-zam-beek') with mouth of zambeze (zahm-bay'- ze) (E. 3) — delagoa b., (round C. of Good Hope) g. of guinea (ghin'-nee) with mouth of niger (ni'-jer) (E. 3 — E. from Eed Sea) — bight of biafra (be-af'ra), bight of renin (ben-een') str. of Gibral¬ tar. (E. 3 — How many from Eed Sea? E. 9 — Eead from Behring Str.). (189.) From Str. of Gibraltar to Behring Str. (along W. coast of Europe and N. coasts of Europe and Asia — PI. II).—str. of Gibraltar, b. of bis'cay, british channel (E. 3)—str. of dover, north or german sea, zuyder-zee (zl-der-zee), or south water divisions. 91 SEA (for latter Pl. VI. B. — R, 3. — R. from Str. of Gibraltar) — in North Sea: mouths of ehine, wesbr (wee'-ser), elbe (elb) (R. 3 — R. from Str. of Gibraltar) — baltic sea, with mouths of oder, vis'tula, niemen (nee'-men) and duna (R. 5 — R. from Str. Gibraltar) — white sea with dwina (dwee'na), spitz¬ beugen or barentz sea (between Is. of Spitzbergen and Nova Zembla), g. of ob or obi (o'-bee) with obi r. (R. 5 — R. from Str. of Gibraltar)—kara'sea, with mouth of yenisei (yen-e-say'e). Asiatic po¬ lar sea with mouth of lena r. (R. é—R. from Gibraltar) — polynia, or ice-free sea, behring str. (R. 2 — How many from Str. of Gibraltar^ R. 25. How many from Behring Str. to Behring Str.? Teacher apply rule 185 A. R. those 66. What were the starting- points for E. Continent? behring str.—str. of Ma¬ lacca—red sea —str. of gibraltar—and behring str. again. How many? 4. How many times too often was each one counted? Twice. How many names did we actually read? 62. Please prove it from the map. The teacher will now require the class to read the waterdivisions over again from PI. HI, then from PI. IV, then from PI. V, then from PI. VI. B; care¬ fully pointing out the objects. (189 A.) North or German Sea, often incorrectly called German Ocean. (189 B.) Zvyder-Zee, dutch zoider, "south", in contra¬ distinction to North Sea with which it is connected. (190.) Seven Seas and Lakes. — (Name seven seas and lakes almost in a line, E. and W., with Str. of Gibraltar), mediterranean sea, with mouths of rhone, po, and nile (R. 4)—black sea, with mouths of danube, pruth (prooth), dniester (nees'- ter), dnieper (nee'-per) (R. 5 — R. from Mediterranean) — sea of az'of, with mouth of don (R. 2 — R. from Mediterranean) — Caspian sea, with mouths 92 physical geography. volga and ural (yoo'-ral) (B. 3 — jB. from Medi¬ terranean)—a. of aral (ar'-al), with mouths of amoo-daria (Oxus) and sir-daria (j ax artes) (jax- ar'-teez) (R. 3 —from Mediterranean) — l.balkash, l. baikal (bî-kal). {R. 2. — How many from Mediterranean to L. Baikal? 19. How many waterdimsions of E. Continent have we now learned without giving any name twice? (Apply rule 185 A.). Answer will be 81. Now read aloud those 81 names from PI. IL). Remark. The class is notified, there has been an error in counting which will be corrected hereafter. (190 A.) Sir or Syr-Daria—Amoo-Daria — Daria, the tartar word for river. Oxus — Jaxartes, the ancient names. (190B.) We now go back and consider the subdivisions of the waters of Mediterranean, Black and Baltic Seas, and of Great Britain and Ireland (191.) Water sub-divisions of Mediterranean and Blaek Seas (without river-mouths) (PI. II. fig. 5). str. of gibraltar, g. of lions, g. of genoa (jen'o-a). (R. 3) — str. of Bonifacio (bo-ne- fah'cho), tyrrhenian (tir-recn'ian), sometimes Tuscan sea (between Italy and Corsica, Sardinia and Sicily, B. of naples (R. 3 — R. from Str. of Gibraltar) — str. of messina (mes- see'nah) (ancient Scylla and Charybdis, Adriatic sea (ad-re-at'ic) or g. of Venice (ven'-iss), str. of otran'to (shortest distance between Italy and Turkey) — (R. 3 — R. from Str. of Gibraltar) — g. of ta'ranto (hollow of Italy's foot), ionian sea (T-o'-ne-an), g. of cor'inth or lepan'to (R. 3 — R. from Str. of Gibraltar) — aegean sea (e-jee'-an) or grecian archipelago (ar-ke-pel'a-go), g. of sa¬ lonica (sa-lo-nee'-ka), g. of Smyrna (R. 3 — R. from Str. of Gibraltar) — Dardanelles (dar-da-nelz'), or hellespont, sea of mar'mora, str. of constan¬ tinople (kon-stan-te-no'pl), or bos'phorus (R. 3 — R. from Str. of Gibraltar.) — For next 3, PI. HI. water d1vi8iok8. 93 fig. 1.} black sea, str. OF kertch OF yenikale (jen -e• kah'-le), sea of az'OF (R. 3 — R. from Str. of Gibraltar. — Now back again to african coast. PI. II. fig. 5.) G. OP siD'ra, G. OF cabes (kahb'es), G. OF aegina (e-jee'-na), or athens (ath'-enz—for last. PI. VI. B.~R 3. — How many from Str. of Gibraltar^ R. 24). Remark. G. of Lions (not Lyons, as that town lies far distant) has its name from the violent storms and waves which frequently cause it to swallow the ship as a lion his prey. Some geographers give it Gulf of the Lion. (192.) Levant. — E. coasts and waters of Mediterra¬ nean are often called the Levant—an Italian term, meaning the "East"; more particularly applied to Turkey, Syria, Asia Minor, Greece, Egypt, etc. (193.) Scylla and Charybdis (in Sir. of Messina) the terror of ancient mariners, and dangerous even to the modern pilot. Charybdis (PI. V. B. fig. 2.)—an eddy or current on the Sicilian side, just outside harbor of Messina — 500 to 1000 feet deep — less the appearance of a whirl¬ pool than a current which sweeps the ship rapidly along —in bad weather, heavy waves and winds render steering almost impossible — when favored by a south wind, a ship, escaping Charybdis, is in danger of being dashed to pieces against Scylla (coast of Italy, N. entrance of the strait). This is a high, precipitous rock, about 9 sea miles distant — by the action of the waters worn, at its base, into hollow cavities, connected with each other, through which the floods rush with a roar said sometimes to resemble the barking of dogs — between principal rock and eddy, a number of other rocks, reefs and whirlpools — the strait, 20 miles in length, offers 23 good anchorages. In the course of ages, the waters have worn away masses of rock, and artificial means have been employed to render the navigation less formidable. The experienced pilot, choosing wind and time, may sail safely through Charybdis and find fishing boats lying quietly under the shadow of Scylla. But, in strong winds, no anchor, it is said, can hold against the stream. 94 physical geography. (194.) Water divisions of Baltic (without river-mouths (PI. III. fig. 4). — Skagerrack, cat'tegat, sound (B. 3) little belt, great belt, (Pi. v.), g. of dantzig (dant'-sio). (E. 8 R. from Skager Rack) — o. of riga (ree'-ga), g. of finland, G. of bothnia (both'-ne - a). (R. 3 — How many from Skager Rack? R. 9—R. water divisions of Mediterranean and Baltic. How many? R. 33). (195.) Waters of Great Britain and Ireland (Pi. VI. B). — murray frith, frith of forth, mouth of humber (R. 3) — THE wash, mouth of thames (temz), str. of dover (R. 3 — R. from Mur¬ ray Frith) — british channel, estuary of south¬ ampton, portsmouth harbor (R. 3 — R. from Mur¬ ray Frith) — plymouth sound, bristol channel st. george's channel (R. 3 — R. from Murray Frith) — cardigan b. (kar'-de-gan), menai str. (men'- ny), irish sea (R. 3.—R. from Murray Frith) — north channel, frith of clyde (kllde), the minch (R. 3 — R. from Murray Frith) — galway b. (gawl'- way — Ireland). (How many from Murray Frith? R. 19. — How many have you read altogether in Mediterranean, Black and Baltic Seas, and in waters of Gr. Britain and Ireland? R. 52. How many of these 52 names had been counted before? Three, namely Str. of Gibraltar, British Channel, Str. of Dover. Read these 49 names from PL III). (195 A.) Remark. Portsmouth harbor (PI. VI. B) — unequalled in the kingdom — fortress considered impreg¬ nable— head-quarters of British navy — a secure shelter for nearly whole fleet at same time — opens into celebrated roadstead (162), called spithead, where vessels in the Channel, during a storm, find a convenient asylum. (196.) Water divisions of Oceania (PI. II). — JAVA SEA (jah'-va), STR. OF SUNDA, BANDA SEA (R. 3) — TORRES STR., CARPENTARIA G. (kar-pen-tah're-a), water divisions. 95 moreton b. (R. 3 — R. from Java Sea) — bot'any b., bass str., great australian bight. (R. 3 — How many from Java Sea! R. 9). (197.) Water divisions of Antarctic Conti¬ nent (PI. II). — Begin with Bransfield Str., near C. Horn. One of the class will please to pass around Antarctic Continent in a circle from W. to E. and read water divisions on PI. II.—bransfield str., near C. Horn, george iv sea, repulse b., porpoise b., disappointment b. (R. 5. — Please point these out on PI. I. K. M.). (197 A.) The mouths of how many rivers thus far learned'! (Rule 185 A — R. 4:5). — Mackenzie, Sas¬ katchewan or nelson r., st. lawrence, potomac, mississippi, amazon, la plata, colorado, colum¬ bia, kwichpack, amoor, hoang-ho, yang-tse- kiang, canton, ganges, indus, tigris and euphra¬ tes, zambeze, niger, rhine, weser, elbe, oder, vistula, niemen, duna, obi, dwina, yenisei, lena, rhone, po, nile, danube, prúth, dniester, dnie¬ per, don, volga, ural, sir-daria, amoo-daria, humber, thames. (197B.) Remark to teacher. Let class have ample time silently to examine map before replying to each of follow¬ ing questions. Names to be all counted including repe¬ titions of starting-points, etc. Questions-. How many water divisions of W. Continent were given? 58. — How many seas and lakes in a line with Mediterranean including river-mouths? 19.— How many subdivisions of Mediterranean and Black Seas without river- mouths? 24. — How many subdivisions of Baltic without river-mouths? 9.— How many waterdivisions of Great Britain and Ireland? 19. — How many waterdivisions of E. Continent from Behring Str. to Behring Str. (excluding those of 7 seas and lakes, of Baltic, and of Gr. Britain and Ireland; but taking in British Channel and Str. of Dover?) 66. — How many waterdivisions of E. Continent altogether, with river-mouths? 137. — How many water- divisions of Oceania? 9.— How many of Antarctic Continent? 96 physical geography. 5. — How many of E. Hemispbere altogether? 151. — How many waterdivisions of whole globe have we named? 209. — How many of these names have been counted more than once? To guide the teacher. For following names counted more than once, deduct — for Behring Str., 3;—. Belle Isle, 1—Mosquito B., 1—Panama B., 1—Str. of Malacca, 1 — Bed Sea, 1—Str. of Dover, 1 — British Channel, 1—Str. of Gibraltar, 2 — Behring Sea or Sea of Kamtchatka, 1. Thirteen must be deducted from two hundred and nine. Ileal number of names, 196. The error, referred to at end of sec. 190, is the double counting of Behring Str. and Behring Sea or Sea of Kamtchatka, which were counted among divisions of W. Continent, and again among divisions of E. Continent. Point 196 out on Pis. III. and IV. (197C.) Remark. The review - lessons on Pis. III. and IV, to be carefully repeated. The advantage of a clear, universal outline far more than counterbalances the time required. We present only a general statement of geograph¬ ical facts. But that statement ought to be as completely learned, and as permanently retained through life, as the multiplication table or the alphabet. LAKES. (plate ii.) (198.) (W: Continent.) Remark a line of fresh water lakes, running in a S. E. direction, through N. America, from Arctic to Atlantic. One, called Great Salt Lake, lies apart to the S. W. among Rocky Mts. We name these by fives. (199.) Lakes of N. America. — (E. of Rocky Mts.) great bear lake, great slave lake, atha- ba'sca lake, lake win'hepeg, lake of the woods (R. Ö) — l. superior, l. michigan (mish'e-gan), l. huron, l. erie, l. ontario (on-ta're-o^—between two last, Falls of Niagara. — R. 5. — E. from Great Bear L.—Lastly, apart, and among Rocky Mts., 4200 feet above sea) great salt lake. — (How many? R. 11.) 'Remark. Lakes Superior, Michigan, Huron, Erie, Ontario pour their surplus waters into Atlantic by the river st. lawrence. lakes. 97 (200.) Lakes of Central America. — nicara^ «ua lake. — (How many from Great Bear Lake7 B. 12.) (201.) Lakes of S. America. — lake titicaca (te-te-kah'-kah), (one of the most elevated of the world'. 11,540 feet above the sea. — How many from Great Bear Lakel B. 13. — Point them out on PI. III., then on PI. IV.) (202.) (E. Continent.) Lakes of Europe. — Of twenty or thirty most prominent, we here name only three, l. wener (way'-ner—Scandinavian Peninsula). lakes ladoga (lah-do'-gah) and one'ga (between Baltic and White Seas. — B. 3. — B. from Great Bear Lake). Bemark. Near the latter, observe other lakes; the names however are of no importance. The adjoining territory, Russian provincp of Finland, is nearly covered with water, forming an immense system of lakes and marshes. There is reason to believe it was once the bottom of the Baltic (282 C). (203.) Lakes of Asia. — Although we have previously (190) read several inland waters of Asia, we here take them again. Caspian sea, sea of ar'al, L. balkash (B. 3.) l. baikal, l. tengui-n0r (ten'- gree-nor), the latter, among Himalaya Mts., highest in the world, 12,500 feet. (B. 5.—B. from L. Wener — then from Great Bear Lake). Remark. A small lake in Asia, the sir-i-kol (seer- ee-kol')—forming one of the sources of Amoo-Daria R., is said to be 15,600 feet above the sea. (204.) Lakes of Afric a. — l. melrhir, l. tsad, tsana or dembea (B. 3) — l. albert-n y anza Or lüt&, l. ukerewe (oo-ker-eh-we) or victoria-ny- anza, l. tanganyika (tahn-gahn-yee'ka) (B. 3.— B. from L. Melrhir) — l. nyas'si, l. ngami (n'gah'- mee) (B. 2. — How many from L. Melrhirl B. 8. — B. 7 98 physical geography. /roTO Caspian Sea — B. from L. Wener — R. from Great Bear Lake). Remark. The words Nyassi and Nyanza mean "lake" in the aboriginal dialect. L. Melrhir, also called Melgig, is salt and below the sea-level. (205.) Lakes of Australia. — lake eyre (air) — a salt lake. (How many from Great Bear Lake? R. 30. Point them out on PI. IV). (206.) Questions. — Define word Strait? (165). The teacher will first read and then cause pupil to repeat definition; then, to give examples. Channel? (166) — Sound? (167)—Belt? (168)—Lake? (169) —Bight? (161) — Bay? (160) —Gulf? (159)— Archipelago? (156)—Sea? (155) —Estuary? (171) —Inlet? (179) —Frith? (171) — Eddy or Whirlpool? (177) — River? (170)—Water-shed? (139) — Basin? (140)—Marsh? (152 A) — Cataract? (173). At close, teacher read remark (180). ISLANDS. (plate n.) (207.) (W. Continent) — Arctic Archipelago, from Behring Str. to Str. of Belle Isle. — baring i., victoria i., king william i. (R. 3). — parry is. with melville i., north devon (R. 3.— Read from Behring Str.) — cockbdrn is., grinnell land, greenland (R. 3.—Read from Behring Str) — iceland. (How many from Behring Str.'t Read 10). Remark. Iceland (PI. II; also PI. 1. figs. I. H. L; also PI. IV) — lying nearer Greenland than European coast, is, by many geographers, included among american polar islands, although its population and civilisation are European.—Baring I. — sometimes Bank's Land-, Cockbum I.—sometimes Baffin's Land. islands. 99 (208.) From Str. of Belle Isle to Mosquito Bay. — NEWFOUNDLAND, ARCHIPELAGO OF ST. LAW¬ RENCE, LONG ISLAND (R. 3). BERMUDA Or SOMEUS IS.*, WEST INDIA IS. (R. 2. — R. from Behring Str.) (209.) From Mosquito B. to B. of Panama.—, marajo i. (mouth of Amazon), trinidad' i., Falk¬ land is. (fawk'-land), terra del fuego is. (fway'-go) (R. 4). — antarctic archipelago, consisting of south georgia, sandwich group, south orkney and south shetland is. (R. 5. — R. from Mosquito B.) — wellington is., chonos is. (ko'-nos—sometimes called Chonos Group or Chonos Archipelago), i. of CHiLOE (cheelo-â', almost cheel'-way) (R. 3. — R. from Mosquito B.)—i. of ju'an fernan'dez, chin'cha is., seal or lobos is. (R. 3. — R. from Mosquito B.) — galapagos (gah - lah - pah'-gos) or tortoise is. (How many from Mosquito Bayf R. 16.—R. from Behring Str.). (209 A.) Marojo I. ( or Johannes I.) — 450 m. in circumference — part elevated by volcanic action — part, by alluvial deposits brought down by the river. (210.) From B. of Panama to Behring Str. or Baring I. — REVILLA-GIGEDO (ra-veel'ya hee-hay- do), VANCOUVER I., QUEEN CHARLOTTE IS. (R. 3.) — prince of wales i., sitka i., kodiak i. (R. 3.— R. from B. of Panama) — Aleutian archipelago (a-loo'-she-an) orrox is., to Behring str. again, (".ß. 7. — How many islands of W. Continent^ R. 38. Point out their places on PI. JV). Let us now return to: (211.) West India Islands (PI. III. fig. 3). — Vast Archipelago — greater part between tropic of Cancer anc^lO"* N. parallel — some reaching more than 3® N. of that tropic and approaching within about 50 miles ♦ Scene of Shakspeare's Tempest, in one of these islands. 7* 100 physical geography. of Florida—extending, in two lines, somewhat in form of a crescent, from peninsulas of Yucatan and Florida to the mouth of Orinoco. They are said to be more than 1000 in number, but, except about 60, are barren islands or mere rocky islets. They are sometimes called Columbian Archipelago, from Co- "lumhus; Antilles (an-teel'), from being opposite to the continent; West hidies, because, when Columbus landed, he thought he had succeeded in finding part of Asia, or the East India Is. (212.) West India Islands divided (fig. 3) into: bahama (ba-hay'-ma), or lucayo is., (loo-kï'-o), greater antilles, lesser antilles, s. american coast is. (R- 4). (212 A.) Among bahama or lucayo is.,* are new providence, cat i. and watlings i. (ot san salvador or guanahani. (B. 3.—R. from Bahama Is.) Remark. The Bahama Is., of coral formation, are said to be about 500 in number — only 12 or 14 inhabited —the rest, mere rocks and sand-banks—many not even explored. On New Providence is the salubrious town and capital, Nassau. — Cat I, — sometimes, but erroneously, supposed to be the San Salvador of Columbus. — Watlings Is. or Guanahani, the real San Salvador, on which Colum¬ bus landed, A. D. 1492. (213.) Among Greater Antilles are: cuba with ISLE OP PINES, JAMAICA (R. 3.) — HAYTi (hay'-tee) or SAN DOMINGO, PORTO RICO (R. 5. — R. from Ba¬ hama Is.). (214.) Among Lesser Antilles are: virgin is., SANTA CRUZ (krOOs), ST. BARTHOLOMEW (R. 3.) — • * Bahama Is. or Bahamas. — One of a class of names which take an s when used alone: examples, Molucca Is. or Moluccas — Bermuda Is. or Bermudas — Lucayo Is. or Lucayos — Madeira Is. or Madeiras (Mah-deh'-rahs). islands. 101 guadeloupe (gaw - da-loop'), martinique, baebadoes (bar-bay'-does) (B. 3.—B. from Virgin Is.) — british trinidad, st. john st. Jan), st. thomas (B. 3. — Bead 9. Bead from Bahama Is.). (215.) Among Soatli American Coast Is. are: curaçoa (ku-ra-so'-a). (How many West India Is. have we read includinq the names of the four qreat divi¬ sions? B. 22.). (216.) West India Islands according to nationalities. — The West India Is. (except Hayti ■which is independent) belong to 8 Powers, namely: Spain, Gr. Britain, France, Denmark, Sweden, Vene¬ zuela, Holland, and the United States. Thus, with the exception of Hayti and the islands belonging to the United States, and Venezuela, they are entirely in the possession of European nations. Spain owns the larger portion: cuba, isle of pines, porto rico (B. 3.) — to Great Britain belong: Bahama is., jamai¬ ca, barbadoes, trinidad (B. 4.—B. from Cuba) to France-. Guadeloupe, Martinique (B. 2. — B. from Cuba) — to Denmark-, santa cruz (B. from Cuba) — to Sweden-, st. Bartholomew (B. from Cuba)—to Venezuela: part of s. American coast is. (B. from Cuba) — to Holland: curaçoa, etc. (B. from Cuba) — to United States: st. thomas, st. juan. (How many from Cuba? B. 15. — B. all West India Is.). (217.) Questions on West India Is. — To whom do the West India Is. belong? (216) — How are they divided? (212) — Among Greater Antilles (an-teel') are? (213). Among Lesser Antilles are? (214) — In what division is I. of Curaçoa? (215).—Name governments to which following Is. belong. Curaçoa? Holland. — St. Bartholomew? Sweden. — Santa Cruz (kroos)? Denmark. — Guadeloupe and Martinique? France. — Cuba? Spain. — Jamaica (ja-may'ka)? Great Britain. — Porto Bico? Spain. — Barbadoes? Gr. Britain. — Isle of Pines? Spain. 102 physical geography. — Trinidad (trin - e - dad') ? Gr. Britain. — St. Thomas and St. Juan"? United States. — (R. from PI. Ill, then from PL IV). (i2. all from Behring Str.). (217 A.) Windward or Leeward Is. {lee'-ward—often, particularly by sailors, pronounced lu'-urd). — The Spanish apply the term windward islands, that is, islands in the wind, or in the direction from which the wind comes, to the whole Lesser Antilles, because, from the eastern position of these islands, they first receive the trade wind. The South American Coast Is. are termed leeward islands, as lying away from the wind—toward the lee, or that part toward which the wind blows. When the wind blows a ship toward the shore, the latter is called a lee-shore. The English, and some american geographers, apply the terms windward and leeward to different portions of Lesser Antilles which are often also called Carihbee Is. (217B.) Remarks on W. India Islands. — Their history, from landing of Columbus till to-day, is peculiarly interesting. The Spaniards exterminated the aboriginal inhabitants of Hayti and introduced African slave-trade and negro-slavery. Since then earthquakes, shipwrecks, hurricanes (connected with currents and trade-winds, as is the case also in East Indies), the atrocities of buccaneers, etc., have followed each other in terrible succession. One of the most interesting events is the history of Toussaint L'Ouverture, the unfortunate hero of the I. of Hayti and finally victim of Napoleon I. (218.) (E. Continent.) From Behring Str. to Str. of Malacca (PI. II.). — kookil is., saghalien i. (sah-gab-lee'-en), island empire of japan (R. 3) — Empire of Japan consists principally of four large islands: yesso, niphon, sikoke (see-kok'), and kioo- sioo {R. i. — R. from Behring Str.) — lew chew is. (loo-choo), formosa i., britishi.ofhong-kong (R. 3. — R. from Behring Str.) — Portuguese i. of maoao (mah-cow'), Hain.an i. (hi-nahn'), singapore {Str. of Malacca). (How many from Behring Str.'i _ß. iß). islands. 103 (218 A.) L of Hung-kong — entrance of Canton R.— belonginjr to England — good road-steads and harbor —free from typhoons (violent tornadoes which sweep other Chinese waters) — as a colony of Gr. Britain on Chinese soil, a valuable and important position — head-quarters of her mercantile, military and naval establishments in that part of the world. Shortest sea voyage to London, 12,900 miles; shortest time, by sailing vessel, 102 days. (218B.) Macao — Portuguese I. and town at mouth of Canton R.—trade, tea and silk from interior, chiefly in hands of Americans and English. (218C.) Singapore ("city of the lion") — a small island off S. extremity of Malay peninsula—purchased, in 1819, by the English from the sultan of one of the insigniflcant Indian states — chiefly valuable as a depot (de-poh') for British and Indian trade with islands of the eastern sea — a vast system of fortifications is now in progress. Pop. about 80,000, among whom, 25,000 Chinese, 30,000 Malays and a few Europeans (A. K. Johnston). "According to a recent authority", says Lippencott, "tigers swarm in the jungles, sometimes carrying off a great number of persons annually". (219.) From Str. of Malacca to Red Sea. — andaman is., nic'-obar is., i. of ceylon (see'-lon) (R. 3.) — mal'dive i., lao'cadive is., i. of so co'tra (R. 6 — R. from Behring Str.). * (220.) From Red Sea, around África, to Str. of Gibraltar. — Seychelles is. (sâ-shel'), ami- rante is. (am-e-ranf), com'oro is., madagas'car i. (a kingdom — R. 4.) — mascarene' is., consisting of rodrigues (ro-dreeg'-ez), Mauritius (maw-rish'e-us) or isle of france, reunion (formerly Bourbon) (R. 4. — R. from Red Sea).— kerg'uelen land (kerg'-e-len), or i. oF desolation, Tristan da cunha (da-koon'-ya), st. helena (sent hel'-ee-na) (R. 3.— R. from Red Sea) — ascension, annobon' i., st. Thomas, fernando po i. (R. i. — R- from Red Sea) 104 FHYSICAL GEOGRAPHY. CAPE VERDE IS., CANA'RY IS., MADEIRA IS. (mah- deh'-rah) (R. 3.—R. from Red Sea) — .^z'ores is. (Hawks Is. in portuguese). (How many from Red Seat R. 19.—R. from Behring Str. — Point out four last on- PI. IV). (220 A.) Madagascar L — the inhabitants are of various races; some with the black skin and woolly hair of the negro; some mulattoes; and some resembling the Malays. The whole population is colored except about the one-twentieth part. "Their religion is a rude species of polytheistic idolatry, and the monarch is the high priest as well as the despotic ruler of his subjects. The prevailing language, called Malagasse, bears no resemblance to those of the opposite coast of Africa, but is very similar in construction and forms to the Tagala, the most perfect of Polynesian dialects. Christianity was introduced, for the first time, in 1818, and the Scriptures have since been translated into Malagasse. Under the late king, Radama, the missionaries were protected, civilization introduced, slave-trade abolished, and schools established; but since his death, a disastrous change has taken place. The profession of Christianity is prohibited under severe penalties, the missionaries expelled, and many of the converts massacred.* (220B.) Kerguelen Land — from the French navigator, who discovered it, A. D. 1772 — about 100 m. long—a mass of naked precipitous rocks and mountains, between 2 and 3000 f. high—inhabited only by sea birds, whales, etc. — surrounded by immense fragments of drifting ice— visited but by whale ships which find, amid the universal desolation, a good harbor and plenty of coal. (220 C.) St. Helena — a huge, volcanic mass of bazalt, partly covered with lava, partly with fertile soil— culminating point, nearly 3000 f.—population 6860, half negroes — climate, temperate. The emperor Napoleon I. confined here by British government, as a too persistent disturber of the peace of mankind —remained from 16 Oct. * Manual of Modern Geography by Rev. Alexander Mackay. Edinburg and London. — one of the best. islands. 105 1815 till his death, May 5, 1821. The island rises almost perpendicularly from the sea—striking; the beholder with astonishment and awe. "Almost impregnable from nature", says Daniel, "the British government has trans¬ formed it into a fortress more formidable than Gibraltar. Every height bristles with fortifications and canon." (220 D.) Tristan da Cunha — was taken possession of, in 1811, by Americans, but afterward abandoned. During the imprisonment of Napoleon I, it was occupied by the British government—at present the seat of a little, well behaved, industrious English population of 9 families or 85 persons, under protection of the governor of Cape Colony — an Episcopalian clergyman — climate, temperate — ships, plying between India and Australia, and not landing at the Cape, here stop for supply of water, etc.—the island well watered and said to be one of the healthiest places of the globe. (221.) From Str. of Gibraltar to Behring^ Str. (Pl. II). — british channel and irish sea is. (counted as one), Heligoland, british is. (i. e. gr. britain and Ireland) (R. 5)—Hebrides (heb'- rid-eez) or western is., Orkney is., shetland is. (R, 3 — R. from Sir. of Gibraltar) — faroe is. (fah'- ro, not to be confounded with Ferro I., the most south¬ west of Canary Is.) — lofoden i. (lof-fo'-den), Iceland (again) (R. 3. — R. from Str. of Gibraltar) — jan mayen i. (yan - mi'-en), Spitzbergen is., nova Zem¬ bla is. (R. 3. — R. from Sir. of Gibraltar) —new siberia is., herald i. (How many from Str. of Gi- braltarl R. 16). Remark. From Herald I. (Pis. II and IV) has been seen, in the distance, an unknown and unexplored coast with high peaks. (221 A.) Shetland I. — The ancients applied the name ultima thdle (ul-ti-mah thu'-le) to what they supposed the northernmost point of the habitable globe; according to some, Iceland-, to others, Norway, to others, with more probability, the largest of the Shetland Group. 106 PHTSICaL geogkapht. (222.) Mediterranean Is. (PL XL 5 —PL VI. B). — BALEAKic isles, Consisting of itiça (e tce'sah), Majorca, misorca (2. 4). — elba. Corsica, bar- disia (B. 3. — B. from Bakarie Is.) — Note, dose to Naples, isCHiA and capri (is'-ke-«) ("ß. 2. — B. from Balearic Is.) — lipari is. (lee-pah're), sicilt, malta (B. 3.—B. from Balearic Is)—iosiab is. (i-o'ne-Ao) and crecias archipelago (B. 2. — B. from BaUarie 3s.) — caspia or crete, rhodes (rod*), ctprcs Give an example or two of some objects whose contiguity, in the planisphere map (PL II), is awkwardly interrupted by the diverging circumferences of the two hemispheres? — Iceland. It is quite cut in two. Kamtchatka. Indeed all the points, bordering on the circumference of one hemisphere, are separated from corresponding points, bordering on the circumference of the other hemisphere. POLITICAL GEOGRAPHY. 181 ■with -which they ought to be connected. Not only the contiguity, but also, of course, the proximity is inter¬ rupted. Places, near to each other, are made to appear remote; for instance. New Zealand and Australia—Japan and Aliaska. The Antarctic Continent, whioh ought to be one figure, a huge ice-mass, is cut in two ; and the fragments recede so far away from each other that we can scarcely bear in mind their contiguity. Polynesia, Australasia, the Tchooktchee P., are also awkwardly separated; the Azores (PI. IV), opposite Lisbon, near Madeira, are made to recede from both; while Greenland, comparatively near Scotland and Ireland, looks more remote than the G. of Good Hope. Among other distortions, are the Atlantic and Pacific — particularly the former. The appearance presents a per¬ petual puzzle to the young student endeavoring to trace a voyage from New York to London. (442.) Kercator's Projection (PI. IV.) — was intro¬ duced by Mercator (mer-ca'-tor), in 1556, for the particular convenience of mariners. It is also called the Cylindrical Projection, because it is drawn as if the earth were shaped like a cylinder, as in PI. VIII. O. A cylinder, in Geometry, is a long, circular body, of uniform diameter, its extremities forming equal parallel circles. If the earth were shaped so, its surface, unrolled, would appear like PL IV;—the tropics of Capricorn and Cancer—the arctic and antarctic circles—the parallel of latitude at the pole — and all the other parallels, would be as large as the equator. The degrees upon each, therefore, would be of the same length. — But the earth is not shaped so. Hence the disadvantage of this map is that, among other peculiarities, the length of the degrees of longitude, and those of latitude, are exag¬ gerated toward the poles; and the relative magnitudes of the polar regions and the objects near them, as compared with those near the equator, are larger than they ought to be. Greenland, Sweden, Norway, British America, Asia (PI. IV), will strike your eye as shapes different from those in Pis. I. II. III. Bearing this in mind, so as not to fall into an error as to the relative dimensions of places in the polar and equatorial regions, the Mercator projection is useful in several respects. It may be safely consulted in connection -with the planispheres; for the errors of the two projections ccrrecl each other. We see the earth's entire 182 VOYAGES. surface at one view. No diverging circumferences interrupt the contiguity, or distort the proximity, of places. The disjoined pieces of Iceland and Kamtchatka—the Atlantic and Pacific—Polynesia and Australasia—re-appear in their natural entireness. We see New Zealand, close to Australia, in its right place, and regular gradation between C. of Good Hope and S. Pole (433,ninth paragraph). The eye follows with pleasure every unbroken outline, and traces the rela¬ tive position of every point—of Kamtchatka and Behring Str. — Tchooktchee P. and Japan — Iceland, Greenland, Norway and Great Britain — New York and London—the Azores and Madeiras—the La Plata and 0. of Good Hope. The youngest schoolboy can go, in imagination, from New York to London, without embarrassment. We have, therefore, chosen the Mercator projection for the following imaginary voyages to different countries and towns of the world, although it will often be found useful to refer to Plates I. IL III. (443.) It would not be an easy task to cross all the regions and visit all the points of the globe. We should meet a variety of obstacles not always surmountable. Some¬ times we should find ourselves among populations speaking languages quite unintelligible—in lands desolated by wars —in oceans blocked up with ice — in burning deserts or frozen steppes, where neither animal nor man can resist the winter storm or the summer drought—in places atifiicted with pestilence or malaria — seas infested with cruel pirates or embarrassed by dangerous marine vegetation—savage districts or islands where we incur the peril, not only of being murdered, but of being eaten by our fellow-beings. Magellan, who gave his name to the Strait, was killed (1521), by the savages of the Philippine Is. Cook was massacred by the natives of the Sandwich Is. (1779). An interesting young Prussian savant, Mr. Schlagintweit, after crossing the Himalaya Mts., from Calcutta to Lhassa (Pis. IV and III), was seized, by the fanatic chief of a Turkish tribe, and beheaded (1857). (444.) Voyage from Kew York to Nishnei-Hovgorod. — Bemark. 1. As it is not the object of these voyage- lessons to convey instruction concerning present routes of tr.avel, steamships, railroads, etc., we do not always choose POLITICAL GEOGRAPHY. 183 the most direct way. 2. Degrees of latitude and longitude, miles, etc., are given without fractions. Point out Nishnei-Novgorod (nizh'-nee). Go to it by Gibraltar.—In what country? Russia in Europe.—In what direction from New York? North-east.—Longitude of New York? 74° W. from Greenwich.— Longitude of Nishnei-Novgorod? 44° E.—How many degrees is Nishnei-Novgorod E. of New-York? 118°.—Latitude of New York? 41°. — Latitude of Novgorod? 56°.—How many degrees does Novgorod lie N. of New York? 15°.— Bound Russia in Europe (Plates IV and III). N. by a part of Sweden, White Sea and Arctic Ocean; E. by Russia in Asia or Siberia and Caspian Sea; S. by Caspian Sea, Persia, Turkey in Asia, Black Sea, Roumania, Austria; W. by Black Sea, Rou- mania, Austria, Germany, Baltic and Sweden.— In what zone lies Russia in Europe? N. temperate and north frigid.—What is the northernmost parallel of Russia in Europe? About 70°. — Conditions of day, night and seasons on that parallel? Longest day, two months; longest night, of course, tbe same. (See Explanation, at left, of PI. IV ; also Text-Book 93 and 94). It thus lies far within arctic circle and the region of intense polar cold. The southernmost parallel ? 3 9 ". Conditions of day, night and seasons on this parallel? Longest day and, of course, longest night—about 15 hours: —not very different from the day and night of Boston and New York. What countries or places lie on that northern seventieth parallel, going E. around the world? Russia in Asia — Russian America — Unoccupied Arctic Lands—Baffin Bay—Greenland—northern part of Norway and Sweden.—What countries or places lie on, or near, the southernmost parallel, going E. around the world? Russia in Asia—Western Tartary or Toorkistan — Chinese Empire—Kingdom of Corea—Empire of Japan—the United States—Portugal — Spain Italy (Rome, Naples) — Greece—Turkey in Asia.— In going from New York to Novgorod, what waters do yon pass through or near? E. across Atlantic—then (Pl. H. fig. 5) — Str. of Gibraltar—G. of Lions — G. of Genoa — Tyrrhenian Sea — Str. of Messina (Scylla and Charybdis)—Ionian Sea — Adriatic Sea — Levant(191)—Aegean Sea or Grecian Archipelago 184 voyages. — Str. Dardanelles or Hellespont — Sea Marmora — Str. of Constantinople or Bosphorus—(now PI. III. Fig. 1)—Black Sea—Str. of Kertch or Yenikale — Sea of Azof—(now PI. IV)—up river Don, cross canal to Volga (largest river in Europe), to Novgorod. — What countries have yon coasted, on your left? Portugal — Spain — France —Italy —Austria — Turkey in Europe — Greece—Turkey in Europe again—a small part of the coast of Roumania — Black Sea — then Russia in Europe. — What countries did you pass on your right? Morocco — Algeria—Tunis — Tripoli with Barca and Fezzan —Egypt—Turkey in Asia (including Palestine or the Holy Land).—The mouths of what great rivers have you passed on your left? Guadalquivir — Ebro — Rhone — Po — Danube — Dniester— Dnieper and Don.—The mouth of what great river on your right? The Nile.—Name towns you passed on, or near, your left? Cadiz — Granada — Marseilles — Rome — Naples —Palermo — Athens—Constantinople—Odessa— Sebastople.—Name towns on your right. Tangier s — Algiers—Constantino — Tunis— Cabes—Tripoli — Alexandria — Cairo — Rosetta — Jerusalem — St. Jean D'Acre —Beiruth — Damascus — Aleppo — Smyrna — Trebizond — Kazan — Novgorod. — On what sea, lake or river stand the following towns? Mar¬ seilles? On G. of Lions.—Constantinople? On Strait of Constantinople or Bosphorus, near Black Sea.— Trebizond? On Black Sea.—Smyrna? On Aegean Sea or Grecian Archipelago.—Alexandria? Rosetta? Cairo? On Nile.—Beiruth? St. Jean D'Acre? On Mediterra¬ nean.— Read rivers of Russia in Europe, beginning with Volga, going W. and N. around. — Volga — Don — Dnieper— Dniester —Prnth—Niemen (nee'-men) — Duna — Dwina—Petchora. Read towns of Russia in Europe. — Nishnei-Novgorod — Kazan — Moscow — Astrachan— Sebastople—Odessa—Kiev—Warsaw — Riga —Reval — St. Petersburg — Archangel — Tornea. On what sea, lake or river stand the following towns? Astrachan? On Volga and Caspian Sea.— Archangel? On White Sea.—Tornea? On Baltic.—St. Petersburg? On Neva R. and G. of Finland.—Reval? Riga? On Baltic.—Warsaw? On Vistula.—Kiev? (Kief) POLITICAL GEOGRAPHY. 185 On Dnieper. — Nishnei-Novgorod? At the confluence of Oka with Volga. (445.) Nish nei-Novgorod. — This town, beside being a great center of trade between Europe and Asia, interests the traveler as the seat of the largest fair in the world. From 2 to 300,000 (and sometimes more) Europeans and Asiatics are collected; sales of wares and products take place, to the amount of a hundred million dollars, within about eight weeks. There, mingle in the immense crowd, the long-bearded Russian tradesman, the Greek, with his beautiful costume of scarlet and white, the Tartar, the Turk, the Jew, the Persian, the Chinese, the Indian, the Mongol, the Thibet merchant, and the agent of the Russian American Fur-Company, with rich furs — brilliant, fiery fox skins — precious ermines of Yakootsk—splendid sables, etc. For these wares, so much prized by the princes and nobles of Turkey, Persia and Russia, the fur merchant receives hundreds of thousands of dollars. (446.) From Nishnei • Novgorod to Fetropanlovsk (sometimes written PetTopaulovski —pe-tro-pow-lof'skee) by Irkutsk and Nicolajefsk. Point out Petropaulovsk.—In what country? Russia in Asia.—In what direction from Nishnei-Novgorod? Nearly E.—Longitude of Nishnei- Novgorod? 44° E. from Greenwich.—Longitude of Petropaulovsk? 159® E.—How many degrees is Petro¬ paulovsk distant from Nishnei-Novgorod? 115°. — Lati¬ tude of Nishnei-Novgorod? 56° N.—How many degrees lies Petropaulovsk S. of Novgorod ? 3 ° S. —Bound Russia in Asia. N. by Arctic Ocean; E. by Arctic Ocean, Behring Str., separating from Russian America, and by Pacific; S. by Pacific, Chinese Empire, Western Tartary or Toorkistan, Persia; W. by Caspian Sea, Europe, Ural river, Ural Mts. and Arctic Ocean. — In what zones lies Russia in Asia? N. temperate and N. frigid zones.—What is the northern¬ most parallel of Russia in Asia? 7 8°.— Conditions of day, night, climate, etc., in places on that parallel? About 4 months uninterrupted day in summer, the same night in winter; of course polar cold and ever¬ lasting ice.—What is the southernmost parallel of Russia in Asia? 38° N.—Conditions of day and night in places 186 VOYAGES, on that parallel? About 15 hours day in summer, the same night in winter, much the same as in New-York. — What towns, countries or places lie on, or near, that northernmost parallel going E. around the world? Grinnell Land—Smith Strait—Greenland—Spitz¬ bergen.—What towns, countries or places lie on, or near, that southernmost parallel going E. around the world? Persia—Western Tartary or Toorkistan — part of the Afghan States—Chinese Empire — kingdom of Corea—Niphon (the principal island of Japan) — San Francisco—Sacra.mento — St. Louis—Louis¬ ville—Philadelphia—and Washington.—What coun¬ tries, mountains, lakes, seas, interesting regions do you pass through, or near, in coming from Nishnei-Novgorod to Pe- tropaulovsk? Ural Mts. — Lake Baikal — Sea of Okhotsk.—What great rivers have you passed? , Irtish —Ob (Obi)—Yenisei, with its branch Toongooska or Angara — Lena.—By what towns did you pass? Kasan —Tobolsk — Barnaul — Krasnoyarsk —Ir- kootsk — Kiakhta, adjoining the Chinese town Maimatchin — Nicolajefsk—to Petropaulovsk.— Read the rivers of Russia in Asia. Obi, with its branch Irtish—Yenisei, with Toongooska or Angara—Lena—Kolyma and Amoor. — Read towns of Russia in Asia? Tobolsk—Barnaul—Krasnoyarsk — Irkootsk— Kiakhta — Nicolajefsk — Petropau¬ lovsk— Okhotsk —Yakootsk — Nishnei-Kolymsk — Olensk. — On what sea, lake or river stand following towns in Siberia or Russia in Asia? Tobolsk? On Irtish.— Barnaul? On Obi.—Krasnoyarsk? On Yenisei.—Irkootsk? On Toongooska or Angara (branch of Yenisei).— Yakootsk? On Lena. — Nicolajefsk? On Amoor.— Nishnei-Kolymsk? On Kolyma. (447.) Irkootsk — nearly 4000 miles from St. Peters¬ burg and 1400 miles from Peking — is almost in the center of Asia, where one would least suppose New York and Paris fashions and comforts. Yet, so rapidly is the world changing under the influence of telegraphs, railroads and steamships, that the traveler will find it, in many respects, resembling the towns of western Europe — a theatre, schools, a library, 19 churches, a seminary, an orphan asylum, manu¬ factures, etc. It is the great center of the Russian-Chinese POLITICAL GEOGRAPHY. 187 trade, with an increasing population of about 25,000, and be¬ tween 2 and 3000 houses. It is the administrative seat of government of the Russian Empire, for all affairs connected with the fleet and marine establishment of the Pacific Ocean; as it has been for Russian American Fur-Company, till the late purchase (523). (448.) Nikolaje/sk — on Amoor R. Here we shall find a modern Russian town and fortified military post, several hundred blockhouses, a new handsome church with a lofty tower, many government buildings, a museum, an observatory, a library of 4000 volumes, many schools, and a brisk trade. The principal european newspapers have sub¬ scribers here. It is a station of the Russian fleet and may become an important point of communication with California. The Russian steamers ply up the River Amoor, on which it stands. The cold is, however, intense and the river is frozen many months of the year. Remark. We will not extend our journey to the cheerless region of northern Siberia — to Olensk, the northernmost town of the Russian Empire—nor to Nishnei- Kolymsk, upon the Kolima River, the coldest point of Russia, where the summer breezes, although they bring millions of mosquitoes, are mingled with snow; while in January the thermometer falls to 40° R. (58° F). (449.) Peti'opaulovsk — capital town of Kamtchatka— principal station of Russian government in this part of the world — population, about 1000 — harbor, formed by a tongue of land, one of the most beautiful and secure upon the earth—by Aleutian Is. closely connected with the Russian Territory, now part of the U. States. (450.) ïrom Fetropanlovsk to Kew York. — Go by New Archangel — San Francisco — Panama—Aspinwall — New Orleans and Key West. — Point out New York.— In what direction from Petropaulovsk? S. E.—-Longitude of Petropaulovsk? 159° E. from Greenwich,—Longitude of New York?7 4° W. — How many degrees does New York lie E. of Petropaulovsk ? 124°. — Latitude of Petro¬ paulovsk? 53° N.— Latitude of New York? About 41° N. — How many degrees does New York lie N. or S. 188 voyages. of Petropaulovsk? 12® S. — Bonnd United States of America. N. by British America; E. by British America, Atlantic, G. of Mexico; S. by Atlantic, G. of Mexico, Mexico; W. by Mexico and Pacific. —In what zone lie the United States? Altogether in the N. temperate zone, but much nearer the torrid than the frigid zone.—Northernmost parallel of United States? 49® N.— Conditions of day, night, climate, etc., on that parallel? 16 honrs longest day and longest night.—Southernmost parallel of the United States? 25® N. — Conditions of day, night, climate, etc., on that parallel? Between 13 and 14 hours longest night, etc. Remark. While the northern parallel sensibly ap¬ proaches the character of the frigid zone, the southern parallel is almost identical with tropic of Cancer. The winters of the North, therefore, are long and severe, while the southern states have a tropical climate. It is to be observed, however, that climate does not exclusively depend on latitude, but is modified by other circumstances; as, for instance, elevation, the ocean, mountains, northern or southern slope, geological character of the surface, winds, etc.—What towns, countries or places lie on, ornear, that northernmost parallel going E. around the world? Quebec — St. John — Newfoundland — Paris — Munich— Vienna — Odessa — Maimatchin — Eiakhta — and Victoria (on Vancouver I.).—What towns, countries or places lie on, or near, the southernmost parallel, going E. around the world? Canary Is.—desert of Sahara — Insalah — Mourzouk — Assouan — Ruins of Thebes — Medina — er-Riad — Muscat —Kelat — Curr achee —Luck now — Calcutta —Canton —Sand¬ wich Is.—What waters do you pass through, or near, from Petropaulovsk to New York? Pacific —then crossing Isthmus of Darien or Panama—B. of Darien—Mosquito B. — Caribbean Sea—B. ofHon- duras—G. of Mexico and Atlantic.—What countries have you passed on your left? Russia in Asia or Si¬ beria— Russian America — British America — United States of America—Mexico—republics of Central America, namely: Guatemala—St. Salvador — Honduras — Nicaragua—and Costa Rica — and that part of the Isthmus belonging to the United POLITICAL GEOGRAPHY. 189 States of Columbia, then crossing the Isthmus, through territory of Columbia, we pass Costa Kica again, Nicaragua—Mosquito Coast—Hon¬ duras — Guatemala — Balize or British Hon¬ duras—Mexico—United States, to New York.—What countries have you passed on your right? Colombia— Hayti and republic of San Domingo. — The mouths of what great rivers have you passed on your left? Kwickpack or Yucon — Frazer — Columbia—Colo¬ rado— Rio Grande del Norte—Mississippi—Hud¬ son.—Name the towns on, or near the coast, you have passed on your left? New Archangel—New West¬ minster— Victoria — Olympia — Oregon City — Sa¬ lem — San Francisco — Sacramento — Mazatlan — Guatemala—San Salvador—Panama—A spin wall— San Juan de Nicaragua or Greytown — Bluefields —Vera Cruz— Mexico—Matam or as— Brownsville — Galveston—New Orleans — Mobile — Key West — St. Augustin—Savannah—Charleston-^Wilming- ton—Richmond—Washington—Baltimore — Phil¬ adelphia to New York.—Name towns on or near, the coast, you have passed on your right? Guayaquil— Quito — Bogota— Kingston — Havana — Port au Prince. — On what lake, river, or other waters stand the following towns? New Orleans? On Mississippi, near its mouth.—Vicksburg? On Mississippi.—Louis¬ ville? On Ohio.—Cincinnati? On Ohio.—Milwaukee? On L, Michigan. — Chicago? On L. Michigan.—Detroit? Cleveland? Bufialo? On L. Erie. — Read from map great rivers of N. America (285)—Towns of United States.—What towns stand on the following rivers, lakes and other waters? On Sacramento R.? Sacramento City (329). — On Rio Grande del Norte? Brownsville (United States), oppo¬ site Matamoras (Mexico).—On Mississippi? New Orleans — Baton Rouge—Vicksburg—Memphis—St. Louis. — On Ohio? Louisville—Cincinnati. — On Potomac? Washington.—On, or near, Chesapeake B.? Richmond — Baltimore.—On Hudson and East Rivers? New York. — On L. Erie? Buffalo — Cleveland — Detroit. — On L. Michigan? Chicago — Milwaukee. (451.J We have now circumnavigated the globe. It would be useless to describe more voyages. The teacher 190 VOYAGE». may lead the pupil, from one point to another, according to hi.s" discretion (see table of questions (453). We suggest a few voyages, particularly for the aid of young persons, who, it is believed, will often be found competent teachers of this work, (452.) Several plans of voyages. — 1. From New York, by C. of Good Hope, to Malacca. — 2. Malacca, by Red Sea, to London. — 3. London, by C. of Good Hope and Calcutta, to Lassa. — 4. Lassa, by Sea of Azof, to Moscow and St. Petersburg. — 5. St. Petersburg, by Rei- kiavik, to Godthaab.— 6. Godthaab, by Cape Horn, to Pa¬ nama.— 7. Panama to Hobart Town. — 8. Hobart Town, by Batavia, to Rangoon.— 9. Rangoon, by Cape Town to C. Horn. —10. C. Horn to Honolulu. —11. Honolulu, by Cook Str. (New Zealand), to Wellington.—12. Wellington to Manilla. —13. Manilla to Yeddo.—14. Yeddo to Antananarivo.— 15. Kouka to Massouah.—16. Massouah to Jerusalem.— 17. Jerusalem to Paris. —19. Paris, by Trieste, Athens, Cairo, to Hurrur.— 20. From Hurrur, by Hobart Town, to San Fran¬ cisco and Great Salt Lake City, to St. John. — 21. St. John, by St. Lawrence and Lakes, to New Orleans. — 22. New Orleans, by C. of Good Hope, to Pietermaritzburg. — 23. From same to same, by C. Horn. — 24. From C. Horn, very shortest line, to Hobart Town, across antarctic con¬ tinent and ocean (PI. I. K). — 25. From Hudson Bay, short¬ est way, to Tobolsk, across N. Pole (PI. I. L).— 26. New Zealand, shortest way, to C. of Good Hope, across ant¬ arctic continent (PI. I. K). — 27. Shortest way from La Guayra to Nishnei-Kolymsk, nearly across N. Pole (PI. 1.1). — 28. New York (PI. IV. sec. 456), by north-west passage, to India. — 29. From San Francisco to Ural Mts., shortest way (PI. I. I). — 30. From New York, through Str. Bab-el- Mandeb, to Mt. Sinai. — 31. From source of Jordan (PI. II. fig. 5), by Dead Sea, G. of Akabah (ah'-kah-bah), through Str. of Bab-el-Mandeb, to Mt. Hotham (Australia). (453.) Table of questions for each voyage. Go from A, (the town you start from), to B, (the town you visit). Remark. The teacher to indicate the route; as for instance, go to Nishnei-Novgorod, from New York by Str. of Gibraltar — or round C. of G. Hope, up Red POLITICAL GEOGRAPHY. 191 Sea—or up the Persian G.—or west, by Salt Lake city, San Francisco and Sandwich Is. Point out B (the town you are to visit). In what country is that town B ? In what direction from A? Longitude of A? Longitude of B? How many degrees does B lie E. or W. of A? Latitude of B? How many degrees does B lie N. or.S. of A? Bound C, (the country in which is situated the town you are to visit.) Remark. This boundary may be sometimes repeated, with more or less detail, according to the discretion of the teacher, taking in towns, lakes, provinces, gulfs, etc. In what zone or zones lies the country C? Northernmost parallel of the country? Conditions of day, night, climate, etc., in places on that northern parallel? Southernmost parallel of the country G ? Conditions of day, night, climate, etc., on that parallel? What towns, countries or places lie on, or near, that northernmost parallel, going E. around the globe? What towns, countries or places lie on that southern¬ most parallel, going E. around the globe; (or, ,if the countries, to and from which, we go, are of small dimen¬ sions , the question might be : what countries or places lie within the two parallels? What waters do you pass through, or near, from A to B? (ör, when the voyage is between two inland coun¬ tries, as from Novgorod to Petropaulovsk, then the question will be : What countries— mountains — rivers — sea(s — lakes — interesting regions, etc., do you pass through, or near? What countries have you passed, on your left, from A to B? On your right, from A to Br The mouths of what great rivers have you passed, on your left, from A to B ? On your right, from A to B? Name the towns, on or near the coast, you passed on your left, from A to B. UNKNOWN EKGIONS. On what sea—lake—river, stand the following towns? (the teacher wUl here select a few of the most prominent towns on the way from A to B.) Bead the rivers of C. (that is the country you are visiting. Read the towns of C. Name the river—sea—lake—on which stands each of the following towns: (the teacher will here select the most prominent towns of C.) These questions, of course, may be multiplied according to circumstances. (454.) Unknown Begions (117, 118). — The actual surface of the globe is reckoned at about 197 million square British statute mUes. Of these, 145 million are covered by the ocean. A glance at PI. II. will show four or five regions, almost unknown to the civilized inhabitants of the earth — the N. polar region (3 million sq. m.)—the S. polar region (8,500,000 sq. m.)—and a part of the African equatorial zone (1,500,000 sq. m.) — total, 13 millions — that is one-fifteenth part of entire globe's surface. To these may be added the central region of Australia, and part of eastern Sahara desert. The supposed advantage of reaching those mathematical points of the earth's axis, called the Poles, is, the important observations and discoveries which may be made in various sciences—among others. Ethnography*, Meteorology(•), Bot¬ any, ZoologyC"), Geology, Astronomy, etc. "As a family", says Behm, "wUl of course know all the rooms of its own house, so man, from the very beginning, has been inspired with- a desire to become acquainted with all the lands, oceans, and zones of the planet, assigned to him as a dwelling place". Among the next great events, to be looked for in the history of geographical discovery, are the arrival of some daring navigator at the point of the N. or S. Pole, and the discovery of the sources of the Nile. For the instruction of our young voyagers, we add a few words upon the latter, and what has been discovered with regard to them (May, 1867). • Eth-nog'-ra-phy—the science which treats of the so-called different races of men. (a) Me-te-or-ol'-o-gy—of the atmosphere and its phenomena. (b) Zo-ol'-o-gy—of animals. POLITICAL GEOGEAPHT. 193 (45Ô.; Sonreei of the Kile. — The Nile is formed, principally, by the union of two great rivers (Plates II. III. IV) — one, (sometimes the Black, but, in English, the Blue NUe, in Arabic, Babr-el-Azrek), has been found to flow through L. Dembea, from a marshy district, 6000 feet above the sea, in about 10® N. lat. The source of the Nile was then supposed to be discovered, (by Bruce), until it became ap¬ parent that the other great branch, the White River or White Nile, (Bahr-el-Abiad), was the ynncip«/ one—and the attempt to ascertain its origin has cost an immense number of lives. The English traveller, Speke (1861—62), found a large river flowing, north-westward, out of L. Victoria-Nyanza or Ukerewe*, 3500 feet above the sea. His reports have rendered it ■probable, although not abso¬ lutely certain (&om ocular demonstration), that it connects that Lake with L. Albert-Nyanza or (Luta), from which latter, it has been demonstrated, by Baker, that the White Nile flows. Our Plates II. III. IV. are thus drawn. At the E. of L. Victoria-Nyanza, wiU be observed another river and lake. These are the river Assua and the L. Baringo. Both, on our map, are drawn only after hear-say— that is, the reports of the aborigines, who declare them even connected with Victoria-Nyanza. But all this is not sufficient to prove that L. Albert-Nyanza and L. Victoria-Nyanza are the sources of the White Nile—any more than, tracing the Rhone or the Rhine to L. Geneva or L, Constance, would show those lakes to be the sources of their respective rivers. A large region, E. of Victoria-Nyanza, between the Mts. of the Moon and that lake, is absolutely untrodden by civilized man. It is possible, if not probable—but it has not yet been demon¬ strated— that the White Nile originally flows from the lofty Snow Mts. He who shall first trace the widening course of some petty, bubbling rivulet, from the group of Kenia or Kilimandjaro, to L. Victoria-Nyanza, will, at last, solve the problem of the source of the Nile, and identify that mountain-range with the Jebel el-Komri, or Mts. of the Moon, mentioned by Ptolemy (see remark 275).— The • It may- be presumed (204) that the world at large will generally find it convenient to give this class of names, thus, in full, — Lake Victoria Nyanza—however often it may be told that the word, lake, is included in the aboriginal name. 13 194 UNKNOWN REGIONS. nnnamed branch, on the maps, between the White and Blue Nile, is the Sobat R, Its coarse has never been explored. (456.) North-West Passage.— We have (182) passed from Behring Str. to Str. of Belle Isle, by -what is called the north-west passage. Let us bestow a few moments attention upon this interesting portion of the earth. More than 300 years ago (1519), Magellan, a Spaniard, sailed from Spain, down Atlantic, discovered the strait bearing his name, and crossed Pacific to Ladrone and Philippine Is. —while one of his ships continued the voyage, around C. of Good Hope, back to Spain. Our globe was thus cir¬ cumnavigated, for the first time, and its spherical form demonstrated. This voyage suggested the idea of a shorter passage to India, around the northern coast of N. America. From that time, until our day, the existence of what is called the north-west passage, has been one of the problems of Geography. — Since the beginning of the 18 th century, a succession of daring navigators, whose names, as well as those of their patrons, are often inscribed upon the straits, islands, etc., have led expeditions into the arctic zone. Behring discovered Behring Sea and Strait (1725—28). Cook passed beyond the 70 th parallel (1778). Mackenzie explored a part of this northern coast (1789). The Hamburg whale ship, Capt. Ocken, sailed up the Behring Str. to 80 th paral¬ lel and reported an open ocean, free from ice, (1815). In 1815 — 18 Kotzebue demonstrated that no connection existed between America and Asia. Parry, Franklin, Ross, and others, have penetrated into these regions and sometimes passed several years. Sir John Franklin (1845) led an ex¬ pedition in search of the north-west passage and never returned. It has been since ascertained that his ship was locked in by ice, near Beechy I. (PI. IV.) in Wellington Canal, near Lancaster Sound, on lat. 75 N. He perished, with 105 companions, June 1847. In 1850, the British Capt. McClure visited Banks Land, demonstrating it to be an island—sailed, from W., through Str. Prince of Wales and discovered the mouth of great Melville Sound. His vessel was afterward seen, by Lieut. Pim, coming from the E. The fact was thus established, of a water communication, between Atlantic and Pacific, by Arctic Ocean. A passage runs from Baffin Bay — through Lancaster Sound— Barrow Str.—Melville Sound or Str.— then through Prince POLITICAL GEOGRAPHY. 195 of Wales Str., or, north--west, through Banks' Str., some¬ times called McClure Str. In 1850 and 1853, two ex¬ peditions, under the patronage of Henry Grinnel Esq., New York, were headed—one, by Capt. De Haven—the other, by Dr. Kane; the latter appeared to confirm the report of the Hamburg Capt. Ocken, that the pole is surrounded by an open sea. The am. expedition (Hayes, May 1861) reached the northernmost known land of our planet—81° 35'—and could see along the coast to a point, 82° 30' —which he named C. Union. There is believed to be a second passage, farther to the North, through Banks' Str. and Lancaster Sound; and a southern one, through Hudson Str.—Fox Channel—Fury and Hecla Str. — Boothia G. to Coronation G. The north-west passage, although thus demonstrated to exist, does not appear practicable as a better way from Atlantic to India, being nearly always blocked up by ice. If, however. Smith Str. or Sound, Kane's Sea, Kennedy Channel should be found an open way, and if the reports of Dr. Kane and Capt. Ocken should turn out to be correct, that a considerable central area of the arctic circle is occupied by a warmer ocean, free from ice—the long cherished hope of reaching the pole, may yet be accomplished; and, possibly, a shorter way discovered from Greenland, London and St. Petersburg to Behring Str. (Pl. I. L). (456 A.) Remark. 1. There is no idea of abandoning polar expeditions. By sledges or ships; by governments or private munificence, the North Pole will soon be reached. A knowledge of the whole globe's surface has become a necessity of science. We must know every inch of Sahara — Australia—New Zealand — New Guinea—Patagonia— central Africa—the polar regions, and even the valleys of the ocean. 2. The U. S. Government hae granted greater sums for geographical works than any government of Europe. 3. "The christian missionaries", says the German Year Book, "now scattered over the globe, have rendered import¬ ant services to Geography; among them. Hue, Livingston, Krapf, etc. Their patient and long-persevering intercourse with half-known peoples and tribes, has advanced our knowl¬ edge of languages and of the different varieties of men." To this we add: their influence, on the cause of christian civilization, has been far more striking and useful. 13* PART TV. OUTLINE VIEW OF PROVINCES,RIVERS, TOWNS, ETC. OF SOUTH-WESTERN EUROPE. (PL. V. AND PL. VL B.) (457,) Remark. We have now acquired an idea of natural land and water divisions, the names and positions of coun¬ tries, towns, mountains, rivers, etc. We have not confined ourselves to our own, nor to other civilized countries. We have examined, with the same attention, the polar, the temperate and the equatorial zones; remote, savi^e lands, and waters scarcely known, as carefully, as those in our vicinity. We have taken a hird!s-eye view of the globe's entire surface. Two regions—United States and Europe— require more particular study. And, first, Europe. In order better to understand PI. VI. B., it is proper to glance slightly at the most striking territorial changes which this portion of the E. Continent has undergone; and briefly to review some of the great historical events which have caused them. (458.) Roman Empire. — At the birth of our Saviour, the world may be said to have lived under the scepter of one man, the Roman emperor, Augustus Cesar, nephew of Julius Cesar. Following the authority of Gibbon, and sometimes using his words, we compress a very general account of the extent of bis empire. It SOUTH-WESTERN EUROPE. 197 comprehended the fairest part of the earth and the most civilized portion of mankind (PL III fig. 5 — also Pis. II and III). The northernmost bends of the Rhine, Danube and Carpathian Mts., formed its N. E. boundary, in Europe. In Asia, its frontier embraced Asia Minor, the territory S. of Caucasus, and a region, east, reaching to Caspian Sea and Persian G. Ex¬ cluding the greater part of Arabia, it took in Palestine, the principal part of Egypt, and all the N. coast of Africa, known as Barbary States; on the N. W., England with "Wales and the lowlands of Scotland to the Friths of Forth and Clyde (PI. VI). The modern countries, standing upon the territory once occupied by the Roman Empire, are, Portugal, Spain, France, England, Belgium, Prussian Rhine Province, portions of Baden, Wurtem¬ berg and Bavaria, Switzerland, Italy, southern prov¬ inces of Austria, including Hungary and Transylvania, Turkey in Europe and Greece, all Turkey in Asia, Egypt, Barca, Tripoli, with Fezzan, Tunis, Algeria and Morocco. The excluded adjacent countries are, Ireland, part of Scotland, Holland, Prussia, with the North German League (N. of the Main), Bohemia, Moravia, Galicia, Russia, etc. Arabia, on the S. E., remained also unconquered. The whole extent of the Mediterranean Sea, its coasts and islands, were comprised within the Roman dominion, which was, in breadth, more than 2000 miles, from the N. European frontier, south to Mt. Atlas and tropic of Cancer—in length, more than 3000 miles, from Atlantic to Euphrates. About as large as the United States of America, and nearly between the same parallels, it was situated in the finest part of the temperate zone, and, like the previous five consecutive world empires (Egypt, Assyria, Babylon, Persia and Greece or Macedonia), it comprehended, within its boundaries, that remarkable country, Palestine " which says Gibbon, " will live for ever in the mem¬ ory of mankind, as, from its narrow limits, has issued forth the religion, adopted by aU the civilized nations of the earth". That country, less than 200 miles long. 198 SOOTH-WESTERN EUROPE. by about 75 miles broad, forms, in our day, several Turkish pashalics, at the E. extremity of Mediterranean. Fig. 5. Pi. II. gives its "narrow limits", with lake Ti¬ berias, river Jordan and Dead Sea. No inferior animal has ever aspired to universal dominion over its fellow beasts. But, to use again the words of Gibbon, "the ambitiom desire of subduing the earth" has been the favorite dream of great con¬ querors. Nebucadnezzar, Xerxes, Alexander, Cesar, Charlemagne, Napoleon — each, in his turn, has been dazzled by a splendid vision of "all the kingdoms of the world and the glory of them". During nearly a hundred years, Augustus and his successors the emperors Nerva, Trajan, two Antonines, etc. — may he said to have, in some degree, attained this coveted prize. The transitory heathen kingdom, which man had established, "by the might of his power and for the honor of his majesty"—"the city and tower whose top was to reach unto heaven"— had risen to its culminating point, at the moment, when a greater than man in the form of a friendless infant, scarcely ad¬ mitted into the stable of a tavern, appeared upon the earth, to lay the everlasting foundation of the kingdom of God. This impressive antithesis is carried out during the whole life of our Redeemer, and, particularly, in his death. While the pure and lowly Jesus, the Savior of the world, who had never committed a sin, was extended on the cross, an atonement for mankind—Tiberias, the emperor of this present world, marked by the vilest vices and the basest qualities, was closing his life in the luxurious island of Caprea, sunk in infamous, disgusting debaucheries; and, by "his infernal machina¬ tions and crimes, exposing the life, the fortune and the honor of every Roman citizen". (459.) Fall of the Roman Empire. — The Roman Empire (1) broke to pieces in the 4th century. The Persians, the Scythians, the Goths and other bar¬ barians, attacked it at every point. Out of its immense SOUTH-WESTERN EUROPE. 199 ruins, liave risen the modern states of Europe. It is a singular circumstance, however, that it did not cease to have a political representative, from the time of Augustus to that of Napoleon I; and the plan of reviv¬ ing it, in more than all its ancient power and gloiy, has never been permanently abandoned. This is one of the secrets of history. (460.) Germanic or Holy Roman Empire. — Among the various political organisations, built upon the ruins of Rome, was Germany. Charlemagne was crowned, at Rome, by the Pope, Emperor of the West, or Emperor of the Romans (A. D. 800). His suc¬ cessors kept up this title about 160 years (A. D. 962), when it vested in the emperor of Germany, thenceforth designated, monarch of the Holy Éoman Empire. The second head was added to the eagle, in order to denote the union of the empires of Germany and Rome. From this time, and through the subsequent period of a thousand years, the Empire of Germany was styled, the Holy Roman Empire. At the breaking out of the great french revolution (1789), its territories were di¬ vided into 10 Circles (PI. V. A. Fig. 1). (461.) Frencli Revolution — Napoleon I. — Under the reign of Louis XV, king of France, the vices of the king and court, the oppressions of the people, the general spread of infidelity, etc., produced a revolution, the most terrific recorded by history. One might almost infer that the great crises of human affairs grow, in intensity, like the plutonio irruptions of our planet (282C). The outbreak reached its height under Louis XVI. who, with his queen, was beheaded. It deluged France with the blood of the scaffold, and devastated Europe with wars. Out of the stormy biUows of these political disorders, rose that young officer. Napoleon Bonaparte, one of the most remark¬ able men, and the greatest soldier, of any age, whose brilliant military genius, and unbounded ambition, nearly 200 80ÜTH-WESTERN EUROPE. succeeded in reducing Europe, and the adjacent parts of Asia and Africa, under his scepter; and in thus reviving the magnificent empire of the Cesars. By his victories over Austria (Marengo, 14. June, 1800,— Austerlitz, 2. Dec., 1805) and over Prussia (Jena, 14. Oct., 1806) he overturned the old Germanic or Holy Roman Empire, already tottering into decay. He created, fpr his brother Jerome, a new kingdom, Westphalia; and raised, other members of the Germanic Confederation, into independent sovereigns, united by a league, called the Confederation of the Ehine. Under these circumstances, the German Emperor, Francis II, by a communication (Aug. 6, 1809) addressed to the great Powers of Europe, officially renounced the title of Emperor of Germany and of the Holy Roman Empire, which his ancestors had worn for a thousand years, and assumed the title. Emperor of Austria. "The Emperor of Germany" says Alison, in his History of Europe, "thus ceased to be the representative of the empire of the Cesars". Napoleon had already ascended to this lofty pre-eminence. He had been crowned Emperor of France, by the Pope, (Dec. 2, 1804). He then exacted that he should be crowned, again, King of Italy and Rome, with the iron crown of Charlemagne, as the new representative pf the empire of the Cesars, and, consequently, a monarch higher than all the other monarchs of the earth. The cere¬ mony took place at Milan (1805). The haughty con¬ queror seized the crown and placed it upon his own head, thus intimating that he reigned by his own power; at the same time, uttering the words: "God ha» given it to me. Beware who touches it!" The Roman States were annexed to France, and the heir apparent of the french throne was invested with the title of King of Rome. (462.) Treaties of Vienna. — The fall of Napo¬ leon Bonaparte was more sudden even than his rise. His splendid fabric was dashed to pieces at Moscow, Leipsic and Waterloo; and he was confined at St. SOÜTH-WESTERN EUROPE. 201 Helena, a rock in the Atlantic, where he died a broken-hearted prisoner (1821). The victorious mon- archs of Europe met, by their representatives, in a Congress at Vienna (1815), and, by those celebrated documents, called the Treaties of Vienna, gave, to the European countries, the political frontiers which, with some exceptions, continued to be their limits until 1866. (463.) Changes since Treaties of Vienna. — Italy, by these treaties, was occupied by seven independent monarchies or states, (PI. V. B. fig. 2. — sec. 482), while the beautiful plains of Lom- bardy and Venice, in northern Italy, were given to the then triumphant Austria. Belgium and Holland were united into one kingdom; and Greece was left under the Turkish scepter. By the revolution of 1830, Belgium was separated from Holland and erected into an independent kingdom; and the Italian war of 1859, (in which France and Sardinia, by the victories of Magenta and Solferino, drove Austria entirely out of Italy) erected the whole Italian Peninsula into one kingdom and, finally, brought Lombardy (1859) and then Venice (1866) under the scepter of Victor Eman¬ uel. A very small region was left with the name of Papal Territory (PI. VI. B) which the now united and powerful people of Italy desire to incorporate as the capital of their kingdom. To these changes, must be added the revolution, by which Greece (1829) threw off the Turkish yoke; the elevation of the Turkish provinces, Moldavia and Wallachia (known as the Principalities of the Danube), to the rank of a nation (1866); and, greatest of all, the resurrection of Napoleonism (Dec. 2, 1851), when Louis Bonaparte (Napoleon III.) seized the imperial sceptre; thus overthrowing the public law of Europe, as founded on the treaties of Vienna. (464.) Germanic Confederation from 1815 to 1866. — By the treaties of Vienna (1815) Germany was reconstructed in such a way as to consist of 202 80VTH-WESTERK EUROPE. 38 states, and, with few essential changes, it so re¬ mained till 1866, at which time, three had been merged into others, leaving only 35. Holland was a member of the Confederation, for two of her provinces—Luxem¬ burg and Limburg; Denmark, also, for Holstein, with Lauenburg. The Germanic Confederation (marked by a red line PI. V. A) then extended from North Sea and Baltic, to Adriatic. It was bounded, N. by North Sea, Denmark (Schleswig), and Baltic; E. by non-German Prussia, Russia, and. non-German Austria; S. by Adriatic, Yenetia and Switzerland; W. by Yenetia, Lombardy, Switzerland, France, Bel¬ gium and Holland. (R. these boundaries again from PI. Y. A). The states of the Confederation were distinguished by 8 different forms of Government, namely: 1 Empire, 5 Kingdoms (exclusive of Denmark and Holland), 7 Grand Duchies, 9 Principalities, 1 Electorate, 1 Landgraviate, and 4 Free Cities. A glance at PI. Y. A, will, in a few moments, acquaint the attentive student with the names, relative size and position of the German States (Pop. 46 millions). It was of this Plate that Alex. v. Humboldt said: "Perhaps no mapever did make Germany so clear." (465.) List of German States before 1866 — One Empire. — Austria. Five kingdoms. — Prussia — Saxony — Bavaria — Wurtemberg — Hanover. Seven Grand-Dttchies. — Baden — Hesse-Darm- Stadt — Luxemburg with Limburg—Oldenburg — Mecklenburg-Schwerin (Shway-reen') — Meck- lenburg-Strelitz (straylitz) — Saxe-Weimar (wï-mar). Seven Duchies. — Nassau — Brunswick — Hol¬ stein, with Lauenburg — Anhalt (formerly Duchies of Bernburg, Koethen (curten), and Dessau) — Saxe- Altenburg — Saxe- Meiningen — Saxe-Coburg- Gotha. Nine Principalities. — Reuss-Greitz (îtze) — Reuss-Schleitz (îtze) —Schwartzburg-Rudolstadt SOUTH-WESTERN EUROPE. 203 — Schwartzburg-Sondershausen — Schaumburg Lippe—Lippe-Detmold —W aldeck — Hohenzol- lern — Lichtenstein (lik'-ten-stîne), on the ea.stern frontier of Switzerland. One Electorate. — Hesse-Cassel. One Markgraviate. — Hesse-Homburg (near Frankfort — very small). Fowr Free Hanse Towns. — Frankfort-on-the- Main (seat of the Germanic Diet) — Bremen — Ham¬ burg—Lübeck. (466.) Thuringian States. — This name is given to the following (PI. V. A); G. D. S axe-Wei- mar—D. Saxe-Coburg-Gotha—D. Saxe-Meinin- gen—D. Saxe-Altenburg—P. Schwartzburg- Rudolstadt— P. Schwartzburg-Sondershausen. (467.) Hanse Towns — called also the Hansa, and Hanseatic League. In the Middle Ages, Ger¬ many, and the neighboring seas, were infested with tyrannical feudal chiefs, banditti, pirates, etc. Many towns, among others those we have mentioned, entered into a commercial alliance for mutual defence, under this name. The number of towns is said to have once amounted to 85. The alliance was dissolved about 200 years ago; but Hamburg, Bremen, Lübeck and Frankfort - on-tbe-Main, still continued in some¬ what similar relations, and were called the free Han¬ seatic cities of the Germanic Confederation. (468.) Prussia, with North Oerman League, after civil war 1866. — Plate V.A. and VLB. show Prussia before this war. Her disjointed territory lay, it has been said, like a pair of garters, on a table. As it consisted of several fragments, it might better be likened to a plate fallen upon the floor, and broken to pieces. Between the two provinces, Westphalia and Rhine Pr. and the rest of her territory, nearly all the small Gerrnan States intervened; so that, in this respect, she could be re- 204 SOUTH-WESTERN EUROPE. garded but as a very weak Power. Now mark the changes after the war (PJ. V. B). Five of the intervening States — one of them, a considerable kingdom — have been incorporated into her territory, namely: Kgd. Hanover — Electorate Hesse-Cassel — D. Nassau — Free City Frankfort-on-the-Main, and Land- graviate Hesse-Homhurg. Not only D. Hol¬ stein, hut the adjacent Danish D. Schleswig are annexed. Twelve States or Free Cities, beside those called Thuringian States, if not incorporated, at least have been induced to enter into close subordinate relations with her, under the name of North German League. They lie wholly, or in part, enclosed within her territory, and are: Egd. Saxony—G. D. Meck¬ lenburg-Schwerin— G. D. Mecklenhurg-Strelitz — G. D. Oldenburg — Northern half of G. D. Hesse- Darmstadt— D. Brunswick — D. Anhalt—P. Lippe—P. Waldeck — Thuringian States (466) including the adjoining states ofReuss — Free Cities Hamburg—Bremen — Lübeck. It requires only a glance at the maps to per¬ ceive the consequent aggrandizement of Prussia. Situated in the center of Europe — with a population of 29 millions — a compact territory — an unbroken frontier on every side — a perfect military organisation— a largely increased coast-line both on Baltic and North Seas—Lübeck, Hamburg, Bremen, converted almost into Prussian ports — she has become one of the greatest Powers of the world. The rest of the states, members of the Germanic Confederation before 1866, and having opposed Prussia in the war, namely, G. D. Baden, kgd. Wurtemberg, kgd. Bavaria, southern half of G. D. Hesse-Darm¬ stadt, i. e., the half S. of River Main, and P. Lich< tenstein, do not form part of North German League. But they have entered into treaties, offensive and de¬ fensive, with the king of Prussia, stipulating, in case of war, to invest him with the command of their troops. We may well presume that these political ar- 80ÜTH-WESTERN EUROPE. 205 rangements are not permanent. It is necessary, however, that they should be understood by every attentive ob¬ server. While Prussia has risen to this great political pre¬ eminence, Austria has suffered a series of misfortunes which have threatened almost her existence. By the Italian war of 1859 she lost Lombardy; by the war of 1866, the territory of Venetia; and she was compelled to retire before the supremacy of Prussia as a German Power. This is not the place to point out the prob¬ able consequences of these great changes. Many believe that Austria has still vitality and allies enough to procure indemnification for her losses, on her south¬ eastern frontier (PI. VI. B.); thus precipitating the banishment of the Ottoman Power from Europe; and rendering the dreaded Turkish question, not only more urgent, but more complicated. COUNTRIES AND PROVINCES OP SOUTH¬ WESTERN EUROPE. (469.) Our purpose in presenting PI. V. A. and B. and PL VI. B. is;—1. To give the limits of the German States (PI. V. A), as they existed from 1815 till 1866. 2. A view of the reconstructed Germany, as far as it has proceeded, since the dissolution of the Germanic Confederation. 3. A somewhat nearer view of the rivers, towns and exterior waters of Great Britain and Ireland. 4. The great historical provinces of Portugal, Spain, France, Prussia, Austria, Roumania, Turkey in Europe, Greece, Italy, and Switzerland; with a nearer view of their towns, and rivers, including Belgium and Holland. In the wars which have already taken place, and those which may be hereafter expected, territorial changes are frequently made, are often the objects of the wars, and are best understood by those 206 SOUTH-WESTERN EUROPE. who have studied the names, relative positions, and antecedents of historical provinces. Thus, 1860, after the Italian war, France annexed the Italian provinces of Savoy and Nice, by the consent, most reluctantly extorted, of the government of Italy, and not without awakening a deep feeling of resentment, on the part of the Italian nation; for ' Savoy is the key to Italy. At the same time, Italy took Lombardy from Austria. One of the first results of the late civil war in Germany, was the cession of Venetia to the king of Italy. The erection of the two provinces, Moldavia and Wallachia, into what may be called an independent kingdom, seems to be the forerunner of greater changes in the Ottoman Empire. The province of Luxemburg — that portion of Holland, for which its sovereign was member of the Germanic Confederation till 1866 — till the question was settled by a european Conference (London, May, 1867) threatened to become the occasion of a general war. It •would be superfluous to give the provinces of all countries; but it is deemed important that the intelligent young American student should have a clear view of the sub¬ divisions of this part of the world, whose great approach¬ ing changes attract the attention of thinking men. (470.) Provinces of Portugal. — Minho — Tras-OS - Montes — Beira—Estremadura—Alem- tejo — Algarve. — Insular Provinces-. Azores—Ma¬ deiras. Remark. Of Portugal, Spain, France, and Turkey, we give the names of historical provinces still retained in those countries, although these ancient divisions, for administrative purposes, have been subdivided into departments, etc. (in Turkey, into eyaUts or pashalics). (471.) Provinces of Spain. — On Atlantic: An¬ dalusia — Galicia — Asturias — Old Castile — Basque Provinces (Biscaya, Guipúzcoa, Alava) — On France: Basque Provinces again — Navarre — Aragon — Catalonia. — On Mediterranean: Cata- SOUTH-WESTERN EUROPE. 207 Ionia again — Valencia — Murcia — Granada — Andalusia again — On Portugal; Andalusia again — Estremadura — Leon. — Central Province; New Cas¬ tile (Madrid). — Insular Provinces; Balearic Is. — Canary Is. (472.) Basque Provinces. — This term is omitted in the Plate, in order to avoid the confusion of crowded names. The three small provinces, com¬ prehended, under it are Biscaya or Vizcaya — Guipúzcoa — and Alava. The Basques are cel¬ ebrated for their courage and energy, and form the best soldiers and sailors of Spain. They boast that, not only no Arab steed has ever stamped upon their soil, but that, though the most ancient representatives of the Spanish race, neither Carthaginian, Roman, Goth nor French, has ever subdued them, or even corrupted their language, which they declare to be that used by Adam and Eve in Paradise. In the 13 th century, they voluntarily became subjects of the Queen of Castile, reserving, however, many inviolable rights. They enjoy a considerable independence, a diet, judiciary, laws and a representation of their own. In fact they form a kind of independent government. For 1300 years, their parliament has been held near an old oak at Vizcaya. (473.) Provinces of France. — On English Channel; Brittany or Bretagne — Normandy — Picardy — Artois — Flanders. — On Belgium and Germany; Flanders (again)—Champagne—Lor¬ raine— Alsace. — On Switzerland; Franche-Comté — Burgundy (Bourgogne) — Savoy.— On Italy; Savoy (again) — Dauphiné — Provence — Nice — On Mediterranean Sea; Provence (again) — Langue¬ doc— Roussillon — I. of Corsica. — On Spain; Roussillion (again) — Foix — G as cony — Béarn. — On Bay of Biscay; Gascony (again) — Guienne — Saintonge — Poitou with Vendée. — CentralProv- inces; Anjou — Maine — Orléanais — Isle de 208 SOUTH WESTERN EUROPE. France (Paris) — Nivernais — Bourbonnais — Ly¬ onnais— Auvergne — Limousin — Angoumais — La Marche — Berry — Tourraine.— (474.) Pro rinces of Prussia (Pl. V. A) — may, at present, be divided into two classes, namely, the 9 original provinces before 1866 — and the 7 prov¬ inces subsequently annexed. Nim original provinces: Pomerania—West and East Prussia—Posen (Prussian Poland) — Silesia (Prussian) — Saxony (Prussian) —Brandenburg —Westphalia — Bhine Province — Hohenzollern — the latter added at a later period, quite isolated in the S. of Germany. Seven provinces subsequently annexed: Egdm. Hanover — Electorate Hesse-Cassel—Free territory and city of Frankfurt-on-the-Main — D. Nassau — Landgraviate Hesse-Homburg—German Duchy Holstein with Lauenburg — Danish Duchy Schleswig. (Now see PI. V. B). (475.) Provinces of Austria (PI. V. A and B and PI. VI. B) — before 1859 might be grouped as follows: 1. German provinces. 2. Non-German prov¬ inces. 3. Italian provinces. German provinces: Bohe¬ mia— Austrian Silesia — Moravia — Upper Aus¬ tria — Lower Austria — Styria — Salzburg — Tyrol with Vorarlberg — Carinthia — Carniola (with Istria, Goritzia, and the town and territory of Trieste).—Non-German provinces: Galicia with Cracow—Hungary with Banat—Bukowina — Transylvania — Slavonia — Croatia — Military Frontier — Dalmatia. — Italian provinces: Lom- bardy and Venetia (the latter two now ceded to Italy). (476.) Coast Land — Littorale — Kgd. Illyria. — These terms were once, and are sometimes yet, applied, to the Duchies of Carniola, Carinthia, Istria, etc., with the town and territory of Trieste. SOUTH-WESTERN EUROPE. 209 (477.) Magyar Provinces. — Hungary and Transylvania are so called. Remark. The subdivisions of Austria, since the revo¬ lution of 1848, have undergone so many changes that, says Daniel, "they are enough to drive any geographer to des¬ peration." (478.) Provinces of Ronmania. — Valakhia — Moldavia. (479.) Provinces of Turkey in Europe. — Bosnia .with Turkish Croatia and Herzegovina — Servia — Bulgaria with Dobrodja — Roumelia (ancient Macedonia and Thracia) — Albania with Thessaly — Montenegro — Jezayr (Dschesair), or the "Islands" — Candia or Crete. Remark. The existence of Turkey in Europe appears drawing to a close. Many of its nominal provinces are in fact independent—particularly Egypt. (480.) Provinces of Greece. — Roumelia — Morea or Peloponnesus — Ionian Islands — Gre¬ cian Archipelago. Remark. — 1. — That part of present kingdom of Greece, called Rumelia, was, under the Turkish govern¬ ment, Livadia; among the ancient Greeks, Hellas. It is not necessary here to give the administrative subdivisions. 2. — The Archipelago, or islands in the Aegean Sea, between the mainland of Greece and Asia Minor, are, on the map, distinguished, from the Turkish islands, by a red ime. PL VI. B. (481.) Cyclades — Sporades.— Observe (PI. VI. B.) a group of islands, lying on the east coast of Greece, somewhat in parallel lines. They may be re¬ garded as insular prolongations of Euboea and Ru¬ melia. 'Among them are: Delos, Syra. They are called the Cyclades (sik'-la-deez), from a Greek word, a circle — because they closely encircle the little I. of Delos. The rest of the islands of the Archipelago, 14 210 80ÜTH-WESTBEK EUKOPB. both greciao and tarkisb, are called the Sporades (spor'- a-deez), from a Greek word, scattered—because they lie scattered around the Cyclades. Among them are: Enboea or Negropont, Hydra, Aegina, etc. (482.) Sabdivlsions of Italy from 1815 to 1859 (PI. V. B. fig. 2). — Kgdm. Sardinia (incind- ing D. Savoy, P. Piedmont, D. Genoa, County Nice, and I. of Sardinia) — D. Parma—D. Modena —D. Lncca — G. D. Tuscany — Papal States, enclosing the little rep. San Marino — Kgdm. Naples with Sicily. The Lombardo-Venetian kingdom formed part of Austria. (483.) Present Provinces of kingdom Italy (PI. VI. B). — Piedmont—Lombardy—Venetia — Emilia— Marca—Umbria—T nscany — Naples or Lower Italy — I. of Sicily — I. of Sardinia. Remark. The Papal Territory has not yet (April 1867) been included among the provinces of Italy. (484.) Cantons of Switzerland (PI. V. B). — Switzerland consists of 22 cantons —? ñ-ench, german and italian. — Bern — Soleure (so-lnr') —Basel — Aargan — Zurich (zn'-rik) — Schaffhausen — Thnrgan (tooP-gow)—St Gall — Appenzell — Grisons — Ticino (te-chee'-no) — Valais — Geneva — Vand (vö) — Nenfchatel (nosh-ah-tel') — Freybnrg (firx'- boorg) — Lucerne (lu-sern') — Zug (zoog) — Schwyti (shweetz)—Glarus (glaP-roos) — Uri (u'-ree) — Unter- walden. Remark. Where names of town and canton are iden¬ tical, the former, alone, is sometimes given. RIVERS AND TOWNS OF SOUTH-WESTERN EUROPE. (PL. VI. B.) (485.) Chief Sivers of England. — Thames — Severn with Upper and Lower Avon — Mersey SOUTH-WESTERN EUROPE. 211 — Eden—Tyne — Humber, with its affluents Ouse (ooz) and Trent—Great Ouse. (486.) Chief Towns of England and Wales.— We first name some great sea and riyerports. London— Dover— Brighton — Portsmouth — Southampton — Cow es — Exeter — Plymouth — Falmouth — Bristol—Swansea andPembroke(Wales)—Chester —Liverpool—Lancaster—Carlisle—N ewcastle- upon-Tyne — Sunderland— Hull —Yarmouth — Colchester. Now we name some of the chief interior towns. Bradford — Leeds —York— Bolton — Manchester — Sheffield — Lincoln — Shrews¬ bury— Derby—Nottingham—Wolverhampton — Birmingham —Leicester—Norwich —Worcester (Woo'ster) — Oxford—Cambridge—Bath—Canter¬ bury — Merthyr - Tydvil (Wales). Towns on the following rivers, beginning at the source. On Thames'. Oxford — London — Greenwich (cele¬ brated for its royal observatory, from which longitude is often measured). On Severn: Shrewsbury — Worcester. On Upper Avon: Stratford (the birthplace of Shakspeare, who is therefore often called the Swan of Avon). On Mersey: Manchester—Liverpool. On Eden: Carlisle. On Tyne: Newcastle-upon-Tyne. On Humber and its affluents Ouse and Trent: Hull — York — Leeds, (for Wales, see 522.) (487.) Chief Rivers of Scotland. —Tweed — Forth — Tay— Dee—Ness — Clyde. (488.) Chief Towns of Scotland. — Berwick — Edinburgh — Dundee—A herd een — Inverness — Paislay — Glasgow—Dumbarton. What towns lie on the following rivers? On Tweedt Berwick. On Earth? Edinburgh. On Tay? Perth — Dundee. On Dee? Aberdeen. On Ness? Inverness. On Clyde? Paisley— Glasgow — Dumbarton. 14* 212 SOUTH-WESTERN EUROPE. (489.) Chief Elvers of Ireland. — Liffey with D ublin Bay— Suir (share) with Waterford Harbor — Blackwater — Lee — Shannon—Corrib (River and Lake) with Galway (gawl'-way) Bay. (490.) Chief Towns of Ireland. — Sea and river- ports; Dublin — Waterford — Cork with Queens- town— Limerick — Galway— Londonderry — Belfast. — Interior towns: Tipperary — Killarney. (491.) Rivers of European Continent. — We review these rivers, adding some of the more important, not previously named, for the purpose of studying their relations to the countries and towns (PI. VI. B). Into Atlantic: Guadalquivir — Guadiana — Tagus — Douro — Minho. — Bay of Biscay: Gironde (with Dordogne and Garonne) — Loire. English Channel: — Seine. — North Sea: Scheldt (Sheld) — Meuse or Maas (with its mouths) — now PI. V. A and B — Rhine (with its 4 principal branches — right bank: Neckar — Main; left bank: Aar — Moselle)—Weser — Elbe (with its branches Havel and Spree).— Baltic: Oder — Vistula — Niemen — (now PI. H) Duna —Neva —Tornea. — White Sea: Dwina. Arctic Ocean: Petchora. — Caspian Sea: Ural—Volga.— Sea of Azof: Don. — Black Sea: Dnieper — (PI. VI.) Dniester — Danube, (with its branches — left bankj; Theiss (tïce) and Pruth (proot); right bank: Isar —Inn—Drave and Save).—Adriatic: Po.— Tyrrhenian or Tuscan Sea: Tiber — Arno. — G. of Lions: Rhone (with its (branch Saone (sown). — Mediterranean: Ebro. (^492.) Remark. 1. The Isar is the national river of Bavaria, having in all times, from its source to its mouth, belonged to the Bavarians. Its banks are rich in fruit and its basin is the principal seat of the old Bavarian population. 2. As the teacher reads the three next sections, very slowly, the pupil will follow each place on the proper map or maps. SOUTH-WESTERN EUROPE. 213 (493.) The Rhine — sometimes called by the Germans Father or King Rhine, is often said to spring from three small streams, the Vorder Rhine — the'Hinter Rhine and the Middle Rhine. In reality it originates in a large number of mountain- torrents, each bearing its name. It is the "highest born" of the German streams, rising in the Swiss Alps, near Mount St. Gothard, about 7000 feet above the sea. It is more than 800 miles long, and its depth varies from 20 to 50 feet. It flows, after various bends, in a N. W. direction, into North Sea. — Examine PI. V. B. and see what states or territories it passes through or between. After traversing a part of Switzerland, it forms, with the broad Lake Con¬ stance, into which it expands, the boundary line between Switzerland, on the one side, and Austria, Bavaria, Wurtemberg and Baden, on the other. Then, flowing directly N., it forms the boundary Hue between France and Baden; thence, intersecting several small German States, it sweeps through the Prussian Rhine-Province and Holland, pouring its waters into North Sea, through a number of broad arms or estuaries which enclose an extensive delta. The River Meuse or Maas, unites its waters with those of the Rhine, in this part of its course; and, strange to say, the principal channels of entrance to the Rhine bear the name of the "mouths of the Meuse"; — while the Rhine preserves its name only in an insignificant stream, called the Old Rhine, which reaches the sea near Leyden. It is navigable, for tolerably large vessels, as far up as Strasburg; for smaller steamers as high as Basel; and boats ascend some distance higher, to Schaffhausen. No German river is so much visited by tourists. In Switzerland, its scenery is sublime. Its impetuous waters rush through the valley of the Rhine, surrounded by the most picturesque crags and lofty alpine peaks. Between Mayence (or Mainz) and Cologne, in the Pr. Rhine Province, the scenery is particulary celebrated. Beautiful mountains and rocks crowd around the river 214 BODTH-WESTEBN EUROPE. shores, which are scattered with rich vineyards, towns, valleys, churches, etc. Sometimes, the mountains rise in an amphitheatre, capped with the ruins of ancient towers and castles, connected with which are the most romantic legends and interesting, historical associations. At other points, they open into delicious valleys, through which numerous affluents flow, swelling the waters of the parent river. The navigation of the Rhine is of great and increasing importance. Perhaps no river is more closely connected with the political state of Europe. The French appear to consider it their natural boundary. Upon this point there is a deep susceptibility on the part both of the German and French nations. This river was first made known to the civilized world by Julius Cesar, who twice crossed it in his wars with the Germans. (494.) The Danube — the second in magnitude among european rivers — rises in Baden, one of its sources being enclosed within the court of a castle, in the small town of Donaueschingen (do'now-esh'ing en). It thence flows through Wurtemberg, Bavaria, Austria, Roumania and Turkey; becomes part of the boundary line between the two latter States; and enters the Black Sea by several channels, forming a large marshy delta. Near its mouth, in consequence of sand-banks and other obstacles, there are difficulties in the navi¬ gation, which have occasioned many disputes between Turkey and Russia. The region, on the right side of the Danube, called the Dobrodja—a pestilential tract — has recently been the seat of Russian and Turkish warfare. The scenery is highly diversified. Sometimes the river rolls along among beautiful eminences, like those of the Rhine, crowned with picturesque ruins — sometimes it washes the rocky angles of precipices and mountains — sometimes, in many circuits, meanders over vast level plains. Here, it is divided into numeroiis channels, enclosing marshy islands — there (as on the borders of Hungary and SOUTH-WESTERN EUROPE. 215 Roumania, at the point called the "Iron Gate"), it rushes, with deafening noise, through a- deep defile, breaking into a series of minor cataracts. Sometimes narrow — sometimes wide — its movement is now dangerously rapid — now measured and slow. It is, nevertheless, navigable through the greater part of its course, though the navigation is often obstructed by rocks, shoals, and whirlpools. It has been described, by a German writer, Biffard, to resemble "a beautiful, intelligent, coquettish woman, full of changes and contradictions. Now, she advances silently, as if lost in reverie — now, she overflows with sparkling mirth. At one moment, she is full of humors and caprices — at another, she proceeds with dignity and reflection. But have a carel—trust her not! Where she is the least deep to-day, to-morrow, we cannot fathom her; and, after years of attentive examination, we know as little of her real character, as in the first hour of our acquaintance". The limits of this work do not permit an ex¬ amination into the political importance of the Danube. From various circumstances, it has been, and still is, closely connected with the interests of Europe. "While the other great rivers", says the American Cyclopaedia, "flowing in a northerly or southerly direction, formed barriers against the invasions of savage nations, the Danube, on the contrary, served as a highway from East to West. Hence, the ebb and flow of the great migration of nations, subsequent to the downfall of the Roman Empire, were the strongest in the basin of the Danube, and, for long centuries, the fate of European civilization depended on the contest of races, in that portion of the continent." (495.) The Main (PI. V. A and B). — We have de¬ parted from our general plan in giving a more detailed account of the Rhine and the Danube, because of the commercial, historical and political importance of those streams. They are examples of rivers by the influences of 216 SOUTH-WESTERN EUROPE. which Europe has taken the lead in civilization. The River Main must not be passed over without a few words. It is the most considerable branch of the Rhine, flowing, for many miles, through a mountainous country, which would otherwise be, in a great degree, closed to commerce and ideas. It opens a communi¬ cation with the south-western sources of the Weser; and, what gives it a still higher value, connects the basins of the Elbe, the Rhine, the Neckar and the Danube. By its westerly course, and connection with the Rhine, it also opens central Europe to the N., the W. and the E. Moreover, Germany is divided by it into N. and S. Germany. It has its source in Bavaria. Traversing the northern portion of that kingdom, it grazes the southern frontier of Hesse-Cassel, intersects the territory of Frankfort, leaving the city of Frank¬ fort on its right or north hank, cuts the G. D. Hesse- Darmstadt into two, almost equal, parts; and then, advancing between the southern part of Hesse-Darm¬ stadt and the D. Nassau, enters the Rhine at: Mainz (or Mayence). Now remark the southern limits of the new North German League, on PI. V. B, and we see an instance of the influence which a river may exercise on political events, arresting the advance of conquering armies and determining, at least for a time, the extent of territories. The south limits of the new N. German League nearly follow the course of that river. Thus may be explained the fact that Germany has been broken into two parts. The new and greatly strength¬ ened Prussia had reason to believe she would not be permitted to pass below the Main, and become sole possessor of that important international highway. Hence, the south limits of the Prussian League, following the course of the Main, take in only the Thuringian States — Hesse-Cassel, the northern half of Hesse- Darmstadt and Nassau—leaving out Baden, the southern half of Hesse-Darmstadt, Wurtemberg and Bavaria. It may be added that, in territorial arrangements, the lower portion of the river has generally been separated SOUTH-WESTERN EUROPE. 217 from the upper. Segments of the Rhine and the Danube formed boundary lines of the old Roman Empire, whose frontiers intersected the Main. Distance, in a direct line, from source to mouth, about 157 miles; but its windings, more peculiar and extensive tban those of any other German river, measure 3C0 miles. (496.) Towns of Portugal. — Seaports: Oporto —^Lisbon — Setubal, or St. Ubes— Lagos. Interior towns: Braganza — Braga — Almeida— Coimbra. Name rivers of Portugal. 'What town on Tagus? On Douro ? (497.) Towns of Spain. — Seaports on Mediter¬ ranean: Barcelona — Ï arragona — Castellon-de- 1 a-Plan a — Valencia — Alicante — Cartagena — Almeria — Malaga — Gibraltar (British fortress and town) — Tarifa. On Atlantic: Cadiz—Santa Maria — Xeres — Palos — Coruna — Ferrol. On Bay of Biscay: Gijon (he-hon') — Santander — Bilboa or Bilbao — San Sebastian. Towns not seaports nearest Atlantic and Bay of Biscay: Santiago — Oviedo — Astorga — Leon —Palencia—Valladolid — Bur¬ gos. Nearest the Pyrenees frontier: Pamplona, or Pampeluna — Saragossa — Lérida — Gerona. Nearest Mediterranean: Tortosa—Murcia—Granada — Cordova — Sevilla. Nearest Portugal: Badajos — Alcantara — Ciudad Rodrigo — Zamora. Central Towns: Segovia — Escurial — Madrid — Cuença — Albacete—Ar an juez—T ole do —Tal a ver a. Towns of the Insular Provinces: Palma on Majorca — Port- Mahon, capital of Minorca—Santa Cruz, capital of the Canary Is.— Iviza, on 1. of Iviza. Remark. 1. Pahs was the port from which Columbus sailed (1492); and to which he returned, after having dis¬ covered the New World. At the gates of the convent, La Rabida, in the neighborhood of Palos, he had once begged a crust of bread. The ruins of the convent yet remain. 2. From Santa Maria, is exported the celebrated sherry 218 SOUTH-WESTERN EUROPE. wine, the name of which is a corruption of Xeres, where it is chiefly manufactured. Name rivers of Spain ? Towns on or near the Guadal* - quiver? on or near the Tagus? on the Ebro? (498.) Towns of France. — On Mediterranean (seaports): Monaco—Nice (neess) — Antibes (an-teeb) —F rej us —T oulon —Marseilles — Cette. Nearest Spain: Perpignan — Pau (pô). -Bay o/ 3iscay (seaports); Bayonne with Biarritz — Bordeaux (Bor-do') — Rochefort —La Rochelle —Nantes-*- L'Orient Brest. British Channel (seaports)'. Cher- burg (Share-burg) — Caen (Kan)—Rouen (Roo-en) — Havre (Hah'-vre) — Dieppe — Boulogne (boo-lon'). On Strait of Dover: Calais—^Dunkirk. Nearest Bel¬ gium: Lille — Arras. (Ar-rah) — Cambray — Laon — Rheims (rîmes). Nearest Luxemburg, Bhine Province, Rhenish Bavaria and Baden: Metz—Nancy—Stras¬ bourg—Mülhausen, or Mulhouse. Nearest Switzer¬ land: Besançon (Be-san-son). Nearest Italy: Cham- bery — Grenoble. Interior towns: Aix (Aeks) — Avignon — Nimes (neem) — Montpellier — Nar- bonne — Toulouse — Perigeux — Angoulême — Limoges—Poitiers—Angers —Tours — Le Mans. Fontainebleau (blö)—Paris with Versailles — Amiens —Châlons (sha-long) — Troyes—Dijon — Autun — Lyon —Vienne —Valence —Etienne — Clermont—Moulins —Bourges — Orleans. What french towns on Garonne? on Loire? on Rhone? on Rhine? (499.) Towns of Belgium. — Antwerp — Malines or Mechlin — Brussels with Waterloo — Louvain — Liège — Namur — Möns — Ghent — Bruges — Ostende. Name rivers of Belgium. What towns on the Scheldt? Meuse? (500.) Towns of Holland. — Groeniugeu— Zwolle — Arnhem — Utrecht — Nymvegen, or SOUTH-WESTERN EUROPE. 219 Nimeguen —Dort—Rotterdam —Hague —Ley- den — Amsterdam — Haarlem — Maestricht — Luxembourg (in Prov. Luxg. PI. V. A). What dutch towns on Rhine? Meuse or Maas? (501.) Towns of Denmark. — Copenhagen — Elsiueur (on I. of Seeland) — Odensee — (on I. of Funen) — Aalborg — Aar hau s. (502.) Towns of P russia. — Name 16 present provinces of Prussia (PI. V. A and B). Pomerania: Stralsund — Putbus — Stettin — Col berg. W. and E. Prussia: Dantzic — Elbing—Koenigsberg — Tilsit —Memel —Insterburg —Thorn. Posen or Prussian Poland: Posen — Bromberg. Prussian Silesia: Goerlitz —Liegnitz —Breslau—Neisse — Glatz. Prussian Saxony : Magdeburg—Wittenberg — Torgau — Halle. Brandenburg: Brandenburg — Berlin — Spandau—Potsdam — Cus tri n —F rank- fort-on-the-Oder. Westphalia: Minden — Biele¬ feld— Munster. Rhine Province: Crefeld — Elber¬ feld— Dusseldorf— Cologne — Aix-la-Chapelle — Bonn — Coblentz — Kreutznach — Treves. Hohenzollem: Hechingen — Sigmaringen. Hano¬ ver: Hanover — Goettingen. Hesse-Cassel: Cassel. Frankfort-on-the-Main: Frankfort - on - the - Main. Nassau: Wiesbaden — Ems. Hesse-Homburg: Hom¬ burg. Holstein with Lauenburg: Rendsburg — Kiel — Gluckstadt — Altona. Schleswig: Flensburg — Schleswig. (503.) Towns of the other States united in new North German League. — Mecklenburg- Schwerin: Rostock — Schwerin— Ludswigslust. Mecklenburg - Strelitz: Strelitz. Oldenburg: Olden¬ burg. Northern half of Hesse-Darmstadt: Glessen. Brunswick: Brunswick. Anhalt: Dessau. Wal- deck: Arolsen. Ldppe-Detmold: Detmold. lAppe- Schaumburg : Buckeburg. Schwarzburg - Rudolstadt : 220 SOUTH-WESTERN EUROPE. Rudolstadt. Schwarzburg-Sondersharisen: Sonders¬ hausen. Thuringian States: Altenburg — Weimar — Gotha—Eisenach. Saxony: Leipsic—Dresden Freiberg — Chemnitz. Free Cities: Bremen — Hamburg — Lübeck. (504.) Towns of the South German States. — Baden: Manheim — Heidelberg — Carlsruhe — Baden-Baden — Constance —F reí burg. Wurtem¬ berg: Stuttgard. Bavaria: Wurzburg — Bamberg — Nuremberg— Ratisbon— Ulm — Augsburg — Landshut — Passau—Munich. Rhenish Bavaria: Speyer (or Spire, Spires) — Landau. Hesse- Darmstadt: M'entz (or Mainz — Fr. Mayence) — Darmstadt — Worms. I (504 A.) Remark. 1. Rhenish Bavaria. —Hhe little territory, on the right bank of the Rhine, sometimes called the Palatinate, because it formed part of one of the old circles of Germany, bearing that name before the French revolu¬ tion of 1789 (PI. V. A. fig. 1), is now a province of Bavaria. 2. Speyer. — The name, Protestant, originated at the Diet held in Spires (1529). The Roman Catholic members, act¬ ing for the Pope and the Emperor of Germany, had passed a resolution, that no further innovations in religious matters should, for the present at least, be allowed. Against this, the Evangelical Estates entered their solemn Protest, declar¬ ing their readiness to obey all orders of the Emperor, except such as they deemed repugnant to "God and his Holy Word." 3. Worms.—Many diets were also held at Worms. That of 1521 is the most celebrated, from the fact that Luther appeared there, in presence of the Emperor Charles V, the princes and nobles of the empire, the dignitaries of the Church, and an immense concourse of spectators. Instead of recanting his doctrines, which seemed the only way to save himself from being burned alive, he boldly reiterated them; and proclaimed, still more solemnly, his conviction of their truth, adding: "Here I stand! I cannot otherwise! God help me! Amen!" 4. Augsburg — is also famous for many events, partic¬ ularly the diet of 1530, at- which the well known Confession SOUTH-WESTERN EUROPE. 221 of Faith, called the Confession of Augsburg, drawn up by Melanchton, and subscribed by the Protestant princes, was publicly presented to the Emperor Charles V. Name rivers of German States (Austria being excluded). What german towns on Rhine? Main? Aar? Moselle? Weser? Elbe? Oder? Vistula? (505.) Towns of Austria (PI. VI. B). — Bohemia: Eger — Carlsbad — Prague — Teplitz —Reichen¬ berg — Gitschin —Trautenau — Nachod—Koe- niggraetz (battle-ground 1866) — Bud weis — Pil¬ sen. Austrian Silesia: Troppau. Moravia: OXmutz — Brunn — Austerlitz. Upper Austria: Linz — Ischl. Lower Austria: Vienna—Neustadt. Styria: Graetz. Salzburg: Salzburg — Gastein. Tyrol with Vorarlberg: Innsbruck — Bötzen — Trent. Carinthia: Klagen¬ furt. Çarniola with Istria: Laibach — Goritzia, and the territory and townshipof Trieste. Hungary : P r e s - burg — Comorn — Schemnitz — Kremnitz — Neu¬ sohl— K ase h au—Tokay—Miskolcz—Debreczin — Gross war dein,Sz egedin (seg'ed-in)—Temes war —Neusatz—There si opol —Punfkirchen—Stuhl- weissenburg — Pesth — Buda — Raab — Oeden- burg. Oalicia with Cracow: Cracow — Wieiiczka — Lemberg — Brody. Bukowina: Czernowitz. Tran¬ sylvania: Klausenburg — Maros — Vasarhely — Kronstadt— Karlsburg—Hermanstadt. Slavonia: Peterwardein — Semlin. Croatia: Agram — Carl¬ stadt— Fiume. Dalmatia: Zara — Spalato — Ra¬ gusa— Cattaro. Remark. Cracow—ancient capital of Poland — (after Congress of Vienna, a small independent republic,) was annexed to Austria in 1846.— Wieiiczka (Vee-litch'-kah) —celebrated for magnificent mines of rock-salt — contains a subterranean town, with streets, churches, statues, etc., all out of the solid salt-rock. Within the mines are a small lake, a rivulet of fresh water, and a chapel hewn out of rock-salt. 222 SOUTH-WESTERN EUROPE. (506.) Military Frontier — is not strictly speaking, a province. The strip of country so called, extending along nearly the whole Turkish frontier, from the Adriatic eastward to Moldavia, and consisting of portions of Croatia, Slavonia, the Banat and Transyl¬ vania, was, in 1807, erected into a kind of military organization, as a protection against the Turks. It is no longer of any importance, although the name is still used. (507.) Towns of Roumania. — Moldavia-. Bo- tuschani—Jassy (yas-see)—Galatz—Kilia. Valakhia: Braila (or Ibrail) — Bucharest (or Boo'kar-esht) — Giurge vo — K raj o va. Remark. Kilia, a fortified town on one of the mouths of the Danube, was ceded to Turkey by the Treaty of Paris, 1855. (508.) Towns of Turkey in Europe. — Bosnia with Turkish Croatia, and Herzegovina-. Banyaluke — Travnik — Serajevo (or Bosna Serai) — Mostar (Herzegovina.) Servia: Belgrade—Kragnyewatz. Bulgaria with Dobrodja or Dobrudja: Vidin — Sistov or Sistova — Rustchuk — Silistria — Sulina — Kostendje — Varna — Schumla — Sofia. Rumelia: Nish—Uskub—Philippopli (or Philippopolis)— Slivno —Burgas—A drianople — Constantinople (or Stambul) — Rodosto — Gallipoli — Seres — Salónica — Bitolia. Albania with Thessalia: Scu¬ tari* — Durazzo"— Avlona — Yanina — Larissa. Montenegro: Cettinie. Candia: Kanea — Rithymno — Candia, or Megalo Kastro — Gerapetre. (509.) Towns of Greece. — Rumelia: Zeitoun or Lamia — Mesolonghi — Lepanto — Thebes — * Rot to be confounded with Scutari in Asia Minor, oppo¬ site Constantinople. eODTH-WESTERN EUROPE. 223 Athens — Piraeus (port of Athens). Morea: Patras — Corinth — Argos — Nauplia — Tripolitza — Sparta — Navarino. Ionian Is.: Corfu (on I. of Corfu). Cyclades: Syra (on I. of Syra). Grecian Sporades: Chaléis (Egripo or Negropont on I. of Euboea) — Hydra (on I. of Hydra)—Egina (on I. of Egina). (510.) Syra or Hermopolis — capital of the govern¬ ment Cyclades — residence of consuls from most European States — principal station of Mediterranean steamers going to and from Constantinople — harbor accessible to large ships. Corinth. — Paul addressed two Epistles to its inhabitants. (511.) Towns of Italy. — Piedmont: Aosta — N ovara—Turin —Alessandria—Cuneo—Savon a — Genoa—Sp'ezzia. Lombardy: Sondrio—Ber¬ gamo — Como — Milan — Pa vi a— Cremona — Sol¬ ferino — Brescia. Venetia: Belluno — Udine — Treviso — Venice— Chiozza —Padua —Legnago (len-ya'go) — Mantua — P eschiera (pes-ke-a'-ra) — Verona—Vicenza. Emilia: Piacenza—Parma — Ferrara — Moden a — Bologna—Ravenna — Forli — Rimini — Carrara. Tuscany: Leghorn — Pisa — Lucca—Florence — Siena. Marca: Sinigaglia (se-ne-gal'ya)— Ancona—Macerata — Fermo. Em- bria: Perugia — Rieti. Naples: Gaeta — Capua — Naples — Porti ci — Pozzuoli — Castel-a-mare — Sorrento —Amalfi—Salerno — Cosenza —Reggio — Ca tan zar o —Taranto — Gallipoli — Otranto — Brindisi —Bari—Foggia— Chieti —Campobasso — Benevento — Potenza-. 7. of Sicily: Palermo — Messina — Catania — Syracuse — Girgenti — Marsala — Trapani — Nicosia — Caltanisetta. Papal States: Viterbo — Civita Vecchia — Rome — Velletri. I. of Sardinia: Cagliari — Sassari. Remark. Mantua, Verona, Peschiera, Legnago, form together the supposed impregnable fortresses, called the 224 SOUTH-WESTERN EUROPE. QuadrilateraL They were ceded, by Austria to France, and by France to Italy, 1866—Austria retiring from Germany and Italy at the same moment (468). (512.) Towns of Switzerland (PI. V. B). — Name cantons of Switzerland. Berni Bern — Thun. Soleure: Soleure. Basel: Basel. Aargau: Aarau. Zurich: Zurich. Schaffhausen: Schaffhausen. Thur- gau: Frauenfeld. St. Gall: St. Gall—Ragatz. Appenzell: Appenzell. Grisons: Chur (koor). Ticino: Lugano — Locarno — Bellinzona. Valais: Sion — Martigny — Lenk. Geneva: Geneva. Vaud: Lausanne — Vevey. Neu/châtel: Neufchâtel — Chaux-de-Fonds. Fribourg: Fribourg. Lucerne: Lucerne. Zug: Zug. Schwytz: Schwytz. Glarus: Glarus. Uri: Altorf (famous in history of W. Tell). Unterwaiden: Stanz. (513.) Lakes. — Nature appears to have gathered the lakes of Europe into two groups—one, distinguished by larger size, in the neighborhood of the Baltic; the other, generally more elevated above the sea, and marked by exquisite beauty of scenery, scattered among the Alps. In the Hungarian plain are several; and a large number, very shallow, are found in the low marshes of Holland. The entire area of the continental European lakes has been estimated at about 38,000 English square miles. Those situated around the Baltic, i. e. Ladoga, Onega, Wener, etc., (PI. II) comprehend more than five-sixths. They are all fresh-water, except the Neusiedler See and L. Balaton, both in Hungary. (513 A.) Remark. Plate II. figs. 1. 2. give a selection of the principal rivers of the world with their length; and the lakes through which they flow — the Rhine, through L. 'Constance, the Rhone through L. Geneva. The two lakes, through which the Nile flows, are the Victoria-Nyanza and the Albert-Nyanza (455). The student will do well to read over all those rivers in figs. 1. 2. with their respective lakes. SOUTH-WESTERN EUROPE. 225 (514.) Lakes of Austria. — L. Zirknitz (Ca- rinthia), 18 sq. m. — Neusiedler See, 150 sq. m., and Platten See (or L. Balaton) 250 sq. m. (the two latter in Hungary). (515.) L. Zirknltz contains numerous tunnels— like holes, 50 £eet deep, called sieves, through which the water alternately quite vanishes, then suddenly re-appears, so that a person can, each year, plant buckwheat, cut hay, fish and shoot water-fowl, in and on same spot. The water sometimes fills the whole hasin in twenty-four hours. The streams, which feed this lake, are also most curious; flowing, in part, on the surface of the earth, then suddenly vanishing, to re-appear again later. (516.) Lakes of Germany. — Koenigsee (Ba¬ varia). (517.) Lakes of Switzerland. — L. Constance or Boden See, 228 sq. m. — L. Qeneva, 240 sq. mk — L. Neufchatel, 115 sq. m. — L. Sempach, 4 sq. m. — L.Zurich, 76 sq. m. — L. Wallenstadt, 22 sq. m. — L. Zug, 135 sq. m. — L. Lucerne or Vierwaldstaedter See 99 sq. m.—L. Brienz, 12 sq. m.— L. Thun, 20 sq. m. Remark. Switzerland has more celebrated lakes, in proportion to its size, than any other country. They are surrounded by lofty mountains, and give, to scenery, already remarkable for magnificence, an additional and ravishing beauty. Vierwaldstaedter See—i. e. Four-forest cantons-lake. (518.) Lakes of Italy (PI. v. B). _ l. Mag- giore, 152 sq. m. — L. Como, 66 sq. m.—L. Iseo — L. Qarda, 183 sq. m. — (Ph VI. B) L. Perugia, or Tr asi me ne. 15 226 SOUTH-WESTERN EUROPE. (519.) Lakes of England. — L. Windermere — L. Dervent Water — L. Keswick — L. Bala (Wales). (520.) Lakes of Scotland, — Loch Lomond (lok) — largest lake in Scotland — twenty-four miles in length, and seven miles in its greatest breadth. It contains more than 30 islands. — Loch Awe — second in magnitude—Loch Ness — Loch Oich—Loch Lochie — Loch Leven — Loch Katrine. Remark. Scotland is remarkable for the number, great beauty and wild grandeur of its lakes ; some of them, in connexion with the deeply indented friths and estuaries which make its coast so striking, have been admirably used for purposes of internal navigation. The Caledonian Canal, one of the greatest works of modern engineering, connects the North Sea with the Atlantic. It is more than 60 miles long, of which 37 miles lie through Loch Ness, Loch Oich, Loch Lochie. (521.) Lakes of Ireland. — Lough Nea (loh-nay) — largest lake in the British Isles — twenty miles long (from north to south),' and ten in breadth — Lough Erne—area fifty-seven sq. m. Lough Allen — Lough Conn —Lough Mask —Lough Corrib — Lough Ree — Lough Derg — Lakes of Killarney, highly celebrated for picturesque beauty; upon their western side the highest mountains in Ireland rise steeply from the edge of the water. Remark. The word lough (lob), by which the lakes are distinguished (like the similar word loch in Scotland), is applied equally to inland lakes and to estuaries, or salt¬ water inlets. (522.) Wales (486). — S. W. portion of Gr. Britain — till 1536, an independent Principality—still retaining its name, from which the title, Prince of Wales —140 miles long — 90 broad — mountainous, Mt. Snowdon, culminating point of the whole island (PI. VI. B). PART Y. OUTLINE VIEW OF TOWNS, RIVERS, ETC. OP ÜNITED STATES OF AMEBICA. INTRODUCTION. (523.) It now remains for us to take a somewhat nearer view of the towns, rivers, etc., of the United States of America. This republic, is bounded N. by British America, from which it is separated by 49th parallel, great lakes, and St. Lawrence; E. by Canada (New Brunswick) and Atlantic; S. by Atlantic, Florida Str., G. of Älexico and Mexico; W. by Mexico and Pacific (from C. Flattery to town of San Diego). It comes in immediate contact with no foreign Power but British America, Mexico, and, since the recent purchase (424), Russia. On the S. E., Cuba and the rest of the West India Isles, bring it into certain relations with 6 European, and 3 American States (211—216. PI. III. fig. 3). Farther, on the N. E., lies the Danish Possession, Greenland, where the christian missionary, by a life of labor, danger and self-sacrifice, is silently carrying out the great work of his divine Master. The Unoccupied Arctic Lands are scarcely inhabited, except by the few Mongol 15* 228 UNITED STATES OP AMERICA. wanderersj originally from eastern Asia, called Esquimaux. Before particularly considering the U. States, it will be useful to take a brief survey of the other countries of N. America. (524.) Russian America, including (PI. 11.) Eodiak I., Sitka I., the Aleutian or Fox Is., and several other groups — lately, by purchase, N. W. territory of the United States in consideration of 7,200,000 dollars. We have thus acquired a part proprietorship in Behring Str., and in Mt. St. Elias. Our flag now floats within the arctic circle, about 71®*^ parallel—a point, where the sun, in summer, remains more than two months above, and, in winter, the same period below, the horizon. Remark (PI. II.) when it is 6 o'clock in the afternoon, on the Yenisei R. (Russia in Asia), it is 6 o'clock in the morning, at the mouth of the Mississippi; and about midnight, at the mouth of the Kwichpack. "Now", Senator Sumner remarks, "as the settlements of this coast came eastward, from Russia, bringing, with the Russian flag, western time, the day is earlier, by twenty-four hours, with them than with us; so that their Sunday is our Saturday; and the other days of the week are in corresponding discord. This must be rectified according to the national meridian". Population, about 54,000 (Esquimaux, Kenaians, Aleutians and other Indians — in 1866, about 900 Russians), generally fishermen and fur-hunters. This territory had never been actually taken possession of by the Russian government. The supreme authority was vested in a Russian Company, whose sole object was to collect furs. We are sepa¬ rated from the territory by British Columbia. (525.) British America — between Unoccupied Arctic Lands, Great Lakes and St. Lawrence — a colony of Gr. Britain, intersected by arctic circle — with a shattered and broken coast washed by dreary and desolate oceans — population (British and French), UNITED STATES OF AMERICA. 229 3,404,240, exclusive of about 155,000 Indians. Its chief political divisions are: Hudson Bay Company's Territory (including Labrador, Rupert's Land, Columbia, with Vancouver I.) — East or Lower Canada — West or Upper Canada, with Anticosti I. — New Brunswick — Nova Scotia, with Cape Breton I. — Newfoundland —Prince Edward I. The vast western region supplies the world (even including Russia) with furs. The fur-bearing animals are decreasing. Canada has a united population of about 2,500,000 — a considerable portion french, still preserving french customs and the Roman Catholic religion. Euperfs Land — central and chief division of the Hudson Bay Company's Territory — capital and principal trading station. Fort York — magnificent forests, vast prairies and a soil yielding European cereals. Red River Settlement — immediately N. of our northern frontier — thriving colony, with a good climate and fruitful soil — wheat, rye, oats, barley in great abundance — drained by the Assiniboin and Saskatchewan rivers — capable of supporting a dense population. Columbia (witb Vancouver I.)—sometimes called New Caledonia—capital, Victoria. Gold has been discovered near the Frazer River — single pieces worth 10 or 15 dollars. A digger has gained, sometimes, 50 dollars a day — one gained 213. Gold is found thickly scattered, not only over this region and California, but also over Washington Ter., Oregon, Idaho, Montana, Colorado and Arizona — generally side by side with silver and other mineral treasures. Vancouver I. — on 50"* parallel — formerly Quadra — in some parts, extremely fertile — splendid timber — rich in coal, fish, furs — excellent harbors — a position favorable for trade with Oregon, Russia, China, Australia — ceded to Gr. Britain (1846). Remark. — A Royal Proclamation, by the British government, took effect July 1, 1867, uniting into one 230 dnited ;statbs of america. Confederation, under the name of canada, the three provinces, Canada, New Brunswick, and Nova Scotia. (526.) Mexico — extensive coast on Pacific and G. of Mexico — intersected by tropic of Cancer — an immense plateau of plutonic origin, from 6 to 9000 feet high, ramifying into separate monntain- chains — population, nearly 8,000,000 — the only limitrophe* country of the United States on the S.— provinces adjoining United States: Tamaulipas, New Leon, Coahuila, Chihuahua, Sonora and Lower California — established religion and only one recognized by the government, the Roman Catholic—education, very backward. Mexico was a Spanish possession till 1810. General Iturhide suffered death by military execution (1824) for having a second time proclaimed himself emperor. Spain recognized the independence of Mexico in 1836. Since then Mexico has been in a chaotic state. In 1862, the Emperor Napoleon III. conceived the idea of placing an Austrian Prince, Maximilian, as emperor, upon the Mexican throne. The attempt to execute his plan by french bayonets, accompanied by enormous bloodshed and suffering, resulted in signal failure, and Maximilian was shot by the Mexican authorities. Slavery has been prohibited, hut the laborers on the great plantations (that is the haciendas) being deeply indebted to their employers, are said to suffer from a condition of thraldom, more insupportable than that of a negro slave. (527.) Cuba, this luxuriant and lovely island, just within the Tropics, has a peculiar interest, from its close proximity to the United States; and from the general opinion that, notwithstanding the prohibition of the slave-trade, that cruel traffîc has continued to he carried on. * Limitrophe — on the limits of. UNITED STATES OF AMERICA. 231 STATES AND TERRITORIES. (528.) The number of regularly organized states is 38. The number of territories, 10, besides a portion of land, 10 square miles, called District of Columbia, ceded, by Maryland and Virginia, as the seat of the national government, and under its immediate jurisdiction. The rapidly increasing population will probably soon transform the territories into organized states. In the following lessons, for the convenience of learning, we, at first, take states and territories together, without distinction. The list of territories will subsequently be learned apart. The states and territories are naturally divided into 12 groups. Where a state belongs, at the same time, to two groups, it will be repeated; as, for example, in the case of Florida, Texas, California, etc. The pupil is begged always to follow this rule in the series of repetitions. (529.) New England States. — Maine—New Hampshire—Vermont (R. these 8). Massachusetts — Rhode Island — Connecticut (R. these 3. — How manyi R. 6 from Maine). Remark. The name, New England States, has no political signification. The region, when a French possession New France, was afterwards called New England. AU these states touch the Atlantic, except Vermont. (530.) Other States touching Atlantic. — New York — New Jersey—Pennsylvania (R. these 3). Delaware — Maryland — E. Virginia (R. these 3. — R. from New York). N. Carolina — S. Carolina—Georgia (R. these 3. — R. from New York). Florida (R. — How many from New Yorkl R. these 10. — R. from Maine). 232 UNITED STATES OF AMERICA. (531.) Toacliing G. of Mexico. — Florida- Alabama— Mississippi (R. these 3). Louisiana — Texas (R. these 2.—How many from Florida? R. these 5. — R. from Maine). (532.) Touching Mexico. — Texas — New Mexico — Arizona (R. these 3). California (How many from Texas? R. these 4. — R.from Florida—R. from Maine). (533.) Touching Pacific. — California — Oregon—Washington (R. these 3. — R. from Florida — R. from Maine). (534.) Touching British America, W. of Lakes. — Washington — Idaho — Montana (R. these 3). Dakota — Minnesota (How many from Washington? R. these 5. — R. from Florida—from Maine). (535.) Touching Great Lakes. — Minnesota —W isconsin—Michigan (R. these 3). Illinois — Indiana—Ohio (R. these 3. — R. from Minnesota). Pennsylvania — New York (R. these 2.—How many from Minnesota? R. these 8.— R. from Florida—R. from Maine). (536.) Lake States which directly touch British America. — Minnesota — Michigan — New York (R. these 3, — R. states from Washington —from Florida—from Maine). (537.) Touching British America, £. of Lakes. — New York — Vermont — New Hampshire (R. these 3). Maine (How many from New York? R. these 4. — R. from Washington—from Maine). Remark. We have now named, how many (states and territories)? Thirty-four. How many remain yet unnamed, including District of Columbia? Fifteen. UNITED STATES OF AMERICA. 233 (538.) Interior States, W. of Mississippi. — Nevada — Utah—Wyoming* (7?. these 5^.Colorado ^Nebraska—Kan sas (B. these 3. — R. from Nevada). Iowa—Missouri — Arkansas (R. these 3.—R. from Nevada). Indian Territory.** (How many? R. these ^10.— R. from Washington—from Maine). (539.) E. of Mississippi. — Tennessee — Kentucky^—W. Virginia (R. these 3). Lastly, District of Columbia. (How many? R. these é.— How many states altogether? R. these 48, bearing, however, in mind that they include territories and one District). (540.) On Arctic Ocean. — The territory, till now called Russian America. (R. the whole 49). (541.) Ten Territories, July 1867. — Of these 49 divisions, 10 are as yet territories. By territory is meant those portions which, from want of sufficient population and other causes, are not yet organized as states. Washington — Idaho — Mon¬ tana— Dakota (R. these 4). Utah—Wyoming — (R. these 2.—R. from Washington Ter.).— Arizona — New Mexico — Indian Territory (R. these 3. — R. from Washington Ter.). Russian America. WATER DIVISIONS—LAKES —ISLANDS- CAPES. (542.) Water Divisions. — On the Atlantic, from B. of Fundy to Florida B. — Passamaquoddy B.— Machias B. — Frenchman's B. — Penobscot B.— * A section of Dakota is called Wyoming, by some maps, altbongh it has not yet been organized as a territory. ** The Indian Ter. is not, strictly speaking, a territory. It is a region set apart, by the government of the United States, as a home for certain Indian tribes. 234 UNITED STATES OF AMERICA. Cai^co B. — Massachusetts B.—Cap Cod B.— Buzzard's B. — Narraganset B. — Long Island Sound — New York B. — Little and Great Egg Harbor — Delaware B. — Chesapeake B. — Albemarle and Pamlico Sounds—Raleigh B. (raw'-lee) — Onslow B. — Long B. — Winyaw B.— Bull's B. — Charleston Harbor — Port Royal Entrance — Str. of Florida — Florida B. G. of Mexico, from Florida B. to mouth of Bio Grande. — Chatham B.— Oyster B. — Charlotte Harbor — Tampa B. — Appalachee B. — Appa- lachicola B.— St. Joseph's B.— Pensacola B,— Mobile B. — Mississippi Sound — Chandeleur B. — Atchafalaya B.—Vermillion B. — Galveston B.—Matagorda B.— Pacific, from, town San Diego to G. of Georgia. — Monterey B. — San Francisco B. — Str. of Juan de Fuca — Puget Sound — G. of Georgia. — On Lakes. — Keweenaw B. (L. Superior) — Green B. — Gr. Traverse B. (L. Michigan) — Mackinaw Str. and Saginaw B. (L. Huron) — Str. St. Mary — Sandusky B. (L. Erie). — Remark to the teacher. — In these sections, the principle of repetition can easily be applied. The pupil may be required, also, to repeat each state, with the water-divisions, islands, etc., belonging to it—as, for example, Maine-. Fassam- aquoddy B., etc. Where a name is not found on the large map, seek it on the corner-figures, 1 and 2. (543.) Lakes. — Maine-. Eagle Lakes—Grand L. — Schoodic Lakes (skoo'dic) — Millinoket — Moosehead — Moosotocmaguntic —Umbagog — Sebago. — New Hampshire: Umbagog — Ossipee Winnipiseogee — Sunapee.—Vermont: L. Cham- plain—L. Memphramagog.—New York: L. George — L. Champlain — Saranac— Black — Oneida — Skaneateles — Owasco — Cayuga — Seneca — Canandaigua — Crooked — Chautauque — Ontario — Erie.—Florida: L. George — Kissime ONITBD STATES OF AMERICA. 235 — Okechobee. — Louisiana-. Pontchartrain — Manrepas — Borgne — Calcasieu. — California-. L. Clear — Tulare — Soda. — Minnesota-. Red L. — Itasca L. — Leech. — Michigan-. L. St. Clair. — Wisconsin-. L. Winnebago. — Nevada: Pyramid L.—Walker L. — Oregon: Klamath L. — Summer L.— Sylvanille L, — Malheur L.— Abert L. — Idaho: Pend Oreille. — Montana: Flathead. — Utah: Great Salt Lake—Utah L. — Sevier L. — Salt L. — (544.) Islands. — In Atlantic: Mt. Desert I. — Nantucket and Martha's Vineyard — Block I.— Long Island and Staten Island — Roanoke I. — St. Helena Is. — Hilton Head I.— In G. of Mexico: Florida Keys—Pine Is.— Dry Tortugas Is.— Cedar Keys — Santa Rosa I. — Chandeleur Is.— In Pacific: San Clement I. — Santa Catalina — San Nicolas — Santa Cruz — Santa Rosa I. — San Miguel.-^ In Great Lakes: Group of Apostles —Isle Royale (L. Superior).— (545.) Capes. — In Atlantic: C. Ann — C. Cod — Sandy Hook — C. May—C. Henlopen — C. Charles — C. Henry — C. Hatteras — C. Lookout — C. Fear — C. Canaveral. In G. of Mexico: C. Sable—C. Romano — C. St. Bias. In Pacific: Pt. Conception — C. Mendocino — C. Blanco — C. Foulweather — C. Lookout — C. Flattery. RIVERS AND THEIR TOWNS. (546.) River basins. — The rivers of W. Con¬ tinent, in magnitude and extent of drainage, excel those of E. Continent. Remark three great river basins 236 ÜNITBD STATES OF AMERICA. inclined, first, to G. of Mexico — second, to Atlantic — third, to Pacific. Let us now consider the rivers flowing into G. of Mexico. (547.) Mississippi B. — marks boundary line between following states, right bank-. Minnesota — Iowa—Missouri—Arkansas—Louisiana; left bank: Wisconsin —Illinois — Kentucky — Tenessee — Mississippi — Louisiana. (548.) Branckes of Mississippi. — Among 50 mighty affluents we select the following, rißht bank: Minnesota—Upper Iowa R. — Red Cedar R.— Iowa R.— Des Moines — Missouri—White R. — Arkansas, largest tributary of Mississippi, after Missouri—Red River, formed by the confluencé of Washita and Bartholomew rivers. Left bank: St. Croix — Chippeway R. — Black R.—Wiscon¬ sin R.—Rock R. — Illinois R. with Fox R., Kan¬ kakee and Sangamon — Kaskaskia — Ohio — Obion R. — Hatchee R.—Yazoo with Sunflower — Big Black R. (549.) Towns on or near Mississippi. — Ft. Snelling — St. Paul — Stillwater — Prescott —Wabashaw — Prairie du Chien—Dubuque — Galena — Davenport — Muscatine — Burlington — Fort Madison — Keokuk — Quincy—Hannibal City — Alton — St. Charles— St. Louis — St. Genevieve — Kaskaskia — Cairo — Memphis — Helena — Arkansas — Napoleon — Columbia — Vicksbnrg — Natchez — Bayou Sara — Baton Rouge— Donaldsonville — New Orleans. Remark. — 1. The pupil, in repeating, will name the state or territory to which the town belongs. 2. The teacher will, here, also, at his discretion, apply the principle of repetition, as in sections 285. 287 and elsewhere. UNITED STATES OF AMERICA. 237 (550.) Towns on branches of Mississippi. — Iowa City — Des Moines — Batesville — Little Rock — Arkansas— Harrisonburg — Shreveport — Natchitoches (natch-i-totch'iz, often pron. nak-e- tush')—Alexandria— O pelo us as— Portage—Wa¬ te rtown — Janesville — Peoria— Springfield — Vandalia — Kaskaskia. — (551.) Missouri R. — flows from Rocky Mts. through Idaho Ter., Dakota — then between Nebraska and Iowa, by Kansas, through Missouri State, where it empties into the Mississippi. (552.) Branches of Missouri R. — Right bank: Yellow Stone with Big Horn and Powder R.— Little Missouri — North Fork — Shyenne — White R. — Niobrara R. — South Fork of Platte or Nebraska with Panee Loup or Wolf R.— Republican Fork — Smoky Hill Fork or Kansas — Osage R. — Gasconade R. — Left bank: Milk R. — James R. — Big Sioux — Little Sioux — Grand R. — Chariton R.— (553.) Towns on Missouri and branches. — Virginia City — Ft. Benton — Ft. Union — Ft. William — Ft. Clarke — Ft. Connor — Ft. Pierre —Yankton — Omaha City — Kearney—Nebraska City — St. Joseph —Atchison — Leavenworth — Platte City — Ft. Riley — Topeka — Lecompton — Wyandot — Independence — Jefferson City — St. Charles — Alton. (554.) Ohio R. — one of the most important —formed by the confluence, at Pittsburg, of the Alleghany and Monongahela with its branch, the Youghiogheny (yoh-ho-gay'-ny), flows through the following states, right bank: Pennsylvania — Ohio — Indiana — Illinois; left bank: Pennsylvania — W. Virginia — Kentucky. 238 UNITED STATES OF AMERICA. (555.) Branches of Ohio.— right bank: Beaver Cr. — Muskingum — Scioto — Miami — Wabash with Little Wabash—left bank: Little Kanawha — Gr. Kanawha — Big Sandy R. — Licking — Kentucky—Rolling Fork — Green R. —Cumber¬ land — Tennessee. (556.) Towns on Ohio and branches. — Main stream: Pittsburg—Alleghany City — Steuben- ville — Wheeling — Marietta — Farkersburg — Guyandotte — Portsmouth — Maysville — Cin¬ cinnati — Newport — Covington — Madison — Louisville—New Albany—H awes ville—E vans- vil le—Cairo — Branches: Nashville — Clarksville —* Ft. Donelson — Chattanooga — Decatur — Florence. (557.) Other Rivers, flowing into G. of Mexico.— Those East of Mississippi: Caloosahatchee — Pease Cr. — Suwanee R. — Appalachicola, formed hy the junction of the Chattahoochee and Flint — Choctawhatchee with Pea R.—Yellow Water—Escamhia—Perdido R.—Alabama, formed by Tallapoosa and Coosa — Mobile R. with Tom- bigby, Black Warrior and the E. outlet Tensaw — Pascagoula with Chickasawha and Leaf — Pearl R. — Those West of Mississippi: Calcasieu — Sabine R. — Neches R.—Trinity R. — Rio Brazos — Rio Colorado — Guadalupe — San Antonio — Nueces — Rio Grande del Norte. (558.) Towns on Rivers, E. and W. of Mis¬ sissippi. (Pupil will name each river.) — East: Atlanta — La Grange—Columbus —Montgomery — Mobile — Selma — Aberdeen — Columbus — Gainesville —Jackson. West: Austin — San Antonio — Corpus Christi — Brownsville — Ft. Fillmore — Mesilla —Belen — Albuquerque — Santa Fé—Taos. UNITED STATES OF AMERICA. 239 (559.) Rivers flowing into Atlantic. — St. Lawrence forms, in part of its course, boundary line between Canada and New York. Towm on British side: Toronto — Ottawa—Montreal—Quebec; on American side: Superior City — Sault St. Mary (so St. Mary) — Sheboygan—Milwaukee—Racine — Kenosha — Chicago — Grand Haven — Port Huron—Detroit — Monroe—Toledo — Sandusky City— Cleveland —Erie —Buffalo — Oswego — Ogdensburg. (560.) Penobscot R. — Maine— 275 miles — lovely scenery — large vessels ascend as far as Bangor —remarkable for a superior slate-quarry (on the branch, Piscataquis) — traverses nearly the whole state and is studded with a number of small islands. Towns: Bangor, Rockland. (561.) Eennebeck Maine — rises in Moosehead L. Towns: Moscow — Solon — Norridgewock — W aterville. (562.) Connecticut R. — longest and one of the most beautiful of New England — 400 m. — rising near Canada, separates New Hampshire from Vermont, and, after having traversed Massachusetts and Connect¬ icut, empties into Long Island Sound, at New London, one of the best harbors of the state. Towns-: Guildhall— Lancaster — N ew bury — Haverhill — Norwich — Hanover—Windsor—Char les town—Brattle bor o — Greenfield — Deerfield — Springfield—Hart¬ ford— Middletown. (563.) Hudson — 300 m. — flows out of the Adirondac Mts. into New York Bay, through enchanting scenery, rivaling that of the Rhine. Principal Towns: Troy—Albany—Hudson —P oughkeepsie —W est Point — New York — Hoboken. 240 UNITED STATES OF AMERICA. (564.) Delaware B. — 300 m. — rises in New York among the Katskill Mts. — flows through following states, right bank-. Pennsylvania, Delaware; left bank: New York, New Jersey. Ships of largest size come up to Philadelphia — steamboats to Trenton. Toums: Easton — Trenton — Philadelphia— Cam¬ den— New Castle—Wilmington. (565.) Susquehanna — largest stream in Penn¬ sylvania—length, 500 miles—traverses New York, Penn¬ sylvania, Maryland and falls into Chesapeake B. — numerous beautiful islands — navigation, obstructed by rocky rapids, carried on by two parallel canals. — Town: Havre de Grace. (566.) Potomac — Length, 350 miles — largest branch, Shenandoah—boundary between Maryland and Virginia — beautiful scenery — navigable for largest ships to Washington City. Principal towns: Cumber¬ land— Georgetown—W ashington —Alexandria — 8 miles below the latter. Mount Vernon, the former residence of Gen. Washington. (567.) Four Bivers flowing into Pacific. — Colorado (called also Colorado of the West) — length, with its branch. Green River, 1200 m. — forming part of boundary between California and Arizona—^.remark¬ able for the great defile, by which it has forced its way through the Rocky Mts. — precipitous banks, 1000 to 1500 feet high — tribes of Indians live along its shores — traces of ancient irrigating canals, showing that this region was formerly cultivated — a great tidal wave at its mouth renders the entrance dangerous except for vessels of light draught. Totm: Fort Y uma. Remark. There are two other American rivers of this name, one, the Rio Colorado, emptying into Matagorda B. (G. of Mexico), the other (Pi. II.), traversing the Argen¬ tine Confederation from Andes to Atlantic. UNITED STATES OF AHERICA. 241 (568.) Sacramento — large and important river — 500 m. long — draining, with its branch, the San Joaquin, the great central valley of California — navigable at all seasons to Sacramento, and for small vessels 150 m. farther. Tovons-. Shasta—Sacra¬ mento—Stockton. (569.) Columbia or Oregon B. — 1200 m. long—enters the Pacific — part of its course, boundary between Oregon and Washington. It is the largest of the Pacific rivers — navigable 145 m. up. Tovons: Ft Walla-Walla — Ft. Vancouver. (570.) Ewichpack or Yucon (Plates IT. IV.) — great river of the yet unnamed N. W. territory of the United States — length, with its windings, 1500 m.— rises in the Rocky Mts. and enters into Behring Sea (Pacific). The Kwichpack and Yucon are considered, by some geographers, to be one river, as on our maps. (571.) The Mississippi — ("Great Water" — "King of American streams") — with its tributaries, one of the largest river systems of the globe, draining one-seventh part of north american continent. It rises in the highlands of Minnesota State, at a place called Hauteur de Terre, W. of L. Superior — length, from L. Itasca, the source of Mississippi proper, 3,200 m.; but, from the source of the Missouri, the main branch, 4,350 m. Flowing, at first, through majestic primeval forests, the solemn uncleared land of the red Indian, from a point, where the earth is covered, a great part of the year, with snow and ice — then, along tracts marked by moss, the fir-tree, and other northern vegetation — it rolls on, between ever changing shores — by populous and rapidly growing cities — receiving, from the Rocky Mts. and Alleghanies, as it advances, about 50 mighty affluents which, in Europe, would be called important rivers — bearing upon its bosom, night and day, hundreds of immense steamers, crowded with human 16 242 ÜKITED STATES OP AMERICA. beings, it sweeps through vast, monotonous savannahs covered with long grass — plantations of sugar-cane, cotton and fruits of the south — into G. of Mexico, at a point where snow and ice are unknown phenomena, and where the odors of the orange, lemon and magnolia are wafted by the breezes of a perpetual summer. There are several falls, among others, those of St. Anthony. It is studded with numerous islands. Its banks some¬ times rise into broken and precipitous bluffs, 150 to 750 feet high, intersected by deep ravines—gentle valleys opening on either side and waving with forests of pine, birch, maple and cedar — wide prairies and wood¬ lands — sometimes inundating its shores for a hundred miles — masses of timber annually drifting down its stream, occasionally forming floating islands covered with vegetation and fixing, into the bottom, the dread¬ ed snag*. As we approach its mouth, it becomes a rapid, desolating torrent, loaded vyith mud — breaking over its banks in immense freshets, forming there large lakes, inhabited by alligators and wild birds — sweeping away whole forests and producing the greatest disasters which are said to be increasing in frequency and extent. About four thousand million cubic feet of solid matter are annually brought down to the gulf. The formation of the delta, by these deposits, is supposed to have occupied a period of 67,000 years. "The facility", says M® Culloch, "afforded by the Mississippi, and its various tributaries, for internal navigation, are wholly unequalled, except, perhaps, by the Amazon and its tributaries, in S. America. In so far, indeed, as navigation is concerned, the Missis¬ sippi should be regarded, from its great depth and comparative freedom from shoals and cataracts, not so much a river as a vast, internal sea, a Medi- *) Snag: — in the western rivers of the United States, the trunk of a large tree firmly fixed to the bottom at one end, and rising nearly or quite to the surface at the other end, by which steamboats, etc., are often pierced and sunk (Webster's Diet.) UNITED STATES OF AMERICA 243 terranean, in fact—extending through all the central and most fertile portion of N. America; and enabling its remotest recesses, though 2,000 or 3,000 miles inland, to maintain a direct communication, by water, with the distant quarters of the globe. It is but yesterday, as it were, since the valley of the Missis¬ sippi began to be occupied by civilized man, and reclaimed from the wilderness; and its astonishing increase. in population and wealth is principally ascribable to the facility, afforded by this noble river, for its intercourse with the other parts of America, and of the world. The trade and navigation of the Mississippi is already, indeed, incomparably greater than that of the Ganges, the Danube, the Elbe, or any other river of the ancient continent. Let, then, the reader, who compares the commerce and importance of the Mississippi, at this moment, with its state only half a century ago, imagine, if he can, what it must be, when all the vast country between the Rocky Mts. and Alleghanies has been fully peopled, when New Orleans has become a second London, and large cities have been built on its most distant affluents! "Vast as are the natural capacities of the Missis¬ sippi for navigation, they have been, and, no doubt, will continue to be, greatly extended by canals and artificial means. It is already united with the grand chain of lakes and the basin of the St. Lawrence; and goods, taken on board at New York, may at present be conveyed to New Orleans without being unshipped, and conversely." (572.) Missouri (i. e., "Mud River") — longest tributary stream of the globe — rises in the Rocky Mts., about one mile distant from the Salmon R., one of the affluents of the Columbia. About 400 miles from its source, it has broken its way through a sublime and extraordinary ravine, 5 or 6 miles long and 150 yards wide, called the Gates of the Rocky Mts., whose black 16* 244 \ UNITED STATES OF AMERICA. granite cliffs rise 1200 feet perpendicularly. A short distance beyond, it pours its floods, during 16 miles, over the Great Falls, second only to Niagara, a descent altogether of 307 feet. These form the first absolute obstacle to navigation, from its mouth, at the Mississippi, (about half a mile wide and 2500 miles from its source). It flows through well-wooded valleys — extensive and beautiful meadows and plains, surrounded by distant and lofty mountains — through a boldly undulating country — by sterile and arid regions — by immense grassy prairies, where the elk, the white bear, the antelope and buffalo are followed by the huntsman, the trapper and the red Indian. It strikes the Missis¬ sippi at a point where that river, to which, in length and mass of water, it is greatly superior, has half completed its course. Some european geographers con¬ sider the Mississippi as only an affluent of this gigan¬ tic stream; but the subordinate rank of the Missouri is determined by the fact that it flows through regions deficient in wood and coal. Its sinuous channel is, more¬ over, sometimes shallow and interrupted by sandbars, snags and rapids, by timber embedded in its channel and by the impetuosity of its current. Some of these obstacles are obviously removeable. The entrance of the Missouri into the Mississippi is described, by Capt. Hall, as particularly striking. "It seemed as if the dirty Missouri had insinuated itself under the clear Mississippi, for we saw it boiling up at a hundred places. First, a small curdling white spot, no bigger than a man's hand, appeared near the surface, which rapidly swelled and boiled about, till, in a few seconds, it became as large as a steam-boat, spreading itself on all sides in gigantic eddies and whirlpools, in a manner astonishingly grand and striking. At other places, the two currents ran along, side by side, without the least intermixture, like oil and water; but this separation was never of long continuance, and the contaminating Missouri soon conquered the beautiful Mississippi: indeed, the stain is never for one moment got rid of, during united states of america 245 the 1,200 miles that the stream fuds over, before it falls into the G. of Mexico." (573.) The St. Lawrence. — The great lakes, the largest mass of fresh water in the world, pour their surplus floods into G. of St. Lawrence by St. Lawrence R., which may he said to rise at the source of the St. Louis, W. of L. Superior. It hears différent names in different parts of its course; between L. Superior and L. Huron—the St. Mary; between L. Huron and L.Erie — the St. Clair and Detroit; between Lakes Erie and Ontario — the Niagara; and from Ontario tO' the sea — the St. Lawrence. Total length, including windings,— 2273 m., of which nearly the whole is navigable. The Miamis River, western extremity of L. Erie, rises so near the northern affluents of the Ohio, as to aflTord means of communication between the lake and the Mississippi. The Niagara River, thirty-four miles in length, presents that great world- curiosity, the Niagara Falls, of which we here say nothing, except to quote the opinion of Prof. Ansted "that the recession of these falls is probably more rapid than is usually supposed, very considerable portions of the rock having fallen, within the memory of man; this is not to be wondered at, when 15 million cubic feet of water have been estimated to pass over it every minute." (574.) Rivers according to States. — Mainet (Fig. 2.) St. John with Aroostook, Allaguash,Wal- loostoock and St. Francis—St. Croix — Machias — Penobscot with Mattawamkeag and Piscata¬ quis— Kennebec with Dead R. — Androscoggin (an-dros-cog'-ghm) — Saco — Piscataqua. — New Hampshire'. Androscoggin — Saco — Piscataqua — Merrimac with Contoocook — Connecticut (Con- net'-i-cut).— Vermont: Connecticut with White R. — Batten Kill—Otter Creek — Onion R.— La Moille R. — Missisque. — MassachuselU: Merri- 246 UNITED STATES OF AMERICA. mac with Nashua—Charles R. — Blackstone — Connecticut with Chicopee, Deerfield and Westfield — Farming ton — Housatonic. — Rhode Island: Blackstone — Pawtucket. — Connectieut: T hames — Connecticut with Farmington — U ousatonic.—New York: (Fig. 1.) St. Lawrence with Oswegatchie and Racket R. — Saranac — Hud¬ son with Batten Kill—Hoosic—Croton — Mo¬ hawk R. with Schoharie—Delaware — Susque¬ hanna— Chenango — Chemung — Alleghany — Cattaraugus — Tonawanda — Genesee — Seneca — Oswego — Black R.—Pennsylvania: Delaware — Lehigh — Schuylkill (skool'-kil) — Susque¬ hanna with N. Branch, West Branch and Juniata—Ohio with Beaver, Alleghany, Clarion Creek, Youghiogeny (yoh-ho-gah'-nee) and Mo- nongahela. —Delaware: Delaware — New Jersey: Hudson — Raritan — Little Egg Harbor R. — Gr. Egg Harbor R. — Delaware — Maryland: Potomac. —E. Virginia: Shenandoa—Potomac—Rappahan¬ nock —Y ork R.— James— Appomattox— Staun¬ ton.— W. Virginia: South Branch of Potomac — Cheat R. — Little Kanawha—Gr. Kanawha with Elk, Gauley and Greenbrier — Ohio with Big Sandy. — N. Carolina: Chowan — Roanoke — Tar —^Neuse — Cape Fear — Deep R. — Catawba — French Broad — Yadkin — Dan.—S. Carolina: Little Pedee—Great Pedee — Lynch's Creek — Black R. — Santee — Con gar ee—W ateree — Broad R. — Saluda — Edisto — Comb ah ee—Sa¬ vannah. — Georgia: Savannah — Ogeechee — Al- tamaha(Al-ta-ma-haw') with Oconee and Ocmulgee — Santilla — St. Mary — Suwanee (su-wah'-nee) with Allapahaw— Flint—Chattahoochee — Eto¬ wah.— Florida: St. John's R. — Kissime — Caloo- sahatchee — Pease Cr. — Suwanee — Appalachi- cola —Chocktawhatchee — Yellow Water — Escambia — Perdido. — Alabama: Pea R.— Es¬ cambia— Tensaw — Alabama with Tallapoosa, UNITED STATES OF AMERICA. ■247 Coosa, Mobile (mo-beel'), Black Warrior, and Tombigby — Tennessee R. — Mississippi: Pasca- goula with Chickasawha and Leaf R. — Pearl R. — Big Black R. — Yazoo with Sunflower R. — Mississippi.— Louisiana: Mississippi with Red River and Washita — Âtchafalaya—Calcasieu — Sabine. — Texas: Red River — Sabine — Neches (Netch'-ez)^Trinity— Rio Brazos (Brah-zos) —Rio Colorado — Guadalupe — San Antonio — Nueces (Nwa'-ces) — Rio Grande del Norte—Pecos. — Cal¬ ifornia: Klamath R. — Sacramento — San Joaquin — Colorado—Minnesota: Mississippi — St. Croix — Minnesota—-Red River of the North — JliicAi- gan: Menomonee — Manistee — R. au Sable — Saginaw — St. Joseph's — Kalamazoo — Grand River — Muskegon. — Wisconsin: Menomonee — Wolf R.—W isconsin — Mississippi — Black R.— Chippeway—St. Croix.—Illinois: Ohio with Little Wabash—White R. — Wabash — Mississippi with Rock R. —Illinois with Fox and Kankakee — Sangamon — Kaskaskia — Indiana: Kankakee — Tippecanoe—Wabash (Waw'-bash) —White R. with West Fork and East Fork — Ohio. — Ohio: Ohio — Muskingum — Scioto — Miami — Sandusky — Maumee. — Nevada: Humboldt R.— Walker R. — Nebraska: Niobrara — Missouri — Panee Loup or Wolf R. — Nebraska or Platte R. — Republican Fork.—Kansas: Missouri—Re¬ publican. Fork— Smoky Hill Fork or Kansas — Neosho — Arkansas. — Iowa: Mississippi — Upper Iowa — Red Cedar — Iowa — Des Moines — Chariton — Missouri with Little Sioux. — Missouri: Mississippi — Grand R.— Chariton R. — Missouri with Gasconade — Osage—Current. — Arkansas: Mississippi —White R. with Black R. — Arkansas — Bartholomew — Washita. — Tennessee: Tennessee with Clinch, Holsten, Hi- wassee. Elk and Duck R. — Mississippi with Hatchee and Obion — Cumberland. — Kentucky: 248 TJNITBD STATES OF AMERICA. Ohio — Big Sandy R. — Licking—Kentucky — RollingR.— Green R. — Cumberland —Tennes¬ see— Mississippi.— Washington Territory. Okonagan —Columbia — Yakima.— Oregon: Willamette R. — Columbia R. — John Day's R. — Malheur R, — Idaho: Clark's Fork — Salmon R. —Lewis or Snake R. — Jfowiana: Missouri with Milk R., Yellow Stone with Powder R. and Big Horn R. — Dakota: Missouri with Big Sioux — Shayenne — James — Little Missouri — North Fork — Shyenne R. — White R. — Niobrora—Utah: Colorado with Green R. — Grand R. — San Juan — Sevier — Jordan. — Wyoming: Big Horn — Powder — Platte R. with Laramie — North Fork and Sweet Wa¬ ter R. — Colorado: South Fork of Platte R.— Republican Fork — Arkansas — Gunnison — Grand R. — New Mexico: Rio Pecos — Rio Grande del Norte. — Arizona: Colorado with Little Colo¬ rado—Rio Gila—Rio San Pedro—WilliamsFork. — Indian Territory: Red Fork of the Arkansas with Arkansas and Neosho — Canadian R. with North Fork of Canadian R. — Red R. with False Washita and North Fork. — District of Columbia: Potomac. (575.) Exercises on Rivers. — PL VI. A. — The States, E. of Mississippi, are here reproduced, upon a somewhat larger scale than on PI. VH., and without names, for a clearer view of the chief rivers. The teacher will read the arabic number and, the pupil, in reply, will name the river from the corresponding number on the map; and also the states through, or by which it flows. River 1. — St. Croix, boundary line between Maine and New Brunswick.— River 2. — Penobscot (Maine). — River 3. — Ken¬ nebec (Maine).—River 4.— Androscoggin (Maine, New Hampshire).— River 5. — Merrimac (New Hampshire and Massachusetts).—River 6. — Con¬ necticut R. (New Hampshire, Verm ont, Massachu- UNITED STATES OF AMERICA. 249 setts and Connecticut).— River 7. — Housatonic (Massachusetts and Connecticut). — River 8. — Hudson (New York and New Jersey).—River 9. — Mohawk (New York). — River 10. — Passaic (New Jersey).—River ÍÍ. — Rar i tan (New Jersey). — River 12.— Delaware (New York, Pennsyl¬ vania, New Jersey, Delaware).— River 13.— Schuylkill (Pennsylvania). — River 14. — Susque¬ hanna (Pennsylvania, Maryland). — River 15.— North branch of Susquehanna (New York, Pennsylvania). — River 16. — West branch of Susquehanna (Pennsylvania). — River 17. — Juniata (Pennsylvania).— Remark. — We now take the Ohio with its head waters and branches—first, the three rivers which unite to form the Ohio; then, the right bank branches, then, the left. Riveris. — Alleghany (New York, Pennsyl¬ vania). — River 19. —Youghiogeny (yoh-ho-gay'-nee) (Maryland, Pennsylvania).— River 20. — Monon- gahela (W.Virginia, Pennsylvania).—River 21. —Ohio (Pennsylvania, Ohio, Indiana, Illinois, W. Virginia, Kentucky). We now come to right hank branches. River 22. — Muskingum (Ohio).— River 23.—Scioto (Ohio).—River 24.—Miami (Ohio, Indiana). —River 25. —White R. and branches (Illinois and Indiana).—River 26.—Wabash (Ohio, Indiana, Illinois).—Now left bank branches—River 27. — Gr. Kanawha (N. Carolina, E. Virginia, W. Virginia).—River 28. — Kentucky (Kentucky) — River 29. — Cumberland (Kentucky, Tennessee). —River 30.—Tennessee (E. Virginia, Tennessee, Alabama, Mississippi, Tennessee again, Ken¬ tucky). Now back to Maryland and the Atlantic basin. River 31.-—Potomac (Maryland, E. Virginia).— River 32. — James R. (E. Virginia). — River 33.— Roanoke (E. Virginia, N. Carolina). — River 34. — Cape Fear R. (N. Carolina).—River 35.—Gr. Pedee R. (N. Carolina, S. Carolina). — River 36. — Santee R. (S. Carolina). — 250 UNITED STATES OF AMERICA. Remark. — The branches of the Santee, flowing out of N. Carolina, bear the names of Gongaree, Saluda, Broad and Wateree, River 37. — Savannah (between S. Carolina and Georgia).—River 38.—Altamaha with branches (Georgia).—River 39. — St. John's R. (Florida) — River 40.—Appalachicola with branches (Geor¬ gia, Alabama, Florida).—River 41.—Alabama (Georgia, Alabama).—River 42. — Mobile with branches (Alabama, Mississippi).—River 43.— Mississippi. States on right hank-. (Minnesota — Iowa — Missouri — Arkansas — Louisiana). — States cm left bank-. (Minnesota again—Wisconsin —Illinois—Kentucky—Tennessee—Mississippi — Louisiana). Now right bank branches. River 44. — Minnesota or St. Peters (Dakota, Minnesota). —River 45.—Iowa (Iowa).—River 46.—Des Moines (Minnesota, Iowa, Missouri). — River 47. — Missouri. — River 48.—White R. (Missouri, Ar¬ kansas),—River49.—Arkansas (Colorado, Kansas, Indian Territory, Arkansas).—River 50.—Red River (Texas, Indian Territory, Arkansas, Louisiana). Now left bank branches'. River 51.— Winconsin (Michigan, Wisconsin). — River 52.— Illinois (Illinois).—River 53.—Yazoo (Missis¬ sippi).—River 54.—Sabine R., (forming part of bound¬ ary line between Louisiana and Texas). — River 55. — St. Lawrence (boundary line for some distance between State of New York and Canada.) — River 56. — Ottawa (branch of St. Lawrence in British America.) (576.) ComparatÎTe Dimensions (Plate VI. A and B.) — These two maps are drawn on the same scale, that the comparative dimensions of countries, lakes, seas, etc., may be determined at a glance, or, more correctly, with a pair of compasses. The teacher will require no aid to lead the pupil through the proper exercises; — such as, for example, the following; Massachusetts corresponds in size to the Kgd. of UNITED STATES OF AMERICA. 251 Wurtemberg — Maryland to Holland — Ireland to Maine — the Atlantic coast of Spain and Portugal would reach from New York City to the southern frontier of N. Carolina, etc. (577.) Towns according to States. — Maine-. (Fig. 2.) Mattawamkeag — Calais — Eastport — Machias — Ellsworth — Bucksport — Belfast — Rockland — Waldoborough — Wiscasset — Bath — Brunswick — Portland — Saco — Biddeford — Wells — York — Berwick — Alfred — Paris — Andover — Farmington — Mos¬ cow— Solon — Dover—Old Town — Bangor — Newport—Norridgewock—^Waterville—Augusta — Auburn.— New Hampshire-. Lancaster — Fran- conia — Haverhill — Conway — Hanover with Dartmouth College — Plymouth — Ossipee — Gilford — Canterbury—Newport — Charlestown — Great Falls — Concord —Dover — Portsmouth — Exeter — Manchester — Keene—Winchester— Amherst—Nashua, Vermont: St. Albans — Derby —Irasburg— Guildhall—Danville—Burlington —Montpelier—Middlebury—Chelsea—Newbury — Norwich — Rutland —Windsor — Manchester — Bellows Falls — Bennington — Newfane — Brattleboro.— Massachusetts: Greenfield — Deer- field — Lowell — Lawrence —Haverhill — New¬ bury port — Andover — Gloucester — Lexington — Lynn — Salem —Nahant — Concord— Boston with Charlestown, Roxbury, Cambridge, Dor¬ chester — Dedham — Abington — Marsh field — Plymouth — Chatham— Barnstable— Nantucket — New Bedford — Fall River — Taunton—Wor¬ cester— Springfield — Chicopee —Northampton — Lenox — Pittsfield — Amherst. — Rhode Island: Smithfield — Pawtucket (half in Rhode Island and half in Massachusetts) — Providence with North Providence —Warwick — Bristol — Newport — South Kingston. — Connecticut: Sharon — Suffield 252 UNITED STATES OP AMERICA. — Stafford—Tolland — Norwich — Stonington — New London — New Haven — Bridgeport — Fairfield — N or walk — Stamford — Danbnry — Waterbnry— Litchfield — Middletown — Hart- fort.—New York: (Fig. 1.) NiagaraFalls—Lewiston — Lockport — Albion — Rochester —^'Oswego — Volney—Pnlaski — Sackett's Harbor—Watertown — Ogdensbnrg — Canton — Potsdam — M alo ne — Rouse's Point — Platts burg — Ticonderoga — Whitehall (Fig. 2.) — Caldwell — Queenshury — Sandy Hill—Saratoga—Johnstown—Schenectady — Cohoes — Lan sing burg — Troy — Albany — Hudson — Catskill — Saugerties — Kingston — Rondont — Poughkeepsie (Po-keep'-see) — Fish- kill—Newburg—West Point—Sing Sing—White Plains—New York—Brooklyn—(Fig. 2.) Hunting- ton—Greenport—Sag Harbor—River head—Islip — (Fig. 1.) Port Jervis — Monticello — Delhi — Binghampton—Owego—Elm ira—Bath—Angelica — Olean — Cub a — Ellicottville — M ays ville — Dunkirk — Buffalo — Batavia — Lyons — Can an¬ da ig ua — Geneseo — Geneva — Havana — Ithaca — Auburn — Syracus e — Salina — Cortland — Norwich —Cooperstown — Morrisville — Utica — Rome — Trenton Falls.— Remark. — The close proximity of populous and growing towns, particularly near New York City, requires the omission of various names, such, for instance, as, Yonkers r-Tarrytown—Green bur g—Morrisiana—Flushing —Newtown—Oyster Bay—Hempstead, and others. New Jersey. -(Fig. 1.) Newton — Belvedere— Orange City — Paterson — Jersey City — New¬ ark— Elizabeth — New Brunswick—(PI. Vll.) Princeton — Trenton — Camden — (i'ig- 2.) Hoboken. — Pennsylcarúax Oil City — Titusville — Erie — Athens—(Fig. 2.) Towanda — Milford — Wilkesbarre — (PI. VII.) Easton — Pottsville — Reading—Norristown—Philadelphia—Lancaster —Harrisburg—York—Chambersb urg—Browns- UNITED STATES OF AMERICA. 253 ville — Pittsburg — Alleghany City. — Delaware'. Wilmington—New Castle — Delaware City — Dover. — Maryland-. Cumberland — Hägers town — Frederick — Baltimore — Annapolis — E. Virginia: Winchester — Harpers Ferry — Alexandria — Fredericksburg — Charlottesville — Richmond —Williamsburg—York town — Fortress Monroe —Norfolk—Portsmouth—Danville—Petersburg —Abingdon—Lynchburg—Lexington—Staunton. —N. Carolina: We Id on—Edenton—Tarboro—Raleigh (raw'-lee) —Newbern—Wilmington—F ayetteville— Charlotte—Salisbury.—S. Carolina: Spartanburg— Yorkville — Camden — Columbia— Georgetown — Charleston—Beaufort—Barnwell — Hamburg — Abbeville—Anderson.— Georgia: Athens — Augusta —M i 11 edge ville — Savannah — Darien — Columbus — Macon — La Grange — Griffin — Atlanta. — Florida: Pens acola — Quincy— Talla¬ hassee— St. Marks—Fer nan din a — Jacksonville — St. Augustine — Key West.—Alabama: Florence — Decatur — Huntsville — Talladega — Mont¬ gomery—Mobile — S el ma — Gainesville—Tusca¬ loosa.— Mississippi: Holly Springs—Aberdeen — Columbus —Jackson —Vicksburg—Natchez.— Louisiana: Shreveport—Harrisonburg—Bayou Sara (bi'-oo-sah'-ra) — Baton Rouge — Madisonville — Lafayette—New O rleans—Algiers—Donaldson- ville — Opelousas — Alexandria — Natchitoches (natch'-i-totchiz). — Texas: Houston — Galveston — Matagorda — Corpus Christi— Brownsville — San Antonio — Austin. — California: Humboldt City — Shasta — Nevada —Marys vi lie — Placer- ville— Sacramento — Stockton—Sonora — Mil¬ lerton— Los Angeles — Ft. Yuma — San Diego — Santa Barbara — Monterey — San José — San Francisco — Benecia. — Minnesota: Minnea¬ polis— St. Paul — Ft. Snelling— Still¬ water—Hastings City—Redwing—Wabashaw— Winona — Mankato. — Michigan: Sault St. Mary 254 UNITED STATES OF AMERICA. — Saginaw — Port Huron — Detroit—Ypsilanti —Ann Arbor — Monroe — Kalamazoo — Jackson — Lansing — Grand Rapids — Grand Haven.— Wisconsin: Superior City — Green Bay—Oshkosh — Fond du Lac — Sheboygan — Milwaukee — Racine —Kenosha — Beloit — Janes vil le — Madi¬ son— Prairie du Chien — Portage — La Crosse — Beaver Dam —Watertown —Waukesha — Prescott.— Illinois: Galena — Rock ford — Chicago — Joliet—Aurora — Ottawa City — Galesburg — Peoria — Bloomington — Quincy— Jackson¬ ville — Springfield — Alton—Vandalia — Belle¬ ville— Kaskaskia— Cairo. —Indiana: South Bend — Fort Wayne — Lafayette —Indiauopolis — Richmond—Terre Haute—Madison—New Albany — Evansville. — Ohio: Toledo — Sandusky City — Cleveland — Steubenville — Zanesville — Marietta—Portsmouth—Chillicothe—Cincinnati —Hamilton—Dayton — Springfield — Columbus. — Nevada: Gold Hill—Virginia City — Austin — Jacobsville — Aurora — Carson City — Dayton. — Nebraska: Omaha City—Bellevue—Nebraska City—Brownville—Fort Kearney. — Kansas: Mar y s vi lie —Atchison—Leavenworth —Topeka — Lecompton — Lawrence —Wyandot — Mound City—lola—Ft. Atkinson — Fort Riley. — Iowa: Dubuque — Davenport— Iowa City — Muscatine —Washington — Burlington —Fort Madison — Keokuk — Oskaloosa — Des Moines — Council Bluffs. — Missouri: St. Joseph — Hannibal City — St. Charl es — St. Louis — St. Genevieve — Jefferson City — Lexington — Independence — Kansas City — Platte City. — Arkansas: Fayette- ville— Batesville — Helena — Arkansas — Napo¬ leon — Columbia — Camden — Fulton — Fort Smith—Van Buren — Little Rock — Pine Bluff. — Tennessee: CI arks vi lie — Leb anon— Knoxville — Chattanooga — Murfre es borough — Columbia — Memphis — Jackson — Nashville. — Kentucky: UNITED STATES OF AMERICA. 255 Covington—Newport — Mays vil le—Frankfort— Lexington — Bowling Green — Paduca— Hawes- ville—Louisville—Danville.— W. Virginia: Whee¬ ling— Parkers burg — Clarksburg — Charleston —Wyoming — Guyandotte. — Washington Territory. New Dungeness — Port Townsend—Whatcom — Olympia — Nesqually or Nisqually—Stei- lacoom — Ft. Walla-Walla — Ft. Vancouver — Pacific City. — Oregon: Astoria — Portland — Oregon City—Dalles City—Auburn — Jackson¬ ville— Empire City —Eugene City—Salem.— /doÄo: Lewis tone—Florence—Ft. Hall—Ho 11 a day — Silver City — Boisee City. — Montana: Ft. Ben¬ ton—Virginia City.—Dakota: Ft. Union — Ft. William — Ft. Clark — Ft. Pierre—Yankton.— Utah: Ogden City — Ft. Bridger — Gr. Salt Lake City — Leb i — Provo — Springville — Fillmore City. — Wyoming: Ft. Connor — Ft. Laramie.— Colorado: Central City—Denver City — Golden City—Colorado City.—Arizona: Prescott—Tucson —New Mexico: Taos — Santa Fé — Albuquerque — Belen — Mesilla — Ft. Filmore. — Indian Territory: Tbalequa — Ft. Arbuckle — Ft. Washita —Ft. Towson. —District of Columbia: Washington — Georgetown — Alexandria. (578.) Bemarks on United States. — We abstain from any historical sketch. The American youth must thoroughly study the history of his country, elsewhere. We translate and compress, however, a passage from a German work, "Meyer's Universum" more valuable as the unbiassed opinion of a foreigner. "In the U. States", says this writer, "we find all the natural conditions requisite for the existence of one single political organization, destined to become superior, in extent, power and prosperity, to the empires of Sesostris, Alexander and Augustus; and not equaled by any existing country. The Creator has spread, over this favored land, fertility— a uni- 256 UNITED STATES OF AMERICA. form facility of internal communication — a singularly vast and rich river-system (which Humboldt called the life-giving element, big with future consequences, and binding, by one common interest, the entire population' together), and a lavish abundance of the two most valuable minerals, coal and iron. These blessings have been bestowed, in the same degree, upon no other region of the globe. "Nature herself has imposed, upon the U. States, the necessity of erne permanent, political system. The exterior configuration and the structure of the interior surface, equally indicate that any separation can be but transitory. The South,* inspired by its separate interest, may dissolve its union with the North; Ibe West may break away from the East; but, they will speedily be compelled to reunite, by the want of natural, interior boundaries, and of all aids of disjunc¬ tion, in a land obviously formed for mutual intercourse. The struggles, and jealous competitions of independent states, would produce collisions; and the strongest Power would soon compel all the weaker, back again into one system, as the sun holds the planets in their orbits. One ultimate union must result from the peculiar configuration of the great interior river-basin, which, by its remarkable uniformity, necessitates a corresponding uniformity in language, customs and political organization. Hence the rapid transformation, and amalgamation, of the affluent heterogeneous nationalities; often erroneously ascribed to the striking assimilation-power of the anglo-american race. It was the obvious will of God, as, in contrast to the structure of the eastern half of the globe, he modeled the outline of the new continent, that it should be the seat of one great nationality, of sufficient power to assimilate to itself all tributary elements. Nature has equally indicated the Ü. States as the * This, bear in mind, 'was written before the abolition of slavery and before the great rebellion. UNITED STATES OF AMERICA. 257 seat of one democratic and commercial state, which, as such, must be inspired with a passion for enlarging its territory. Its position, between the two great oceans of the globe, and the vast number of internal rivers, invite the American to navigation and foreign commerce. Agriculture and trade possess less attraction. The native American is more likely to become a merchant or mariner, than a farmer; and to leave the laborious, and less profitable cultivation of the soil, to the european emigrant. Commerce, however, developes the lust of gold, habitual excitement and the spirit of speculation. Should the population increase in the past pro¬ portion, this country will reach its culminating point in about 400 years. In the mean time, it offers ample room for the immense european emigration. It will then have a population of 500 millions. As the price of labor becomes cheaper, and the resources of the soil and industry, the' mines, the waterpower, steam, etc., shall be fully developed, it will supply all the countries of the earth with its produce and manufactures. If it be true that Europe has, during so many centuries, held the sceptre of the Old World, because of its superiority, to Asia and Africa, in the commer¬ cial, and other facilities, offered by its broken, indented coasts, peninsulas, bays and seas, and its interior river-systems — what a role is reserved for the United States, which, in extent of coast, internal lakes, seas, natural and artificial navigable streams, etc., already surpass Europe fivefold; and whose colossal mineral and other resources increase with every year." We cannot lay the above remarks before the American youth, without reminding them, that the great world - empires, described by history, fell into corruption and decay, because of their lust for gold, their ambition, pride, luxury, and sensual enjoy¬ ments, their ignorance of, or disobedience to, God. The american continent, thus wonderfully constructed, was, doubtless, at a later period, given to man, that 17 258 REMARKS ON EARTH'S SURFACE. he might build up a great political fabric, upon a -new system, more in harmony with the lessons of experience and with the light of Revelation. This is our mission as a people. It should be our aim to surpass other nations, not in wealth, luxury, pride, territory and military conquests, but in virtue, temperance, justice, righteousness, humility, faith in God and obedience to his Word. These, and these only — no virgin continent, no river-system, no gold mines, no form of government, without them — will permanently' secure peace, liberty and christian civilization^ MISCELLANEOUS REMARKS ON EARTH'S SURFACE. (579.) Let us now rapidly (PI. II) cast our eyes over the rest of the earth's surface, and mark the principal plains, table-lands, etc. And first, America (here read section 247). (580.) Plains and Valleys of N. America. — One vast plain extends from Arctic Ocean to G. of Mexico, and from Alleghanies to Rocky Mts., interrupted only by a more elevated region, near the parallel of the five lakes. A large portion is covered with immense, magnificent forest trees, while hundreds' of square miles are occupied by monotonous tracts of sand, clothed only with gigantic pines, denominated pine-barrens. That part, N. of parallel intersecting the five lakes, is, in a great degree, characterized by the sterility of the frigid zone; but the rest (an area of one and a half million square miles) is of almost unexampled fertility. Some parts of this plain, in the northern United States, bear- the name of prairies, — in the southern, savannas (144, 145). This plain, in the United States, being bounded on the E. and W. by mountains, forms three principal valleys: the valley of the St. Lawrence, the great valley of the Mississippi and the valley of the Ohio. REMARKS ON EARTH'S SURFACE. 259 (581.) Plains and Valleys of S. America. — The eye here easily follows several great valleys, spreading into vast plains; the valley of the Orinoco — the valley of the Amazon — the valley of the La Plata or Parana. The most' level part of the earth's surface is said to be a tract in the valley of the Orinoco, greater in extent than France, a large part of it entirely destitute of trees', called llanos (146 — 149). The plains of the Amazon valley are called silvas, from their mighty and impenetrable forests occupying more than one million square miles, 200,000 of which are annually laid' under water by the inundations of the Amazon. Humboldt says, these forests truly merit the name of "primeval". "The intense, tropical heat and the abundant' moisture acting upon the wonderfully rich soil has", says Prof. Ansted, "produced an inconceiv¬ able exuberance of vegetable and animal life, which actually offers a bar to civilization as great as the sterility of the African desert". Farther S., 25"' parallel, from the valley of the La Plata to Str. of Magellan, extend treeless plains, about 2000 miles in length and averaging 300 miles in breadth, called pampas. (582.) Plains and Valleys of Europe and Asia — are distinguished without difficulty. Observe the level parts of England, Scotland and Ireland, Wales'and North Scotland being mountainous. See what a stupendous plain, the largest in the world, crosses N. Europe, interrupted only by Ural Mts., and extends nearly to Behring Str. Leaning toward the N., it rolls its mighty rivers into the German and Baltic Seas and the Arctic Ocean. In different parts, it bears the local names — Sarmatian Plain, traversed by Oder, Vistula, Niemen and Dwina — Siberian Plain, that vast level of N. Asia, some frozen parts of which (PI. II.) are called tundras. — Kirghiz Steppes, in the neighborhood of Caspian Sea and Sea of Aral. Trace the valleys of the Danube (traversing the Hungarian 17* 260 REMARKS ON EARTH'S SURFACE. plain, 300 miles long, and from 300 tj 400 feet above the sea-level) — the Po (winding through the beautiful plain of Lombardy) — the Rhone — the Rhine — the Amoor — then the Ganges and Indus (flowing through the plain of Hindostán) — the Tigris and Euphrates, uniting into one stream. In south-eastern and Asiatic Russia, and in the flats of Tartary, these tracts are termed steppes (from a Russian word, signi¬ fying barren). A wilderness (in India called a jungle) differs from a desert, as being often covered with luxuriant vegetation. The term is applied also to wild, harren spots among rocky mountains, as, for ex. in Arabia. These plains, in various countries, have different characteristics. Here, they form a vast extent of frozen ground or snow — there, barren, burning -sands—here, luxuriant gardens of tropical vegetation — there, gloomy desolate wastes; now, a monotonous level, varied by moderately sized hills, without order or system — again, for many miles, the soil rises into long waves or undulations perfectly uniform in structure. (583.) Plains and Valleys of África. — The most remarkable plain of the globe is perhaps the desert of Sahara—about 2500 miles long by 1200 miles broad — extending from the valley of the Nile to the Atlantic and even projecting its submarine sand-banks, far beyond the coast, into the ocean (PI. III).. The eastern and more favored portion, known as the Lyhian Desert, is generally formed, not of sand, but of hard, horizontally-bedded sandstone rock, perfectly smooth and level. The western portion is one white, solitary, desolate, awful sea of burning sand. "No animal — not even an insect—breaks the dread silence; nor is a tree or a shrub to be distinguished during days of incessant travel. In the glare of noon, the air quivers with the heat reflected from the red sand, and the night is chilly, under the clear sky sparkling with its host of stars" (Ansted). Oases, however, (151) are found KEMAKKS ON EARTH'S SURFACE. 261 at intervals. Among the frightful features of this desert are the simoon, a hot, dry wind which, sometimes, for 12 hours, so fills the air with sand, as almost to obscure the sun — and the absence of rain, except during short intervals, sometimes 20 years apart. Hot springs are found, surrounded by a luxuriant vegetation — salt mines, etc. Caravans cross it in various directions, in danger of death and great suffering, from thirst, and from exposure to the simoon. (584.) Desert of Kalahari — in the southern extremity of Africa, between Orange R. and L. Ngami (Pi. II.), sometimes called the South African Sahara, although, by no means, an uninhabitable, sterile waste. It is occupied by the Bushmen and the black Kalahari, and inhabited by immense numbers of wild beasts: ostriches, antelopes, buffaloes, elephants, giraffes, lions, leopards, panthers, hyenas, etc. A part lies within the tropics. The surface is sometimes a waterless, sandy waste, sometimes a vast sea of grass which, on the E., is succeeded by thick impenetrable forests. The town, Lattako, lies in the neighborhood. (58o.) Table-lands, etc., of N. America. — Thousands of feet above these lower plains, spread the higher table-lands or plateaux, found not only on Aîontinents, but on islands. In N. America, the great plain of Mississippi R. rises on the N. to the heights before mentioned, about the parallel of the five lakes, and on the W., to. a wide and lofty plateau, 7000 to 9000 feet high which occupies a great part of Mexico and extends also to California, where its elevation is about 6000 feet above the sea. (586.) Table-lands of S. America. — Besides the elevated tracts of the Guiana and Brazilian Mts., the summit of the Andes presents table-lands of more limited extent, but far greater height. That of Desa¬ guadero (Bolivia and Peru) — 500 miles long, 50 miles 262 REMARKS ON EARTH'S SURFACE. broad, including L. Titicaca and city of Potosi — lies higher than 13,000 feet. The table-land of Quito is 10,000 feet high — 200 miles long — 30 miles broad. (587.) Table-lands of Europe and Asia. — In Europe, the central plateau of Spain rises 3000 feet. From the Adriatic and the Balkan Mts., an elevated plateau extends across Asia to Pacific, bearing, upon its gigantic pedestal, the loftiest mountains of the globe. It includes the table-land of Persia — the desert of Gobi, etc. The latter has not been thoroughly explored. Its mean height is given at 4000 feet. (588.) Table - lands of Africa. — Southern Africa appears to rise to a considerable elevation, in successive terraces, from the coast to the interior, and even a considerable portion of the desert is an elevated table-land, bearing mountains estimated, by Dr. Barth, at from 3000 to 5000 feet high. (589.) Gulf Str cam. — traceable back eastward far as Pacific — proceeding from C. of Good Hope, N. W. across Atlantic, into Mexican Gulf, and, assisted by river - current of Mississippi, bursting out again between Florida and Cuba — near Azores, breaks into several branches, and spreads out thousands of square miles, covering colder waters of ocean and Bank of Newfoundland with fog. The warm air and vapor of tropical regions are thus borne to the continent of Europe, softening its climate, occasioning verdure of Gr. Britain and Ireland and perceptible even at Spitz¬ bergen; while the shores of western continent, in same latitudes as British Isles, are nearly uninhabitable on account of cold. Remark, however, climate of eastern continent is modified by another cause, namely, its greater extension east and mest; in consequence of which it remains longer under the sun, during the daily rotation, thus receiving and retaining more heat. One writer thinks the course of gulf stream influenced KEMARKS ON EARTH'S SURFACE. 263 by sub-marine coral-banks; another, that it has melted the European glaciers of the Ice-Period (but, in that case, what has melted those of N. America?). Herschel considers that its action has excavated Caribbean Sea and Gr. of Mexico; and that it will, sooner or later, cut through Isthmus of Darien. Should this be so, the climate of western Europe might become neárly as cold as Labrador and Hudson B. It is probable that the current receives its original impulse from the great antarctic drift-carrent, uniting with the equatorial current (caused by the earth's rotation); "and that its force is increased by the trade winds. {589. A.) Japán Current. — A similar current of N. Pacific wraps coasts of Jesso and Kurile Is. in fogs, like those of Newfoundland — mitigates the cold of Kamtchatka and Aleutian Is., to whose coasts it bears the remnants of ships Wrecked in tropics, and the costly woods of Sumatra and Java — in latitude of Japan it is deflected eastward back aCross Pacific, gathering, in its circuit, a 'sargasso sea, N. of Sand¬ wich Is. (PI. II), and bringiiig a milder and moistér atmosphere to western coast of N. America. (590.) Depth of tbe ocean. — Many attempts harve been made to measure the greatest depth of the •ocean (PI. IV). Such soundings are not always reliable, there being no certainty that the line sinks directly toward the bottom. It is supposed that the greatest depressions of land, beneath the ocean-level, about equal the greatest elevations of mountain-peaks above it. (591.) Primeval Forests. — The following rapid sketch of tropical nature is compressed from Humboldt, Daniel, v. Kloeden, etc. The term "primeval forest" is often used vaguely. It belongs particularly to the great Brazilian forest which is so impenetrable that it is scarcely possible, even with the axe, to clear a passage between the enormous tree- 264 REMARKS ON EARTH'S SURFACE. trunks, eight to twelve feet in dianaeter. This forest includes a large part of the interior of S. America. Its area, many times greater than that of Germany, exhibits a wonderful luxuriance, resulting from the combined inñuence of extreme moisture and high temperature. It is vain, says Humboldt, to ask, of what trees it consists, as a countless number of families are crowded together and new forms are always presented. (592.) Nature on Equator — a South Amer¬ ican River — Day. — D-aring the noontide hours, the mighty river rolls on, sparkling and flashing. Nature lies silent under the equatorial heat. Sun directly in the zenith. Not a breath. The naked rocks and bowlders* are covered with immense numbers of iguanas, lizards and spotted salamanders, which, motionless, with uplifted head and open mouth, delight to inhale the burning air. Serpents, whose colors eclipse the most brilliant flowers, come forth, from hollow tree-trunks, or hiding places in the ground, sun themselves on the rocks, or, winding up the trunks and branches of trees, watch for insects or birds. The crocodile lies in numbers on the shore, waiting for the capibara (ca-pib'a-ra), an animal between the hog and the rabbit, 3 or 4 feet long, vhich is devoured, in the forest, by the tiger, in the river, by the crocodile. Alligators swarm everywhere. Turtles and water-serpents glide through the waves. The bear, the black jag'-u-ar (american tiger — largest and most blood-thirsty variety), the panther, etc., come sometimes down to drink at the river-side, along paths which generations of beasts have worn through the impenetrable woods and which human feet (592 A.) * Bowlder: — a stone or rock, found on the sea shore, and in, or near rivers—worn smooth or rounded by the action of the water. Any rock apparently transported from a distant place by water, glaciers etc. Such masses, of enormous size, are sometimes found upon the highest mountains. REMARKS ON EARTH'S SURFACE. 265 have never trodden. The animals all fear, watch, hate and avoid each other. Most of the living creatures seek rest and shade. The larger beasts sleep or sculk in the black depths of the forest. Butterflies, of strangely gorgeous hues, flutter from flower to flower, or drink at the cool streamlet. The huge owl, sits motionless upon his shaded branch, impatient for the night. Myriads of chafers flash, like glittering jewels, through the air. Upon invisible wings, the humming bird hangs in the sunshine, clothed in the glory of the rainbow. Nature would lie as in the stillness of death, but for the fluttering and humming of millions of insects in the lower strata of the atmosphere, inter¬ rupted, occasionally, by the blowing of the freshwater dolphin, the distant scream of a monkey, or the deep tones of the toad and frog, blending with the monotonous chant of the cicada and locusts. At length the burning orb descends toward the west. The noonday heat begins to subside. The beast-world awakens and comes forth with extraordinary activity. Monkeys, by hundreds, issue from the forests, sporting, leaping, fighting, screaming. Birds of wonderful form and magnificent plumage, appear on all sides, now sweeping onward in solitary flight, now swarming in numbers along the odor-breathing shores. Flocks of flammingoes, and other water-birds, occasionally darken the air like a cloud. The whole parrot-tribe, conspicuous from their striking tints of deep blue, green or red, pierce the ear with discordant screeches. The toucan taps the tree-branch with his hollow bill and utters his plaintive cry for rain. (593.) Night. — The sun goes down. The countless creatures of the day seek rest. The night animals, among them the blood-thirsty vampire-bat, awake; the beasts of prey come forth, raging with hunger. Millions of flashing fire-flies illuminate the darkness. The wild nocturnal sounds render sleep impossible. Various utterances of the ape-tribe are 266 ADDENDA. heard; sometimes, soft, plaintive, almost flute-like; again, breaking into shrill, passionate discords. The black jaguar is the terror of the whole monkey-tribe. His screams often proceed from the high tree- branches, mingled with the sharp screeches and \ Wallings of the monkeys seeking to escape. The cougar adds his roar. Now, these noises are heard singly; now, they break forth spontaneously in one universal chorus, filling the vast forests with shrieks of rage, pain and despair. They appear to originate in some accidental combat. The jaguar, for instance, pursues the peccary (pec'ca-ry). The latter, flying in terror, breaks, with crashing noise, through the interwoven branches which impede his flight. The apes, on the tree-tops, terrified hy the sound, join their cries. This arouses the larger animals and alarms innumerable birds, till the whole solemn forest- world is thrown into disturbance. Such general commotions occur more frequently on stormy nights, amid violent torrents of rain, when flashes of lightning illuminate the scene, and peals of thunder enhance the tumult and disorder of the earth. ADDENDA TO PREVIOUS SECTIONS. (594.) Milky Way. Addition to section 11. — It has not always the same appearance. It becomes more visible, the higher it mounts into our heavens, and is seen to far greater advantage, at certain hours of the night and at particular epochs of the year. There are moments when its misty, irregular masses — .separated by black, empty spaces — projecting mysterious branches — breaking into billows of light — heavy clouds of world - dust — seem preternaturally near, and become a most impressive revelation of the Creator's power. "Is not God in the height of heaven? and behold the height of the stars, how high they are! .. . Praise ye the Lord from the heavens: praise him in the heights. Praise ye him, all his angels: praise ye him. ADDENDA. 267 all his hosts.... Praise him, ye heavens of heavens, and ye waters that be above the heavens." ^595.) Addition to 19 A. — On the other hand, the next nearest star which, because of its distance, man has not yet been able to measure, may be so remote that, even from Neptune — even from alpha Centauri — yes, even from Capella (PI. VIIl. C.) — it would still continue as immeasurable as from our earth. With regard to stars named in sec. 19, they are (except alpha Centauri) in our nori/iCTO - hemisphere sky; North Star, Capella, Vega, visible every clear evening — Arcturus and Sirius (latter very brillant), in winter and spring. Many stars, not above horizon in the evening of any particular season, become visible at a later hour of the night, by the rotation of the earth. (596.) Addition to 20. — On second reading, the pupil may pause, to examine chief stars in PI. I. A, which we have not yet named. The two at top of picture, nearly over the sun and earth, are Castor and Pollux, in constel¬ lation Gemini or Twins. The two, below the earth and sun, on the right, near Milky Way, are part of constellation Canis Minor (Lesser Dog)-, the largest, Procyon. Capella, although cut off from the picture by the upper edge, is visible every clear night at New York, to the N. W. of Castor and Pollux,, on the left (or east) of the Milky Way. In comparing this plate with the natural heavens, do not forget you are facing the south; your back is turned to North Star; east, therefore, is on your left hand, west on your right. Sirius is S. E. of Orion's belt; Aldebaran, N. W. (597.) Addition to 32. — You have only to grasp the idea of our globe, hanging upon nothing, (as in PI. I. B.), surrounded, on every side, by the infinite, starry heavens. As, wherever we are on the earth, we have a circular view (30 and 31), so, when we look away from the earth, we have also a circular view. Again, — when we stand upon our large, convex globe, we see only one half the hollow, celestial sphere (because the globe itself hides the other half from our view. But for the globe, we should see the whole of the concave, celestial sphere (30. 268 addenda. 32.) Now, if the earth were removed from beneath our feet, and we hung in our Light-car, in empty space, as an aeronaut* in his balloon, we should seem to be in the center of this stupendous, hollow sphere, which would completely encircle us — above —around — on every side— sparkling with stars and constellations,** far distant from our eye, and not sweeping over us as they usually seem to do, but quite immoveable. Now, picture to yourself our earth, hanging in the center of this hollow, celestial, unmoving sphere (PI. I. B.) The earth, with its pole always pointing to the N. Star, revolves, from W. to E., on its axis, once every day. It is plain that, as the earth thus revolves, from W. to E., the motionless heavenly sphere will seem to revolve, from E. to W. As the earth revolves, on its axis, with its îf. and S. poles at its extremities, so the heavenly sphere will seem to revolve, on its axis with its N. and S. poles at its extremities. And this axis of the heavenly sphere will be the same as that of our earth, except that it will correspond, in length, to the greater dimensions of the heavenly sphere. If the earth did not revolve, the heavens would not seem to revolve. If the earth were to stof revolving, the heavens would stop revolving. If the earth were suddenly to re¬ volve from E. to W., the sun, moon and stars would suddenly seem to turn backward and to revolve from W. to E. The only reason why there seems a N. pole of the heavens is, because the N. pole of the earth is directly under it. The S. pole of the heavens is, of course^ that point exactly opposite the S. pole of the earth, although it is not marked by any star as the N. pole of the heavens is and is not visible from our northern latitudes. A person (PI. I. B), standing on N. pole of the earth, would have the N. pole of the heavens over his head. He could see the heavens, on every side, as far down as the equator of the heavens — that is, just one half of it. A circle, supposed to be drawn around the heavens,' exactly equi¬ distant from the poles of the heavens we call the * aeronaut (a-e'-ro-naut) — one who floats through the air in a balloon. ** We must, however, suppose the light of the sun suspended: otherwise, in the above case, the stars would be invisible, as during our day. ADDENDA. 269 equator of the heavens. This, of course, exactly corresponds to the equator of the earth. A person, standing on the N. pole, could see no part of the heavens south of the equator of the heavens. Of course, he could not see the S. pole of the heavens. He never could get a view of that, till he traveled down as far as the equator of the earth. A person, at N. York, or any other place, in the same northern latitude, could not see the S. pole of the heavens, although he could see the N. pole of the heavens, i. e. the North Star. You understand now, why the S. pole of the heavens is as far below our southern horizon, as the N. pole is elevated above our northern horizon; and what the poet means, when he says: *^One pole rides high; one, plunged beneath the main. Seeks the deep night, and Pluto's dusky reign." (597 A.) Addition to 30 and 31. — A glance at PI. I. B will help you to understand the difference between the sensible horizon and the rational horizon. Suppose yourself standing at the point of the North pole —your sensible horizon would be that circle limiting the very small portion of the earth's surface within your view (too small to be represented in the picture even by the point of a pin). Your rational horizon would be the circle limiting your view of the heavens. Now, wherever you may be on the earth's surface, you can always see one half the heavens. At the North pole, you would see the heavens as far as that line called equator of the heavens, (in the picture it is a line; in the heavens, of course, it is a circle drawn around the heavens). If you stooil on the equator,, where the word west is written, you would see that half of the heavenly sphere intersected in the picture by the line called axis of the heavens. (598.) — Addition to 74. — In other words, spring and summer together, in our northern hemisphere, are 8 days longer than autumn and winter together. (599.) — Addition to 74. D. — The difference of distance between points B and E and points A and D cannot be very perceptible in a diagram. But it will become clear by a moment's reflection. The two extremities of an ellipse" form the two points at the greatest distance from each 270 ADDENDA. Other. These two points, being A and D, are not B and £. (600.) Âdditon to 74 G. — One reason why S. pole is colder than N. pole appears to be this: the southern hemisphere, in, consequence of the 7 or 8 days longer autumn and winter, and of the preponderance of ice— loses more heat, in a year, than the northern hemisphere does; and more than is compensated by the longer duration of the southern-hem. spring and summer. A further con¬ tinuation of this subject would lead us to the Great Year •— to the Ice Period — to the supposed gradual overflow, by the ocean, of the continents and islands of the N. and S. hemispheres, alternately, once about every 26,000 years— and to other points which, however deeply interesting, are beyond our present plan. (600 A.) Addition to 83. — "Between the tropics", says M'® Sommerville, "the rains follow the sun: when he is north of the equator, the rains prevail in the northern tropic; and when he is south of that line, in the southern. Hence one half of the year is extremely wet and the other half extremely dry; the change taking place near the equinoxes. Nevertheless, in countries situated between Sth and IQth parallels of latitude, north and south, there are two rainy seasons and two dry ; one occurs when the sun passes the zenith in his progress to the nearest tropic, and the other at his return; but, in the latter, the rains are less violent and of shorter duration. At sea, within the region of the trade winds, it seldota rains; but in the narrow zone between them, known as the variables, in both the great oceans, it rains almost continually, attended by violent thunder-storms". (601.) Addition to 93. — The space within the polar circles may be divided into six circular zones, in each of which, the difierence of the time of perpetual sunshine is one month. If we begin with arctic circle, the N. extremity of that zone, in our summer, has one month perpetual sunshine—the next nearer the pole, two months — and so On. The point, called the pole, six months. Of course, the same in antarctic circle. TRADE WINDS. 271 (602.) Addition to 138. — What can the following passages refer to if not to this Ice-Period? By the breath of God frost is given : and the breadth of the waters is straitened. (Job XXXVII. 10). Out of whose womb came the ice? and the hoary frost- of heaven, who hath gendered it? The waters are hid as with a stone, and the face of the deep is frozen. (Job XXXVUI. 29. 30.) He casteth forth his ice like morsels: who can stand before his cold?' He sendeth out his word, and melteth them: he causeth his wind to blow, and the waters flow. (Ps. CXLVII. 17. 18.) TRADE WINDS. (603.) In the earth's daily rotation (32), the atmosphere, which encompasses it on every side (a huge air-ocean) to the distance of 500 miles upward, is borne around with it. So stupendous a mass — so unfixed, un¬ solid, elastic, impressionable — cannot but be affected, by this motion, very differently from the rocks, plains and mountains. The latter objects are drawn around more rapidly. As our planet rotates from W. to E., it is thus always leaving its airy envelop a little behind it. The effect of this is exactly as if the air moved continually around the globe from E. to W. Thus the first tendency of the earth's rotation is to produce one broad, perpétuai east wind over its entire surface. There is such an air- current moving around the globe. It is called the trade wind. (608 A.) But the trade wind is not uniform. The atmosphere of our planet does not flow in one nnbroken movement from E. to W. There are contrary, and even conflicting winds. What are their causes? Here is one. The velocity of the earth's movement is very unequal at different points of its surface. At the equator, it is a thousand miles an hour — at the poles, nothing — at each intervening point or parallel, it is different. This very unequal movement of the earth's surface cannot but be transferred to the atmosphere and cannot but agitate it unequally as we advance from the equator to either pole. 272 TRADE WINDS. (bUoiJ.j The tendency to a universal east wind, a natural consequence of the earth's rotation, is most clearly visible in, and near tropical regions. The trade wind here blows with remarkable steadiness and constancy, over large areas of ocean and certain portions of continents and islands. Its northernmost limit, about 30° N. parallel —^ its southernmost limit (PI. IV.), 32® S. parallel. These limits, however, vary with the seasons, following the sun N. and S. The northern limit is sometimes 25° N. parallel (between parallels 25° and 32®, therefore, it is a periodical wind.) Instead, however, of blowing directly from E. to W., as it would do if resulting solely from the earth's daily rotation, the trade wind blows, in N. hem., from N. E.; in S. hem., from S. E. What is the cause? Let us suppose the earth did not rotate on its axis. The at¬ mospheric movement from E. to W. (with its various complications growing out of different rates of velocity (603 A.), in that case, would not exist. But the repose of the atmosphere would be disturbed by another very pow¬ erful agent — the sun's heat. We have seen (88 — 89) how the frigid zones are almost withdrawn from the sun's rays, never receiving them perpendicularly; and (90) how the sun perpetually pours perpendicular floods of light and heat upon the torrid zone. The sun is one million, four hundred and five thousand times larger than the earth. The air of the tropical regions is, of course, heated, by this mighty orb of fire, to a much higher degree than that of the frigid zones. It thus becomes rarified and lighter, and, rising to the upper regions, leaves a vacuum* which thé cold, denser air of the northern latitudes rushes down to fill. This generates a universal movement of the atmos¬ phere, from the poles toward the equator. Thus, if the earth's daily rotation on its axis were suspended, all that easterly wind, arising from the westerly rotation, would cease. There would then be no wind except that caused by the high temperature of the tropical regions. Every part of N. hem. would have a wind from the N.; while (603 C.) *) Vae'ii-um — an empty space ; a portion of space void of matter; a vacuity. A perfect vacuum, or space void of all matter, seems not to exist, upon the hypothesis of the luminiferous ether (32). ("IVorc. Diet.) TRADE WINDS. 273 «very part of S. hem. would have a wind from the S. The daily rotation and tropical heat, acting together, produce the present trade winds which, if not disturbed by still other causes, would blow, regularly and con¬ stantly, over a great portion of the globe's surface: in the N. hem., from north-east-, in the S. hem., from ■south-east. Supposing the earth a smooth, absolute sphere of ivory, like a billiard-ball — without oceans, valleys, forests, mountains, or other inequalities, either in configu¬ ration or material of the surface—then, at Boston, New York, San Francisco, London, Berne, Jerusalem, Petropaulovsk, ■Greenland, Nova Zembla, Behring Str. — that is, every where in N. hem., we should have a uniform, never ceasing, never changing north-east wind; and the traveller over the S. hem. would find a S. E. wind even at Wilkes Land, Kerguelen Land, Tristan da Cunha Is., Graham Land, New Zealand, etc. Remark, however, the wind would diminish in proportion to the distance from equator ; ■and various winds would result from the different rates of velocity (603 A). (603 D.) Why do these two winds not blow uniformly over the whole earth? Several causes; among them ■continents and mountain-ranges, which become more heated than the ocean (for instance, the desert region of Africa, the districts of Hindostán, Indo-China (S. of Himalaya), valleys of Orinoco, Amazon, etc.) and thus create new winds. (Yet the trade winds are very perceptible in low plains of Amazon and Orinoco and also in desert of Sahara itself.) ( 608 E.) Another cause, — changes of seasons, bringing sun's center, at one time, vertical over tropic of Cancer; at another, over tropic of Capricorn. Of course, as it is the sun's heat which causes the rarification of the air in tropical region, this periodical movement of the sun (nearly 50 degrees backward and forward, N. and S.) cannot but affect the winds. Add currents, which sweep around the globe, across different zones, causing new changes of temperature—add also presence or absence of vapor—direction and reflection of mountains—radiation of heat in the night. These influences disturb the regular 18 274 TRADE WINDS. course of the wind, particularly on continents, and evea on parts of the ocean, where winds are frequently variable and, sometimes, contrary to the general law. In Atlantic, between New York and Liverpool, the prevailing wind is, not from E. to W., nor from N. to S., but from W. to E. The same is observed in Atlantic from coast of Senegal and desert of Sahara; for nearly 100 m. out to sea the wind blows from the W.—also on W. coast of S. America (Chili and Peru). These exceptions are caused by proxim¬ ity of land. In that part of the ocean, between Str. of Gibraltar, Canary Is. and West Indies, the trade winds are much more perceptible. Perhaps the discovery o^ America would have been longer delayed, had not these favorable and tranquil winds wafted the frail bark of Columbus toward the island of St. Salvador. Perhaps it was this E. wind, so frequently alluded to in the Old Testament, which, thousands of years ago, first bore some wandering members of the human family from the old" to the new world. (603F.) On each side of equator is a belt, 6° broad, called "belt of calms", without trade wind; because, in that zone, instead of blowing directly from E. to W. (as- it ought to do from the rotation), thte heated and rarified air is continually rising and probably returning to polar regions by upper currents. The limits of this belt, also, like those of the regular trade winds, vary with the seasons, and from the same cause. (603 Gr.) The trade winds blow, with greatest strength and regularity, in S. hem. (PI. I. M) ; because that hemi¬ sphere oifers fewer interruptions. "It is by the facilities they thus afford to navigation", says Appleton's Am. Cycl., "that they have acquired name of trade winds. By taking advantage of them, vessels may run a regular cour.«e, often for weeks together, without shifting a sail, and all the time enjoying delightful weather, which everywhere prevails under the regular trades. This course may be before the winds, or obliquely across their line, in either direction. Where their regularity is disturbed by local causes, at certain seasons, as in the periodical changes of the monsoons, terrific storms are of frequent occurence. trade winds. 275 alternating with periods of calms and light variable breezes. At these times are experienced the most violent extremes of heat, rain and tornadoes, accompanied by waterspouts, the most vivid displays of lightning and awful bursts of thunder. The region about Madras, in India, is particularly exposed to the violence of these phenomena, which recur every 6 months. Vessels, at these periods, avoid the coasts; and so violent are the storms of wind, that even the fish from the sea are often found upon the tops of the houses, being blown off from the waves, or carried up by the waterspouts and then blown inland." The following extract from Dana's admirable two years before the mast illustrates some of our sections upon Astronomy as well as the Trade Winds. His ship has crossed the equator and is steering S. to double C. Horn. "This was glorious sailing. A steady breeze; the light trade-wind clouds over our heads; the incomparable temperature of the Pacific — neither hot nor cold; a clear sun every day, and clear moon and stars each night; new constellations rising in the south, and the familiar ones sinking in the north, as we went on our. course—stemming nightly toward the pole. Already we had sunk the North Star and the Great Bear in the northern horizon, and all hands looked out sharp to the southward for the Magellan Clouds, which each succeeding night we expected to make. 'The next time we see the North Star', said one, 'we shall be standing to the northward, the other side of the Horn'. This was true enough, and no doubt it would be a welcome sight; for sailors say that, in coming home from round Gape Horn, and the Gape of Good Hope, the North Star is the first land you make". ^603 Magellanic Clouds, or Cape Clouds — visible to naked eye in S. hem. (PI. I. B). The telescope resolves these wonderful objects, not into stars, but into other nebulae (19). They are crowded with immense stars. The larger cloud occupies an apparent space 12 times greater in diameter than our full moon. It surpasses in splendor the whitest world-dust clouds of our Milky Way. Berschel counted in it nearly 500 immense stars, about 300 nebulae, and 46 star-groups. The Arabs call it the "white ox". These two clouds of light revolve, at different distances, around the South Pole. Humboldt calls them 18* 276 OCEAN CURRENTS. ^objects unparalleled in the world of forms exhibited throughout the firmament; and by which the picturesque effect of the southern hemisphere is heightened. They rivet the attention of travellers by their individual isolation and the intensity of their light"'. Job (IX. 9) seems to allude to them: "which maketh Arcturus, Orion and Pleiades, and the chambers of the soutK\ OCEAN CURRENTS. (604.) Suppose the earth in following condition. 1. It does not advance on its annual journey. 2. It does not turn on its axis. 3. No continents, islands, etc.; an orb of water, surface covered with one unbroken ocean. 4. This universal ocean, of uniform depth. 5. Without difference of temperature (frigid and temperate ^ones warm as, tropics). 6. Without winds. 7. Gravitating power of sun and moon, suspended. 8. Moon's monthly revolution around earth also suspended. (604 A.) What would be the state of the ocean, with regard to tides and cúrrente, in 604? Rest—perfect rest. A steamship (if there were one) might circumnavi¬ gate this watery globe, in all directions—across poles — across the equator — and find it, every where, peaceful and motionless as a lake. Instead of this repose, our oceans are subject to enormous agitations. The globe's entire waters rise and fall, twice every day — many estuaries and rivers are visited by periodical inundations or bores. Beside this, immense masses of water,, hundreds of miles, thousands of miles long, make their way across the oceans with much greater velocity than the surrounding floods. At different points are found whirlpools, like the Maelstrom, Charybdis, etc. Whence come these violent movements? We will examine the causes, one by one, successively. (604B.) Make a single change in 604. Restore the annual movement of the earth around the sun. How would that effect the ocean? Probably not at all. Our planet. OCEAN CUKRENÏS. 277 advancing on its way around the sun, finds little — we may say, no interruption, opposition or friction, in space. The entire atmosphere, remember, advances with it, and both together, earth and atmosphere, move so softly through the rare, delicate ether (32. 603 C), that it is probable, if disquieted by no other agency, the ocean would continue to sleep in placid tranquillity, notwith¬ standing the velocity of 19 miles a second, or 68,000 miles an hour. We have no reason to believe that oceanic movements are produced by the annual revolution of the earth around the sun. (604 C.) Now make a second change in 604. Restore also the diurnal movement of the earth on its axis. Here we have a new motion, of another kind, which, as we have seen, is communicated to the atmosphere (603), and which cannot but disturb also the immense mass of denser water. This rotation, from W. to E., produces a movement of the globe's waters from E. to W. The solid globe moves somewhat faster than its ocean envelop, which is thus always left a little behind. This produces the same effect, as if the globe stood still and the ocean moved in a westerly direction. If the earth were a cylinder (442) rotating from E. to W., every point of its surface would go round with the same velocity and there would thus be one universal, uniform current, from E. to W. (604D.) The earth however is not a cylinder, but a globe and all the points of its surface, as we have seen (603 A), cannot move with equal velocity. Where is the velocity greatest? At the equator (23. 24. 32.) It there moves a thousand miles an hour. The velocity diminishes in proportion to the distance from the equator, N. and S., till, at the polar points, it ceases altogether. The ocean cannot but be affected by these various rates of velocity. (604E.) Now add a new agent to 604 — continents — gigantic dikes—built up, for thousands of miles, in front of the globe's broad current — almost at right angles with equator—marked by deep indentations, curved recesses and angular projections. Add again innumerable islands, grouped in close proximity, or stretching in chains. The 278 OCEAN CURRENTS. great body of water, with its tendency to advance around the globe from E. to W., is now opposed by these im¬ mense barriers. It rushes between the islands of Oceania, West Indies, etc., as between the abutments of a bridge. Its mass, compressed and thus augmented in volume and strength, strikes against continents, sweeps into, and then out of, gulfs, and by the worn coasts of peninsulas, capes and promontories — is broken into various currents, branch¬ ing now to the N., now to the S. — now deflected back again from one continent to another, in an easterly direction (Gulf stream, Japan current), that is from W. to E., and this deflected current, ' again breaking apart, and a portion flowing to the N. E., another to the S. E. Remark, there are prodigious, unexplored irregularities at the bottom of the sea—submarine continents, with mountain - ranges, valleys, coral rocks and forests, which impede or accelerate the advance, and augment the conflict of oceanic movements. (604F.) We now come to another agent, one of the most powerful and constant, namely, the heat of the sun. The tropical waters, like the air (603 B), are so much heated by his vertical rays that they become lighter and suffer a continual loss by evaporation. The tropical ocean is thus annually lowered many feet. This generates new and universal oceanic movements. Currents of cold, dense water rush, from the frigid zones, toward the equator, to displace the lighter, heated water, and to supply the waste of evaporation. If the earth were in the condition pictured 604, and this cause were added unthout the others; the result would be two currents (and only two), one from the N. Pole, the other from the S. Pole, each setting heavily toward the equator. But when, to the difference of temperature, are added the other causes, such as the earth's movement on its axis at such different rates of velocity on different parallels—continents—island- chains and groups—yet unknown, submarine irregularities— the result of all these combined causes, aided by others less general, is numerous currents sweeping across the ocean, in various unexpected and sometimes opposite directions; so that the original impetus derived from the rotation of the earth, although clearly discoverable, is very much modified. In some cases, a current on the surface moves in one direction, while a submarine current, beneath. OCEAN CURRENTS. 279 moves in another; or two currents, side by side, move in opposite directions. A glance at PI. I. L. and M. will show, why the general laws act, with more unbroken power, in the southern hem. than in the northern, being "there opposed by fewer interruptions. The tendency of the great mass of ocean water, even in closed seas, is to move onward in a certain direction, although the direction is not always what we should expect from the planetary rotation. ■(604 G.) Name chief causes of ocean-currents: 1. Rotation of the earth. 2. Unequal velocity of rotation, diminishing, from a thousand miles at equator, to nothing at poles. 3. Continents, islands, etc. 4. Inequalities at bottom of sea. 5. Rarification and evaporation of water in tropical regions by sun's heat. Among other, minor «auses are winds — unequal pressure of atmosphere — river-floods—changes of temperature—melting of iee, etc. The student is now prepared to inquire, under standingly, both of men and books, and to learn for himself, whatever he may desire, with regard to number, name and nature of ocean - currents. TIDES. (605.) The ocean presents three different kinds of movement: Currents; Tides, or the Tidal Wave; Wind-Waves. The first of these we have traced to their origin (604). Wind-Waves, explained hereafter (606). The Tidal Wave, we shall now examine. And first, remark, while studying the tides, separate the thought of ■currents altogether from your mind. Tides have an origin quite distinct from that of currents; although winds, tides aud currents unavoidably mix with, and modify each other. We now read section 604. (605 A.) Here, in 604, the ocean is motionless. No tides — no waves — no winds — no currents—no whirlpools. Now take PI. I. fig. E. Alter the circumstances of the earth, as described in 604, in one respect. Restore gravi- 280 TIDES. tating povier to the moon; that is, its power of attraction.*" What would take place? The attraction of the moon would pull the earth a little toward it. And the fluid ocean, being more susceptible, would, in a greater degree- than the rest of the earth, yield to its attracting power. The surface of the ocean would consequently be raised up a few feet on the meridian of the moon. 1/ the earth did not rotate on its axis; and if the moon did not move around the earth, as it does every month, this watery elevation would remain stationary. The ocean's surface would be a certain number of feet higher, on the side next the moon, than elsewhere. Remark, however, that the moon attracts most strongly the side of the earth nearest to it, and it attracts the center of the earth more strongly than the opposite side of the earth. The earth is thus a little drawn away from the waters on the opposite side, which causes these waters apparently to recede. Thus, on the meridian of the earth next the moon (or upper meridian), the waters are heaped up; and on the opposite side (or lower meridian), also, the waters are heaped up. Now these two elevations of the ocean are two tidal waveSy — in other words two high tides — (which we have not yet set in motion). Remark, while the waters, on the upper and lower meridians, are heaped up, the waters, situated half way between them (on the meridians 90® E. and 90® W.)—what would be the state of the ocean there? Its surface would necessarily be depressed. At each of those two points therefore (although without motion) we have a low tide. There would thus be, always, somewhere on our globe, at the same moment, two high tides simultane¬ ously, and two low tides simultaneously, at points removed 90® from each other — each high tide removed 180® from the other high tide: and each low tide 180® from the other low tide. Take PI. I. fig. E. Imagine yourself in a ship, in the Atlantic (where the word East is written), with the moon in our zenith. We should then have a high tidal wave. The other tidal wave would be on the opposite side of the globe (where the word West is written). Each tidal wave would, of course, have the breadth of * Of course the earth and moon attract each other mutually ; but the purpose of illustration is gained without going into that question (on this point see 605 D.) TIDES. 281 12,000 miles, that is half the globe's circumference. One of the low tides would be on the middle meridian (across which the word equator is written); the other low tide would be on the corre.sponding meridian on the opposite side of the globe's surface.* (605 B.) But, in nature, these tidal waves are not motionless. The surface of the water rises and falls twice every day all over the globe. Whence do our stationary tidal elevations receive this motion? Answer; from the rotation of the earth. As the earth rotates, from W. to E., once in 24 hours, the moon seems to revolve around it from E. to W., once in 24 hours; and as she revolves, she drags (by her power 'of attraction) this broad tidal wave after her. Here we have the first cause of tides. A great tidal wave would thus advance every day around the globe, immediately beneath the inoon, followed by another great tidal wave, on opposite side of globe, and, of course, at opposite hour of the day. Half way between these two tidal waves, two depressions of the ocean, that is two low tides, would follow each other, at their respective distances, and, of course, also at opposite hours of the day. (605 C.) The action of the moon is not powerful enough to raise much of a tidal wave in small seas and lakes, except where their po.sition particularly exposes them to the inundations of the great tidal wave of the ocean, or where the formation of the coast is such as to compress the broad, advancing wave within a too narrow channel, by which its height and strength are increased in .proportion to its narrowness. Thus- the Baltic and Mediterranean, being turned toward the West, without any such peculiar coast formation, are feebly affected. But the Yang-tse-kiang R. (289 B), the Hoogly (branch of the Ganges — 290), the Amazon R., Bay of Fundy, etc., from their geographical positions, are more directly exposed; and the height and fullness of the wave are augmented by the converging lines of their coasts and, perhaps, other (605D.) * The teacher will prevent the class from going into various irrelevant questions which might be disputatiously raised against all illustrations. 282 TIDES. local causes. Thus, as the advancing wave enters difierent •estuaries and river-mouths, it greatly varies in height. At New York, 6 to 8 feet; St. Francisco, 7; Amazon, 15 or 20. At B. of Fundy, it rushes up from the sea with such rapidity as sometimes to overtake swine feeding on the shores, rising to the height of 60 feet (Am. Cycl.). At the Hoogly, 10 feet; Bristol Channel, 40; at french port, St. Malo (British Channel), 60; at Yang-tse-kiang, •sometimes 100 feet. The tidal wave enters with dangerously augmented height and strength into many estuaries and river-mouths beside those we have mentioned (for instance sec. 567.) It might be asked, why is the wave so immense at places like Bristol, St. Malo, G. of California, etc., apparently sheltered as much as the Baltic and Mediterranean. Remark, however (605 G), the wave-tide rolls up the Atlantic from the south (i. e. from south-east) flowing westward and then eastward. The Mediterranean is protected by the colossal peninsula of western Africa which extends before it like a mole; the Baltic has the additional protection of the British Isles. The tidal wave is said to flow up the Niger 120 miles from the sea. ^605 E.) We have now accounted for the two chief phenomena; 1. two high tides every day. 2. two low tides every day. Let us again read 604. Bear in mind, we are speaking here, not of currents, but only of tides. What change did we first make in the condition of the earth as supposed in 604? We first restored to the moon its gravitating power (605 A.) What effect has that on the ocean? It attracts the waters, on the side of the globe next the moon, a few feet away from the earth; and it attracts the earth a few feet away from the waters on the opposite side of the globe. This would produce (supposing the earth stationary as in 604) a stationary elevation of the waters on the two sides of the globe thus affected. What was the second change we supposed in 604? We restored the diurnal revolution of the earth on its axis. What effect had this on the stationary elevation of the waters before mentioned? The same as if the moon really revolved around the earth, by her power of attrac¬ tion, dragging the broad tidal wave around the globe TIDES. 283 after her. Thus if the earth were in the condition of 604, and we were to make the two chancees above named, 1. the attracting power of the moon, 2. the daily rotation of the earth — then a great tidal wave would advance around the globe — followed by another great tidal wave on the opposite side — each of these followed at 90» distance — by corresponding depressions of the ocean — called low tides. I am now about to ask a question which requires »your utmost attention. Fir.st hear what is said, in sec. 24, of the rotation of the earth. (The teacher will please read this section). Now if the earth rotate with such punctu¬ ality, what effect would this have upon the tidal waves and depressions thus advancing around the globe under the moon ? Ought they not to arrive at any given point with absolute punctuality? Ought it not to he high tide, or low tide, at New York, or at any other given point, every day at the same second as the day before—indeed at the same one-hvndredth of a second^ Yet remark how the facts of nature sometimes contradict our theories. Instead of this punctuality, the attentive observer will find that the tides of each day arrive, not only 50 minutes late, but, every day 50 minutes later than on the preceding day. Suppose the high tidal wave arrive at N. York to day at noon-, to morrow, it will arrive about one-, the next day, about two-, 12 or 14 days afterward, ahovA midnight-, in about 28 days, N. York will have the same high tide at noon again (thus going around, as it were, in a drelef* What can be the cause? Let me read 604 again, and see if it contain any hint as to the origin of this irregularity; which, however, remark, although it may be called an irregularity, in one sense, has in it a perfect periodicity resembling that of the earth's rotation, except that it completes itself in a month instead of completing itself in a day. Can it arise from the earth's annual movement around the sun? No. From the daily rotation? No. From the presence of continents? No. From the difference of temperature? No. From winds? No. From the gravitating power of the sun and moon? No. From the moon's monthly revolution around the earth? Yes, that must be the cause of the daily retardation. If the moon did not * Do not forget, however, there are two high tides every day. 284 TIDES. revolve around the earth once in every 28 days, then the tides would move with the same wonderful punctuality as that which marks the earth's diurnal rotation (that is in in the condition supposed by sec. 604). But the moon is not immoveable. While the earth is revolving from W. to E., thus causing the moon to drag the tidal wave after her, in her apparent journey from E. to W., the moon is, in reality, moving backward all the time (her monthly rotation around the earth) from W. to E.; thus retarding, by her real motion, the tidal movement which advancing by her apparent motion. Remark, we more readily believe that this retardation is caused by the moon's monthly revolution, from the fact that the two periods exactly coincide—that is, the interval between two noon high tides at New York exactly coincides with the period of the moon's monthly revolution.* Or let us explain it another way. If the moon's monthly rotation around the earth were suspended, the earth's own revolution, on its axis, would bring her across our meridian at the same second every day. But, as she moves backward, so to speak, i. e. from W. to E. on her monthly rotation, she reaches our meridian 50 minutes later every day; and that corresponds exactly with the 50 minutes retardation of the tide. Thus the tides beautifully reflect the separate movements of the earth and moon. (^bUÔJb.; We have now accounted for the following phenomena: 1. The daily simultaneous elevation of the ocean water on two sides of the globe. 2. Simultaneous depres¬ sions, at the same moment, on two other sides of the globe, caused by the attraction of the moon. 3. The advance of these watery elevations and depressions every day around the globe, caused by the daily rotation of the earth. 4. The reason why (instead of advancing with absolute punctuality, as would be the case, if the movement derived from the rotation of the earth were not disturbed by any other cause) the tidal wave arrives, every day, 50 minutes later than on the preceding day. * In other words, the tide-wave arrives 50 minutes later every day, because'the moon arrives 50 minutes later on our meridian every day. TIDES. 285 (^bUoVr.J Now mark aoother tidal plienomenon. Have we always high tide, at any point of the coast, exactly when the moon crosses our meridian? By no means. The high tide comes a certain time after the moon has passed our meridian. This time is different in different places. Take PI. VI. B. At Cadiz, we have not high tide when the moon is on our meridian, but 1 hour 15 minutes afterward; at Lisbon, 4 h.; at Bayonne, 3 h. 30 m.; at Brest, 3 h. 45 m.; at Plymouth, 6 h. 5 m.; at Cherbourg, 7. h. 45 m.; at Calais, 11 h. 45 m., etc. If the earth were a perfect sphere, of equal temperature, wholly without continents and islands, encircled by an ocean of uniform depth, this would not be so. The tidal wave would be regular and punctual*. But the wave of tide, like the ocean currents, is held back by continents and islands — by the impediments at the bottom of the ocean ^—by the motions of earth and moon in their orbits — by the inertia and friction of the water — by opposing winds and currents — by the submarine sloping terraces which sometimes resist its advance near the shore. This delay, which is called the retard or age of the tide, is, at New York, sometimes, 24 hours; at Boston, 36 h.; even at C. of Good Hope, 14 h. The causes are not yet fully understood. Remark the tide wave consists of a movement of the ocean to its lowest depth. From the position and extent of the continents, it is not possible for it to continue its uninterrupted and punctual flow around the globe, from E. to W. "The great reservoir of \vater in which regular tidal action occurs, is not only in the southern hemisphere, but nearer the antarctic circle than the equator (PK 1. K). The source of the tides is therefore to be sought in the expanse of sea occurring within the soutJi temperate zone., where the great central agitation seems to commence, and whence on all sides it appears to flow northwards. The Atlantic (PI. IV) thus receives, from the souths its great wave of tide, which gradually becomes a curve, whose convexity is more and more northwards, until after passing the tropic of Cancer, the advance of the wave is so greatly retarded on the coast by the narrowness of the channel, that a portion of it has reaohed the latitude of the southern extremity of Greenland by the time that another portion has scarcely passed Cape Blanco on the African coast, and Cuba in the West Indies. The great wave of tide passing northwards, in this narrow channel, thus forms an enormous stream tide on the shores of Britain and North America; but it has, by this time, become so complicated, that it is difficult to trace its relations with the moderate and regular.^ndulation produced originally by the attraction of the moon. So also in the Pacific, the tide is so checked by the sub-marine * In that case, without looking at the shore, we shonld always be able to say, we have now high tide, because the moon is in our zenith; or low tide, because she is in our horizon. 286 TIDES. irregularities of surface, that for a considerable part of that vast ocean, there is scarcely any wave of the kind exhibited. In the Indian Ocean, on the other hand, the tide wave, little interrupted by such causes, makes its way in an irregular curve to the shores of India, and there divided by the pyramidal form of the peninsula of Hindostán, one portion'proceeds up the Bay of Benga!. and the other toward the Persian Gulf; the former having no escape, and not dissipated by irregularities in the form of the land, gradually increases in height as the bay narrows, and finally reaches the mouth of the Ganges, where it expends its force on the shores in the form of the well known and terrific bore of the Hooghly. In point of fact, therefore, the tides, although formed entirely by the attraction of the sun and moon, by no means follow the apparent course of those bodies. After the wave has once entered the canal of the Atlantic, it moves continuously northwards, with very various velocity, but at first at the rate of nearly a thousand miles per hour. In the first twenty-four hours, it has brought high water to Cape Blanco on the west of Africa, and Newfoundland on the American continent. 'In the morning of the second day, this great wave having been driven eastward, reaches the western coast of Ireland and England. Passing round the northern Cape of Scotland, it reaches Aberdeen at noon, travelling in/precisely the opposite direction to that of its first progress, and also opposite that of the sun and moon. Still proceeding onward, at midnight of the second day, it reaches the mouth of the Thames, and on the morning of the third day brings the merchandise of the world to tlte port of Loudon. It thus takes more time to reach London from Aberdeen than to pass over an arc of 120®, (8000 miles,) between 60® south latitude and 60® north. The velocity of the progress of this wave is greatest where the water is deepest, and where the configuration of the shores ofifers the fewest obstacles." {Prof* Ansted), (605 H.) Two other phenomena remain to be accounted for. The causes thus far enumerated, namely the grav¬ itating power of the moon, the earth's daily rotation, the moon's monthly rotation, ought to act with uniform regularity. The tides ought to arrive, with the retardations, mentioned in 605 E; and in 605 G; but they ought to be always of the same height. How therefore .shall we account for the fact that, at two periods of every month, the tidal wave acquires extraordinary height and fullness; and at two other periods of every month, it suffers a diminution of height and fullness—that is, it is higher or lower than it ought to be, from any cause heretofore enumerated. Can these phenomena result from the annual or diurnal movement? No. From islands or continents, etc.? No. From inequalities of ocean bottom? No. From difference of temperatur¿? No. From winds? No. From gravitating power of moon? No. Her gravitating power, we have already seen, exerts a uniform influence. What then can be the cause? If we observe nature with proper attention, we shall discover that, at the two periods of the month when these two unusually high tides, called spring - tides, occur, the sun and the moon are 1. either in a line with the earth and on the same side of it (that is in conjunction)', 2. or in a line with the earth and exactly on opposite TIDES. 287 sides of it (that is in oppositiori). In both these cases there will be a high tide of peculiar fullness on the tw» sides of the globe in a line with the sun and moon whereas, when the sun and moon are placed dififerentlj with regard to the earth—i. e. at the time of the moon's quadrature, when the moon and earth are on one line,, and the sun and earth are on a line perpendicular to the moon's line; then, instead of pulling the same way and combining their power to produce a tide of unusual fullness, they at,tract in different directions-, and while the moon has a tendency to produce a high tide on her upper and lower meridian, the sun is exerting his feebler power to- produce a high tide in a different direction. The spring¬ tide, therefore (288 A.), ought to occur twice a month, near the times of the new and full moon; and the neap-tider (157) ought to occur twice a month, near the times of the quadrature of the moon. "Quadrature", says Berschel, "is the position of the moon at the two points of her orbit, equally distant from the conjunction and opposition". (605 K.) Remark. In this rapid sketch, as in others, we present only an outline. Of course, highly interesting details remain untouched. For instance, the moon (in that meandering line which she pursues around the advancing earth) is, at one time, more than 20,000 miles nearer us- than at another (thus not more remote than 10 times the circumference of the earth). Many a man has travelled a much greater distance. The tides are affected by these- circumstances (605 L). The moon's volume is about 6 million times less than that of the sun; and 54 times less than that of the earth — her circumference not so- great as the arctic circle; yet, being our nearest neighbour, she exercises a threefold greater power of attraction than the sun. The distance of the latter luminary explains why he does not produce any tide; although, from his stupendous dimensions, he effects the above mentioned modifications- of the lunar tides. (605 L.) A few separate facts, viewed together, may help the student to a clearer understanding. 1. Twice a day, at intervals of about 12 hours 25 minutes, all the ocean coasts and estuaries of the globe are visited by an inundation. This has no connection with ocean - currents. 288 TIDES. The latter are not periodical, 2. In 6 hoars, the flood reaches its maximum and immediately begins to retire again from the rocks and strands. In about 6 hours more there is an ebb-tide. 3. The tide rises in less time than it ebbs. 4. Of course (as the earth's daily rotation - time is always absolutely the same (24), the tide-wave ought to arrive every day at •precisely the same second. Its regular arrival is delayed by the fact that, in consequence of the . moon's real, backward movement, from W. to E., she crosses our meridian, every day, 50 minutes later. Hence the tide arrives, every day, 50 minutes later. 5. The tide-wave does not arrive at the moment—sometimes, not even on the day, when the moon crosses our meridian, because (like the currents 604 E), by the intervention of continents, etc., it is subject to various degrees of retardation (605 G). 6. The unusually high tides (spring-tides) which occur twice a month (288 A — 605 H) ought to occur exactly at the times of the new and full moon. And the unusually low tides (neap-tides) ought to occur exactly at the times of the quadrature. This is not the case. Those phenomena never take place on the days of th change of the moon; but many hours afterward, from the retarding causes already mentioned. 7, We have the greatest of all tides, sometimes, at the equinoxes; because the sun then crosses the equator (71. 73). When the moon is, at that time, near the same plane, their united power of attraction over the waters of the globe is the greatest. The weakest floods, consequently, occur at the solstitial points. 8. The sun and the moon arc sometimes nearer the earth than at other times (605 K—74 H—Pl. VIII. K). The nearer they both are, the higher is the flood-tide. The floods of the winter-solstice, therefore, are higher than those of the summer (but not higher than those of the equinoxes). 9. In the center of the ocean the tides are not high. 10. Bodies of water, like Caspian, Mediterranean and Black Seas, isolated (iz'-o-la-ted) from the ocean and connected only by a narrow passage, are but slightly affected by tides. A strong current toward the E. enters Mediterra¬ nean by Str. of Gibraltar (but does not come out of it again), owing to the fact that this sea does not receive water enough from rivers to compensate for the loss by evaporation. But the tide-wave is scarcely observable. Hudson Bay, in the direction of the tide-wave, has distinct WIND-WAVES. 289 tides. 11. As the air is only another kind of ocean, enveloping the earth, so it is influenced by the rotation, as we have seen in the trade winds. It is subject, also, to aerial or atmospheric tides, resembling ocean-tides, resulting from attraction of the sun and moon. (606.) Wind-Waves. — Every schoolboy knows what a wave is, on a river or lake; but he has not reflected what it becomes in the "great deep". In narrow seas or even on the ocean, when the wind blows off" the land, there is not room for the formation of those gigantic billows which the ship has sometimes to encounter. But when there is sufficient breadth of water, and the wind is "such as to permit a gradual accumulation of volume and force, we have those appalling surges which make C. of Good Hope and G. Horn the terror of mariners — the "Cape of storms" and the "abode of the tempest". The height of the waves there, in a heavy gale, is estimated at about 40 feet from the hollow of the trough (pron. troff). Two ships, side by side, would thus often lose sight of each other. Off Australia, the waves are some¬ times, 20 feet; in Mediterranean, 16 feet. Remark a difference between the tide-wave and the wind-wave. While the tide-wave consists of a movement of the whole ocean from its lowest depth, the wind-wave extends only a comparatively small distance below the surface. The force of waves breaking against exposed points of rocky shores, sunken reefs and headlands, is immense. Heavy cannon, long before sunk in the bottom of the sea, have been washed far up upon the shore. For instance, the Eddystone rocks (English Channel near Plymouth, PI. VI). They consist of several ridges about 700 f. in length, at high tide entirely covered. It required all the genius of a great engineer, at an immense expense, to erect a light¬ house strong and massive enough to confront the tremen¬ dous breakers which had already carried away a previous tower; and "which have been known", says Hörschel, "to dash up above its top, to 150 feet higher than the sea level, and descend like a cataract on its summit". "The violence of the swell at the light-house", says Am. Cycl., "renders communication with the shore extremely difficult, even in serene weather; the sea frequently rises above the light; the strong plate glass of the lantern having 19 290 ISOTHERMS. been more than once broken by the waves. Three light- keepers are employed and the house is always supplied with provisions for 3 months, and a stock of 500 gallons of oil". (607.) Isotherms or Isothermal lines (l-so-turms). — If our globe were a perfect sphere—of polished ivory—without oceans — winds—mountains—plateaux — terraces— or any inequalities of surface, climate would probably depend upon latitude. The tropics and the polar circles would mark gradations of temperature with as much precision as- they now do the different conditions of day and night. But, instead of being a polished sphere of one substance, the earth, (however nearly spherical, when its irregularities of outline are compared with its entire dimensions) presents a very unequal surface, compared with the height of a man; is composed of widely different materials and is subject to various influences; among which are the direction and height of mountain-ranges — the slope of the country leaning toward or away from the sun — exposure to polar winds — shelter from them by mountain-ranges—nature of the soil—degree of cultivation of country—drainage— forests — direction of prevalent winds—proximity of the ocean — large tracts of water — desert—character of ad¬ jacent ocean - currents—elevation above the sea-level, etc. Thus we find (PI. IV) England, Scotland, Ireland, N. Germany, Sweden, etc., enjoying a mild climate; while the opposite coast of British America (Labrador), about the same parallel, has a winter of eight months; the clocks stop from the cold; and the bedrooms of the Moravian missionaries, although provided with enormous stoves from Europe and immense iron balls, kept heated red-hot all night, have the inside walls caked with ice and the bed¬ clothes frozen. The western shores of the continents are warmer than the same parallel of the eastern shores; as for instance, London and Nicola,Jefsk or Petropaulovski. The mouth of the Thames lies nearly on the same parallel as the mouth of the Amoor. Again, some places near equator are colder than others at a far greater distance. Kerguelen Land (220 B), almost beyond the habitable regions of the globe, is little farther from equator than Str. of Dover, Brussels, Dresden, and the vine-clad banks of the Rhine. The parallel of Edinburgh, in whose mild climate snow POPULATION TABLE 291 seldom falls, is the same as that of C. Horn; while Hammerfest (350 A) is several degrees nearer the pole than Graham Land, Repulse Bay, and Wilkes Land. If within the antarctic, instead of arctic circle, it would be separated from human beings by coasts of eternal ice. Instead of being able, therefore, to mark the different climates by parallels of latitude, they must be marked by very irreg¬ ular lines, called Isotherms or Isothermal lines (from two greek words, signifying equal and heat). These are imaginary lines passing through points on the earth's surface which have the same mean annual temperature. POPULATION TABLE. (608.) It is not possible to say with certainty how many human beings are, at this time, living on the globe. All the usual estimates are conjectural and probably vary from the truth by many millions. The general impression is that the total number amounts to 1350 millions. The following table, prin¬ cipally on the authority of the "Geographisches Jahr¬ buch" of Justus Perthes, Gotha, 1866, is perhaps the latest and most reliable. AMERICA 74,500,000 EUROPE 285,000,000 ASIA 798,600,000 AFRICA (from 60 to 100 million negroes)*. . . 188,000,000 AUSTRALIA 1,116,970 OCEANIA (including Australia) 30,000,000 N. AMERICA. Danish America (total) 114,622 Greenland 9,404 Iceland 66,987 Danish West Indies (Santa Cruz) 22,862 * Africa. Population, extremely uncertain — latest explorers report interior far more densely peopled than has hitherto heen supposed — their estimates of 200 millions are considered too high. We have thought it safer to take Boehm's estimate of 188 millions. Some even consider 120 millions nearer the truth. — Oceania—estimates, here eijually unsafe, vary from 21 to 35 miUions. 19* 292 POPULATION TABLE. British America (total) 4,404,396 Possessions N. of United States (total) . . . 3,444,914 (besides 155,000 independent Indians.) ' Upper Canada 1,396,091 Lower Canada 1,111,566 New Brunswick 252,047 Nova Scotia (with Cape Breton) 332,264 Prince Edward 1 80,857 Newfoundland 122,638 British Columbia 50,000 Vancouver 1 23,000 Red River Settlement 65,000 British West Indies (total) 933,847 Bahama Is. (5,500 white) 35,287 Jamaica (13,800 white) 441,264 Virgin Is 6,051 Barbadoes (16,500 white) 152,727 Trinidad (5,340 white) 84,438 British Honduras or Balize 25,635 Bermuda (or Somers) Is 11,451 French America (total) 277,954 French Fishery Is. (St. Pierre, Miquelon) . 2,497 French West Indies 275,457 Guadeloupe 118,867 Martinique 136,956 United States of America (1860) including Alaska, 54,000 ; St. Thomas, 12,660; and St. Juan, 1,715. 31,994,969 Mexico 8,259,000 Republics of Central America (total) 2,650,471 Guatemala 1,180,000 San Salvador 600,000 Honduras 350,000 Nicaragua 400,000 Costa Rica 120,471 West Indies (total) 3,935,352 Spanish West Indies 1,982,817 Cuba (of whom 793,484 white) 1,396,530 Porto Rico (300,406 white) 583,308 Swedish West Indies (St. Bartholomew) . . 2,800 Dutch West Indies (Curaçoa, etc.) 31,931 I. of Hayti (total) 708,500 Rep. of Hayti 572,000 Rep. of San Domingo 136,500 S. AMERICA. Columbia (of whom 126,000 independent Indians) 2,900,000 Venezuela 2,200,000 POPULATION TABLE. 293 Guiana (total) 246,795 French (about '/is white) 27,137 Dutch (of whom 7500 maroons*) 57,632 British (143,538 negroes) 162,026 Brazil (1,715,000 slaves) 10,045,000 Paraguay 1,337,439 Uruguay 240,965 Argentine Confederation (besides 40,000 independent Indians) 1,377,000 Patagonia 30,000 Chili (independent Indians 10,000) 1,676,243 Bolivia (245,000 Indians) 1,987,352 Peru 2,500,000 Ecuador (200,000 Indians) 1,300,000 EUROPE. Great Britain and Ireland (total) 29,935,404 England and Wales 21,210,020 Scotland 3,153,413 Ireland 5,571,971 Possessions in Europe (Heligoland, Gibraltar, Malta) 165,317 Total population of entire British Empire . 174,156,673 Sweden and Norway (total) 5,560,108 Sweden 4,070,061 Norway 1,490,047 Russia in Europe (total) 67,619,425 Russia Proper 61,061,801 Poland 4,840,466 Finland 1,717,158 Total population of the Russian Empire . . 76,083,818 Germany 38,016,968 North German League (total) 29,220,922 Prussia Proper (with Lauenburg) before 1866 19,304,843 Added in 1866: Hanover 1,923,492 Hesse - Cassel 737,283 Nassau 466,014 Frankfort City (and territory) .... 89,837 Territory ceded by Bavaria 32,976 Territory ceded by Hesse-Darmstadt 75,102 Schleswig-Holstein 960,996 Total population of Prussia. . 2^,590,543 * Maroon — a name given to free blacks living on the mountains in the West Indies. 294 POPDLATION TABLE. Saxony 2,343,994 Mecklenburg-Schwerin 552,612 Mecklenburg-Strelitz 99,060 Oldenburg 301,812 Saxe-Weimar 280,201 Brunswick 292,708 Anhalt 193,046 Saxe Meiningen '..... 178,065 Saxe-Coburg-Gotha 164,527 Saxe-Altenburg 141,839 Lippe - Detmold 111,336 Waldeck 59,143 Schwarzburg-Rudolstadt 73,752 Schwarzburg-Sondershausen 66,189 Renss 130,396 Schanmhurg - Lippe 31,382 Hesse - Darmstadt, N. of R. Main .... 225,696 Hamburg 229,941 Lübeck 50,614 Bremen 104,066 Bavaria 4,774,464 Wurtemberg 1,748,328 Hesse - Darmstadt, S. of R. Main 816,902 Baden 1,433,551 Lichtenstein 7,994 Germanic Confederation before the war of 1866 . 46,057,916 Belgium 4,940,570 Holland (total) 3,735,682 Holland Proper 3,529,108 Luxemburg 206,574 Denmark 1,617,170 Portugal (total) " 4,351,509 Continent 3,987,861 Azores 251,884 Madeiras 111,764 Spain (total) 16,302,625 Continent 15,752,607 Balearic Isles 278,660 Canary Is 256,408 Spanish population of Tetuan (Morocco) . . 14,950 Rep. Andorra 12,000 France 37,472,732 Switzerland 2,510,494 Italy 24,263,320 Papal Territory 692,112 Monaco 1,887 Rep. San Marino 7,080 Austria 32,572,932 POPULATION TABLE. 295 Turkey in Europe 15,725,367 Turkey Proper 10,586,000 Roumania 3,864,848 Wallachia 2,400,921 Moldavia 1,463,927 Servia 1,078,281 Montenegro 196,238 Greece (with Ionian Is. 225,861) 1,329,236 ASIA. Turkey in Asia (Asia Minor, Armenia, Syria, and part of Arabia) 16,050,000 Arabia (without Turkish possessions) 4,000,000 (1,219,000 Wahabees, 76,500 Bedouins.) Persia 5,000,000 Beloochistan 2,000,000 Hindostán, or British India 135,694,323 French colonies in India (Pondicherry) 229,533 • Portuguese colonies in India (Goa) 527,067 Indo-Chinese States (total) 21,109,000 Birman Empire 4,000,000 Empire of Siam 5,000,000 Empire of Anam (Cochinchina) 11,000,000 French Cochinchina 900,000 Independent States of Malay Peninsula . . . 200,000 Wild wandering tribes of the Peninsula . . 9,000 Chinese Empire (total) 477,500,000 China Proper 450,000,000 Mongolia 3,000,000 Manchooria 3,000,000 Corea 9,000,000 Tibet 11,000,000 Japan 35,000,000 Russia in Asia (total) 9,327,966 Caucasus 5,057,028 Siberia 4,270,938 Afghan States with Herat 4,000,000 AFRICA. Morocco 2,750,000 Algeria 2,999,124 Tunis 600,000 Tripolis with Fezzan and Barca 750,000 Egyptian States 7,465,000 Egypt Proper 4,306,691 Nubia 1,000,000 Kordofan 400,000 296 POPULATION TABLE. Abyssinia 3,000,000 Galla Country, S. of Abyssinia to the equator . . 7,000,000 Somauli Peninsula 8,000,000 Portuguese Possessions on E. coast of Africa (Mozambique, Sofala etc.) 300,000 Cape Colony 267,096 British Kaffraria 81,353 Kaffraria (between British Eaffraria and Natal). . 100,000 Land of the Kafifres, N. of Natal and Transvaal Rep. 440,000 Orange River Rep 50,000 Transvaal Rep 120,000 Land of Bechuanas, N. of Transvaal Rep 300,000 Land of Damara and Namaqua 60,000 Portuguese Possessions on W. coast (Angola, Ren¬ gúela, etc 9,057,500 Empire of Moropue (Molua) 1,000,000 Empire of Cazembe 530,000 Dahomey 150,000 Ashantee with tributary provinces and Gold Coast 4,500,000 Liberia 250,000 French Senegambia (Senegal) 170,101 Portuguese Possessions in Senegambia ...... 1,095 Dutch colonies on Guinea Coast 120,000 Sierra Leone (English Possession) 41,806 Empire of the Fellata or Foolah Country 22,300,000 Sahara 4,000,000 Unexplored negro countries on both sides of equa¬ tor according to reports 42,000,000 OCEANIA. MALAYSIA Sumatra with south-western islands 2,600,000 Java 13,649,680 Borneo with the neighboring smaller islands 1,200,000 Celebes 473,040 Molucca or Spice Is 376,029 Philippines (with Sooloo Archipelago) . . . 6,000,000 AUSTRALAYSIA Australia 1,116,970 Tasmania 89,977 New Guinea 1,000,000 New Zealand 154,296 New Caledonia 26,680 POLYNESIA Ladrone or Marianne Is 5,610 Marshall Archipelago 10,460 Sandwich or Hawaian Is 69,800 POPULATION TABLE. 297 Feejee Is 200,OOU Friendly Is 25,000 Society Is 7,500 Tahiti 9,086 Marquesas 10,000 , ISLANDS IN INDIAN OCEAN Andaman Is 10,000 Nicobar Is 5,000 Ceylon • • • • 1,919,487 Maldive Is 150,000 Laccadive Is. 6,800 I. of Socotra 3,000 Mauritius (with Seychelles 7,486) 322,517 Rodriguez, Amirauté Is 1,569 Reunion 205,972 Comoro Is 49,000 Madagascar 3,000,000 Zanzibar 250,000 ISLANDS IN ATLANTIC OCEAN Tristan da Cunha 35 St. Helena 6,860 Fernando Po and Anhabon 5,590 St. Thomas 8,000 Cape Verde Is 89,310 Races of Men. — Rthuography—(from two greek words, signifying nation and to describe). Mankind is generally divided into 5 classes : 1. White, Caucasian, or Indo-European race (500 to 600 millions — Europe; S. W. Asia; N. Africa; America). 2. Mongolian — (yellow, 300 to 400 millions — N. E. and Central Asia; China, etc.; Hungary; W. Russia). 3. Negro or Ethiopian — (100 millions — Middle and S. Africa; some islands of Oceania; America). 4. American — (13 millions). 5. Malay — (20 millions — Oceania; Indian Ocean). The Papuans and Alfuras (i. e. negroes of New Holland, New Guinea, and other islands) are sometimes counted as a sixth race. 298 ETHNOGRAPHY. The so-called "races" are marked by striking differ¬ ences in size, color, hair, physiognomy, skull, etc., reasonably ascribable to the variety of circumstances in which human beings have been placed for so many thousand years. The theory that these races, not descended from two individuals, have separate origins, has many advocates. But it has never been, in any way, demonstrated; and is opposed by the most eminent authorities; among whom, Alex. V. Humboldt. It is not without striking arguments. But those, against it, are far more convincing; and it is un¬ justifiable by any evidence drawn from reason, nature or Revelation. No two men arc alike—not even persons of the same family. Innumerable causes — climate — nature —food— occupation — accidents—epidemic maladies—elec¬ tricity — magnetism, etc., introduce physical changes, .perpetuate and amplify them. The Arab is in harmony with his desert; the Esquimau has been dwarfed by the influences of his arctic zone; the Greek, developed into beauty by the balmy air of his azure sky. The Laplander iind Hungarian present vast difterences; yet their languages indicate a common origin. The attempts to establish a theory of separate races, have failed before the evidences of unity. The more science advances, the more we find nature simple, and acting on a plan. Tacitus classed the Germans as a distinct race. Cuvier divided mankind into three races; Prichard, into 7; Bory de St. Vincent, into 15; others, into 16; others, into 22. These contradictory conclusions, and the impossibility of distinguishing how many races there are, denote that the supposed boundary lines do not exist. Humboldt declares "the more we study races, languages, traditions and customs, the more we shall find one single organic type in the great family of the human race, modified by circumstances which science will, perhaps, never have the means of determining". Daniel, in his great work: "Handbuch der Geographie", 1868, says: "Careful anatomical and physiological* investigations have demonstrated that the physical differences, found in man, belong to one species; and that the so-called different * PHYSIOLOGICAL—PHYSIOLOGY (from two greek words, signifying nature and a discourse)—the science of nature, more generally restricted to the science of living bodies, or of natural organizations, animal or vegetable. ETHNOGUAPHY. 299 races do not originate from different stocks, but are mere varieties of one stock. Two circumstances, among others, indicate this unity. 1. The numerous degrees, transitions, or shades of color, and forms of skull, discovered by modern science, pass almost imperceptibly into each other. 2. In every race, are individuals bearing the type of one of the other races." "The christian" says Paul Janet, one of the most able of living french writers, "may well wonder at the incon¬ sistency of philosophers who reject Scripture, while receiv¬ ing systems equally incredible, and far less proved; who declare man, an accidental development of the beast; and Plato and Paul, descendants of a gorilla; yet who will not admit that an Ethiopian could proceed from a Caucasian, or an American Indian, from a Mongol."