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Cornell Hniversity Library
THE EVAN WILHELM EVANS
MATHEMATICAL SEMINARY LIBRARY
THE GIFT OF
LUCIEN AUGUSTUS WAIT
Maas MATHEMATECH og giay vo |
7348-1
wii
DYNAMICS.
Cambringe:
PRINTED BY C. J. CLAY, M.A. AND SON,
AT THE UNIVERSITY PRESS,
A TREATISE
ON
DYNAMICS.
BY
W. H. BESANT, D.Sc, F.RB.S.
LECTURER OF SsT JOHN’S COLLEGE, CAMBRIDGE.
LONDON:
GEORGE BELL AND SONS.
CAMBRIDGE: DEIGHTON, BELL AND CO,
1885
+r
PREFACE.
THE object of the present Treatise is to introduce the
mathematical student to some of the earlier and easier
branches of Kinematics and Kinetics.
In the chapter allotted to Kinematics, I have deduced the
expressions for velocities and accelerations, as far as possible,
from the definitions and axioms of the subject.
In the applications to Kinetics, or, in other words, in the
combination of these expressions with the Laws of Motion,
for the determination of the motion of a particle or of a
system, I have adopted the same plan of operations.
I have assumed, and made free use of, the methods of
Analysis, for the performance and simplification of the
requisite calculations.
The methods employed, and the order of thought which
is followed, are those which during my experience as a teacher
I have found to be most effective in the elucidation and
development of the ideas of Kinetics.
The majority of students do not easily or rapidly absorb
general ideas, and they are most effectively assisted by the
gradual development of a subject through simple cases, and
illustrative examples.
vi PREFACE.
With this view I have endeavoured to explain the
application of the Laws of Motion to the determination of
the motion of a particle and of systems of particles, com-
mencing with easy cases, and leading up to a few of the
interesting and important cases of the motion of a body in
space.
My especial object has been to illustrate the direct appli-
cation of the Laws of Motion, and thereby to produce a
treatise of an elementary character, but of Educational utility
to the student who is commencing the study of theoretical
Kinetics. .
Iam very much indebted to Professor W. H. H. Hudson, of
King’s College, London, for useful suggestions and criticisms,
and to Mr G. B. Mathews, Professor of Mathematics at the
North Wales University, and Mr J. Brill, B.A. of St John’s
College, Cambridge, for their kind assistance in the correction
of manuscripts and proof sheets.
I venture to hope that the explanations and illustrations
of the text, and the numerous examples appended to the
several chapters, will be of assistance to the student in
mastering the elementary ideas of the subject, and pave
the way for the consideration of the higher branches and
the more difficult problems of the great science of Dynamics.
W. H. BESANT.
September 16, 1884,
ARTICLES
1
3—30
31—53
54—74
75—89
CONTENTS.
CHAPTER I.
PAGE
Introductory . ‘ : i 7 ‘ ‘ 1,2
CHAPTER II.
Differential Equations ‘ : ‘ : j ; 3—5
CHAPTER III.
Kinematics. : q ‘ ; : . : . 6—31
Examples . ‘ s . 7 5 : ‘ ‘ 31—37
CHAPTER IV.
Laws of Motion . 2 4 . 3 ‘ ‘ 38—51
CHAPTER V.
Rectilinear Motion . Fi ‘ ‘ . 5 ‘ 52—68
Examples . 3 7 3 . S 5 ‘i ‘ 69—82
CHAPTER VI.
Accelerations Parallel to fixed Axes . ‘ “ « » 88—95
Examples , . , rr Sr ro
ail
Vili
ARTICLES
90—121
122—140
141—157
158—168
169—176
177—201
202—229
230—251
CONTENTS.
CHAPTER VII.
Radial and Transversal Accelerations
Examples
CHAPTER VIII.
Tangential and Normal Accelerations
Examples
CHAPTER IX.
Motion in Three Dimensions
Examples
CHAPTER X.
Hodograph and Brachistochrone
Examples * Z %
CHAPTER XI.
Two Particles acting on each other .
Examples
CHAPTER XII.
Energy and Momentum
Examples
CHAPTER XIII.
Equations of Motion .
Examples
CHAPTER XIV.
Motion of a system in Three Dimensions.
Examples
PAGE
104—181
131—144
145—165
165—180
181-196
197—204
205—215
215—219
220—225
226—228
229—248
248—257
258—286
286—298
299—324
325—334
DYNAMICS.
CHAPTER I.
1. THE problems usually discussed under this head are
those which relate to the geometrical connections between
given motions, or given kinds of motion, and those which
relate to the action of forces, and the motions and changes of
motion produced by forces.
The former belong to pure science, and deal with the
geometry of motion, a branch of mathematics to which the
name Kinematics was applied by Ampére.
Strictly speaking the word Dynamics includes Statics,
the discussion of the equilibrium or balancing of forces, and
Kinetics, the discussion of the effects of forces on the motion
of bodies. Mechanism belongs to Kinematics, including such
problems as result from considering trains of wheelwork or
any connected machinery.
To Kinetics belong the consideration of the forces setting
such machinery in motion, or keeping it in motion, the
problems of Physical Astronomy, and others of important
practical application.
We shall commence by a development of the formule of
Kinematics, and afterwards proceed to consider the applica-
tion of the formule, and of the Laws of Motion, or Laws of
Force, to the determination of the motion of a particle, and
of a system of particles, produced by the action of given
forces, or, conversely, of the forces required to produce given
motions. The idea of a particle, or of a material point,
capable of being set in motion, or of having its motion
B. D. 1
2 DYNAMICS.
affected, by the action of force, is a mathematical abstraction
leading to the simplest forms of Kinetics. The determina-
tion of the motions of the bodies constituting the Solar
System belongs to this class in virtue of the facts that the
Planetary Bodies are nearly spherical in form, and that their
dimensions are very small in comparison with their distances
from each other and from the Sun.
Moreover the mathematical idea of a solid body is that of
a system of particles, and the discussion of the motion of a
single particle therefore naturally precedes the discussion of
the motion of a body or system of particles.
It will be seen that Newton’s Laws of Motion connect the
action of a force ona particle with the accelerations produced,
and lead to the formation of differential equations, the
integrations of which give the solution of the problem of
determining the motion.
It will appear further that Newton’s Laws are sufficient
for the determination of the motion of a system of particles
or bodies, whether rigidly connected or not, and lead, in a
similar manner, to systems of differential equations containing,
in their solution, the motions of the body, or of the various
bodies of the system.
CHAPTER II.
DIFFERENTIAL EQUATIONS.
2. THERE are certain differential equations which occur
so frequently in the discussion of questions in Kinetics, that
we think it worth while, for convenience of reference, to give
a brief solution of them.
(1) The equation, a +yf' («) =F (a), is at once solved
by the integrating factor
F(z)
es
leading to ye f@ | F(a) oe” dat C.
For example, if ay +—_ =tan2, the factor is tan 5, and
> da ~ sin & 2? 2’
therefore
y tans = 2tan 5 — a +C.
(2) TY + nly =0.
Multiply by 2 dy and integrate, then
dx
ty) eee a x da _,1 1
(Z =n’ (ce —y") or dy *n Jeay
". y =ccos (nx+a),
or y =A cos na + B sin na.
4 DIFFERENTIAL EQUATIONS.
(3) TY _ hy =0,
As before,
(y= nv (y? +e jy Oak ;
dz dy ~mn [yt +
-, ne=log ——~7—,
from which we obtain
y= A e+ Be™.
The equation oy + n?y = aa +b is reduced to one of the
two preceding by assuming
wr 4(QYeq=Fq), let $=
dy _ dz 7@ = d.2
da? da “dy ?° dy’
and the equation becomes, putting v for 2’,
Ft 2S) e= Fy)
which is of the ag (1).
then
dy dy
(5) ne ae
The solution of this equation is effected by the calculus
of operations, leading to
e”™™ D -1
Utena +5(1+ 5045)
D representing the operation © , and the expression affecting
+ by =e" 4 a".
x” being expanded in ascending powers of D,
The complementary function Ae + Be** must be added,
a and @ being the roots of the equation.
m+am+b=0.
DIFFERENTIAL EQUATIONS. 5
If the roots of this equation are imaginary and of the form
a+B4/1, the complementary function takes the form
e*” (A cos Ba +B sin Bz).
“q2
(6) a — n'y = COs ra.
The calculus of operations, or the variation of parameters,
gives as the integral,
=— eat + Ae’ + Be.
(7) ae n'y = cos re.
The solution is
= == + A cos nx + B sin nz.
If n=r, then, writing the solution in the form
es a as vas +Acosnz+Bsin na,
n—r :
and finding the limiting value of the fraction when n=7,
we obtain
y=5-sinne +A cos nv + Bsin nex.
72,
(8) oY +a BY + by = cosa.
This leads to
_ D-aD+b = cos ra
I=(p by ae D cos ra = (D — aD +b) Gary aie
the complementary function of course being added ;
_._ (b=7") cos ra + ar sin rx
19 barca
a and @ being the roots of the equation,
2+ az+b=0.,
+ Ac + Bef,
CHAPTER III.
KINEMATICS,
3. Definition. The velocity of a moving point, when
uniform, is measured by the number of units of length passed
over in the unit of time.
If the velocity be not uniform, it is measured at any
instant by the space which would be passed over in the unit
of time if the velocity were to remain the same as it is at
that instant.
To express this idea mathematically, let s be the space,
that is, the number of units of length passed over by the
moving point in the time ¢, and s+ ds the space passed over
in the time t+ 8, so that 8s is the space passed over in the
time 6¢, and, if d¢ be so small that the velocity is not sensibly
changed in the time &t, the limiting value of the expression 7
that is é is the measure of the velocity.
Or we may argue as follows, If v be the velocity at
the time ¢ and v + év at the time ¢ + é¢, then 8s lies between
vot and (v + dv) dé, and therefore ultimately,
v= di .
4, Ifthe velocity of a moving point be variable, it is said
to have positive acceleration, if the velocity be increasing,
and negative acceleration, or retardation, if the velocity be
decreasing.
KINEMATICS. 7
Tf the rate of increase of the velocity be uniform the
acceleration is measured by the increase of the velocity in
the unit of time, and, if variable, it is measured at any
instant by what would be the increase of velocity in the
unit of time if the rate of increase were to remain what it is
at the instant in question.
Mathematically, if » be the velocity at the time ¢, and
v+6v at the time ¢+6¢, the measure of the acceleration,
: see oee «x» OY
in the direction of motion, is —.
dt
Or, if f be the acceleration at the time ¢, and f+ 6f at the
time ¢ + ét, dv lies between fot and (f+ 5/) 5, and therefore
ultimately,
dv
=e
5. The composition and decomposition of velocities and
accelerations.
Supposing a moving point to possess, or to have
impressed upon it, two velocities in different directions,
there arises the question ; what is the resulting motion ?
To solve this kinematical question, we must invent
machinery to represent coexistent velocities.
BF D
A E
Imagine then a point to move uniformly along a straight
line while the line is carried parallel to itself at a uniform
rate. The point will then have two coexistent velocities.
Let EF be the moving line, and, while the point moves
from £ to F, let the line move from AB to CD. Then PE
is to HA as the velocity of the point along the line is to the
velocity of the line, that is, as CD to AC;
8 KINEMATICS,
Therefore APD is a straight line, and the point P actually
moves from A to D.
AD therefore represents the resultant velocity in
magnitude and direction.
This proposition is called the Parallelogram of velocities.
In the same way, if a point have two coexistent accelera-
tions, taking AB and AC to represent the velocities added
per unit of time, or which would be added per unit of time,
due to the accelerations at the instant in question, it follows
that AD represents the resultant velocity superposed, or
which would be superposed, per unit of time.
This is the Parallelogram of accelerations.
Conversely, any velocity or acceleration, represented by a
line AD, can be decomposed into two velocities or accelera-
tions, AB, AC, in any assigned directions,
6. Change of wnits in the measures of velocities and
accelerations.
If v be the measure of a velocity, the meaning is that v
units of length are passed over in the unit of time.
If a feet and ¢ seconds be the units, and if v’ be the
measure of the same velocity when a’ feet and ¢’ seconds are
units, it follows that
av_av
or?
for each expression represents the velocity in feet per second.
If f be the measure of an acceleration when a feet and ¢
seconds are units, the meaning is that
the velocity per ¢ seconds added in ¢ seconds = fa in feet;
*. velocity per second added in ¢ seconds =~,
d
*. velocity per second added in one second 2 .
If f’ be the measure of the same acceleration when a@
feet and ¢’ seconds are units, it follows that Le is the measure
KINEMATICS, 9
of the same acceleration referred to a foot and a second, and
. fa _fe
ee Ee
= f°
7. Angular velocity and angular acceleration.
If a straight line turn round in a plane it is said to have
angular velocity, and if this angular velocity be variable it is
said to have angular acceleration.
If @ be the inclination, at the time #, of the moving line
to any fixed line in the plane, then, exactly as in Articles (8)
and (4) the angular velocity is de or 6, and the angular
a 2 os
acceleration is ay or 0.
It must be observed that this is quite independent of any
motion of translation which the line may have, and simply
measures the rate of turning round,
When we speak of the angular velocity of a point P,
moving in a plane, about a fixed point O in the plane, we
really mean the angular velocity of the straight line OP.
If the velocity and direction of motion of P be given, a
simple expression can be obtained for its angular velocity
about a fixed point 0.
_ For if OP=,, and if p be the perpendicular from O on
the direction of motion of the point, and v its velocity, the
angular velocity is equal to the resolved part of the velocity
perpendicular to OP divided by OP, and therefore
aye ap al?
r r
8. Expressions for accelerations.
If z, y, 2 be the co-ordinates of a point, referred to a
system of fixed axes at right angles to each other, x, y, and z
are the distances of the point from the planes of yz, 2a,
and xy,
10 KINEMATICS.
The velocity parallel to x is thg rate of increase of the
distance from the plane yz, and, as in Art. (3), is represented
by - or by 4, employing fluxional notation.
And, similarly 4% and =
parallel to y and z.
If u, v, w be these velocities, the accelerations parallel to
the axes are, by the same reasoning as in Art. (4), = i 7 , and
, or y and 4, are the velocities
: ay. and
dae dy az
dt’ dt
dt’?
- ,or w%, 0, and w; that is, are or &, i,
and 2.
We shall in all cases limit the use of the symbols 4, # to
the case in which the time is the independent variable.
9. It must be carefully observed that the velocity of
a point in any direction is the rate of change of the distance
in that direction, and is equal to the limit of the change of
distance divided by the change of time, when that change
is indefinitely small.
And similarly, the acceleration in any direction is the rate
of change of the velocity in that direction, and is equal to
the limit of the change of velocity divided by the change of
time, when that change is indefinitely small.
10. Radial and transversal velocities and accelerations.
KINEMATICS. 11
Let r, 6 be the polar co-ordinates of a moving point,
and u,v the radial and transversal velocities, that is, the
velocities in direction of OP and perpendicular to OP.
P being the position of the point at the time ¢, and P’ at
the time ¢+ d¢, and if OP’ =r + 6r,
OP'cos80— OP _dr_.
St =a
OP'sin 80 rd0 _ a
3% dE
If u+ du, v + 6v, be the velocities at P’ in direction of
and perpendicular to OP’, acceleration in direction OP
(u + Su) cos dO — (v + dv) sin dd —u
u=limit of
and v=limit of
= limit of SE
_d_ db
dt dt
2, .
=5a—0 (G) at o8
acceleration perpendicular to OP
= limit of 2 + 6v) cos dO + (w+ du) sin dé —v
~ «bt
dv dO dO, drdé
ata ae tae a
4, 9291 2 (.d0
=7 0+ 270 =" a" a
It should be noticed that, ifr =0, that is, if the moving
point is passing through the origin, these expressions are
¥ and 276.
11. The expressions for radial and transversal accelera-
tions may otherwise be obtained in the following manner.
The component accelerations parallel to w and y being #
and ¥,"
12 KINEMATICS.
the radial and transversal accelerations are respectively
& cos 6 + ¥ sin @, and ¥ cos 6 — #sin 0.
Putting r cos @ for 2, and rsin @ for y, these expressions
become i . .
r—ré*, and ré + 276.
12. Case of uniform motion in a circle.
If x and @ are both constant, and if @ = a, the transversal
acceleration vanishes, and the radial acceleration =—o’r;
that is, the resultant acceleration is directed to the centre
of the circle and is equal to the radius multiplied by the
square of the angular velocity.
13. Velocities and accelerations referred to two axes, at
right angles to each other, moving in a plane about the origin.
If Ox, Oy be the positions of the axes at the time ¢,
Oz’, Oy' at the time t+ dt, 2Oz' = 60, and uw, », velocities
parallel to x and y at the time ¢,
NL (a + da) cos80—(y+dy)sind0—a« dx dd
ae ag St ~ at 9 Gt’
oe + 8x) sin 86 + (y + 8y) cos 80— y _ =¥ do
8t ft” ag
KINEMATICS, 13
If u+6u, »+8v be the velocities of P’ parallel to 2’
and y/,
acceleration parallel to Ox
L (u + du) cos 86 — (v + Sv) sin 86 —u
= Lt di ,
ai ,d8_ ae, (d_ yO gd
“ab de ae * (ai ve ae dt’
and acceleration parallel to Oy
=r, et™ sin 86 + (v + dv) cos 86 —v
ot z
as dv do d’y dey? ao dx dé
= ae 9 () bea ee
In fluxional notation, the velocities are
&— 6, and y¥ +26;
and the accelerations are
u—v6 and 6 +u6,
or a — yO — 26 —2y6, and 7 + 26 — y@ + 2006.
14. Case of a point moving on the surface of a right
circular cone.
14 KINEMATICS,
PN being perpendicular to the axis, let OP=r, and the
angle between the moving plane VPO and a fixed plane
“AON =6, and let Q be the projection of P on a plane
through O perpendicular to the axis of the cone.
d’.ON d’r
Acceleration parallel to ON = Geo ype Oe (1),
acceleration in direction NP = that of @ in direction OQ,
d’. OQ dQ\*
=“ *—09 a) , by Art. (10)..eeseees (2),
dr. ; ;
= Gpsin a—rsina (J) ;
and perpendicular to the plane VPO
=, dt Of es | , a0
Sane (r sina) =—— a (« ay
Multiplying (1) by cos a, (2) by sin a, and adding, we find
that the acceleration in the direction OP
2 2
=r sinta (3) =f—rsin’ a6’.
Multiplying (1) by sina, (2) by cos a, and subtracting, the
acceleration in the direction of the normal PG to the surface
dé\? .
=rsinacosa () =frsin a cos a6”,
15. Case of a point moving on the surface of a sphere.
KINEMATICS. 15
OAC being a fixed plane, and OC a fixed radius, and PN
perpendicular to OC, take ¢ as the angle between the planes
OAC and OPC, and 6 as the angle COP.
The accelerations in the directions, ON, NP, and per-
pendicular to the plane OPC, are respectively
a a, . J dd\?
ap (4 08 8), yp (asin 8) — asin 0 (2) :
Tk Py ag Sl
and zane a (2 sin OF ‘
Multiplying the second of these by cos 0, and the first by
sin @, the difference of the products is the acceleration in
direction of the tangent at P to the meridian curve CP, and
is equal to e :
. af ~ a sin 6 cos 0. ¢’.
Similarly the acceleration in the direction PO
=a? + asin’. ¢’.
16. In the general case in which the position of a
moving point at any time is defined by the polar co-ordinates
r, 0, p, the accelerations of P in the directions perpendicular
16 KINEMATICS.
to Oz in the plane CPA, and perpendicular to that plane are
the same as the accelerations of Q, and are therefore
2 \ 2 :
= (r sin 0) —r sin 6 (2) and ao Gi sin? 0 a ‘
the former in the direction NP and the latter perpendicular
to the plane CPA.
Also the acceleration parallel to Oz
@.ON @
= = A cos 6).
If p, t, « be the component accelerations in the directions
OP, PT perpendicular to OP in the plane CPA, and
perpendicular.to that plane, it follows, by resolving’ the above
accelerations, that
p= — re? = r¢? sin? 0,
T=70 + 276 —rd* sin 0 cos 6,
o=rd¢ sin 6 + 27¢ sin 0 + 2rG6 cos 0.
_ 17. Tangential and normal accelerations of a point moving
in a plane curve.
E
KINEMATICS. 17
If v be the velocity at P of a point moving in a curve,
and if s be the arc OP of the curve measured from some
fixed point O,
y=
~ dt"
The tangential acceleration at P
= (v + dv) cos 86—v_dv_ d's
=n 8t ~ de at
and the normal acceleration :
= (v+6v)sindp¢ _wdd_vdd ds_v°
ae ae aE pe
if p be the radius of curvature'‘at P.
If the motion of the point be uniform motion in a circle,
v and p are constant, and, if w be the angular velocity, v= ap.
The tangential acceleration is then zero, and the normal
acceleration, measured inwards, is equal to op, as in
Art. (11).
18. Accelerations of a point moving in a tortuous curve
in directions of the tangent, the principal normal, and, the
binormal.
If x, y, 2 be the coordinates of the point referred to fixed
rectangular axes, we have,
dr _de ds
dt ds dt’
Vx dsd«, /ds\ dx
and therefore a See t (5) a
ay _ ds dy , (ie) ay
at dt? ds (a ds*’
de de de, (ib)
dé dé ds" \dt/ ds**
18 KINEMATICS.
Now oe ‘ ay fe are the direction-cosines of the tangent,
ds’ ds’ ds
and if p be the radius of absolute curvature,
da dy az
Pp ds’ » P ds? » p ds? >
are the direction-cosines of the principal normal.
The above equations therefore prove that the resultant
: a @
acceleration of the point is compounded of the acceleration on
2
in direction of the tangent and of the acceleration : (=) in
direction of the principal normal.
It follows at once that there is no acceleration in direction
of the binormal.
Or, the direction-cosines of the binormal being pro-
portional to
dy@z dz@y dzd«a dx’d@z dad’y dy d«
ds ds* ds ds*’ ds ds* ds ds*’ ds ds* ds ds*’
if we multiply the above equations by these three quantities
respectively, and add them together, the right-hand member
vanishes identically.
19. These results can also be obtained by the consider-
ations that the osculating plane is the plane containing two
consecutive tangents, and that the consecutive osculating
plane is obtained by an infinitesimal twist round the tangent.
The circles PA, PA’, in the accompanying figure, are
consecutive circles of curvature, the angle between their
planes, 67, being the angle of torsion, and the circles being,
in general, small circles on the sphere of curvature. The
circles may be in certain cases coincident, or either of them
may be a great circle.
If P' be a consecutive point on the circle PA’, de be the
angle of contingence, that is, the angle between the tangents
at Pand P’, v the velocity at P, and v + du at P’,
the changes of velocity in directions of the tangent PT,
the principal normal P#, and the binormal are
KINEMATICS, 19
(v + 8v) cos Se — v, (v + dv) sin Se cos dy,
and (uv + 8v) sin de. sin 87;
dividing by S¢, we obtain in the limit, the expressions
dv vw
= and —
at p
from the first two, and the ratio of the last expression to
o¢ vanishes in the limit.
The Principles of Relative velocities and Relative accelera~
trons.
20. If P be a moving point, A, B, C,...other moving
points and O a fixed point, the velocity.of P in any direction
is the sum of the velocities, in the same direction, of P
relative to A, of A relative to B, of B relative to C, and so
on, and of the last moving point relative to O.
For if u be the velocity of P in the direction considered,
U,) Uy)-..U, of the moving points in the same direction,
Us (U —U,) + (U, — Uy) Fereeee + (thy, — Up) + Uns
which establishes the statement.
The same principle is equally true of accelerations,
du_d d :
for Ti = age ~ tq aa Mt aise vy |
that is the acceleration of P is the sum of the relative
accelerations.
21. By aid of the foregoing principle, the expressions of
Art. (18) are at once obtained.
2—2
20 KINEMATICS,
For u=velocity of P relative to NV + velocity of NV
=—y¥6 + &,
and so v=y+20.
Again, the acceleration of N in the direction Oz
=#— 26",
and that of P relative to V in the same direction
=~ (y8 + 2y8);
therefore the acceleration of P in the direction Ox
= & —«f — 6 — 246;
and similarly the acceleration of P in the direction Oy
= ij — 6 + 26 + 200.
22, We can also obtain the expressions for the accelera-
tions in the following manner.
The velocities of a moving point P, at any time ¢,
parallel to two moving directions Ow, Oy can be represented
by u= ON, v= QN,
and the accelerations parallel to 2 and y will be the rates of
change of « and v in those directions and will therefore be
u%—v0, and 6+.
Observing that ; ;
u=a@—y6, andv=y+26,
we obtain the expressions given at the end of the last
article.
KINEMATICS. 21
23. Component velocities and component accelerations
of a@ moving point referred to two axes turning round the
origin nm any given manner.
Let 6 and ¢ be the inclinations, at any instant, of Ox and
Oy to some fixed line in the plane, and represent by w the
angle «Oy or ¢ — 0. :
The velocity of P relative to V is yp perpendicular to
PN, and this, by the triangle of velocities HPN, decomposes
into — yd cosec w, and yd cot a, ;
parallel to # and y. '
The velocity of V in direction Ox is #, and perpendicular
to Ox is «6.
The latter, by the triangle of velocities ONF, decomposes
into —26 cot a, and 26 cosec a,
parallel to # and y.
Hence, the velocity of P being compounded of its
velocity with regard to N, and of the velocity of NV, the
components parallel to # and y are respectively
& — «0 cot w — yd cosec a,
y + 26 cosec w + yd cot w.
Tn exactly the same manner the component accelerations
are at once seen to be
22 KINEMATICS.
a — 06" — (a6 + 2a) cot w — (yp + 29d) cosec w,
4 — yO + (wb + 246) cosec w + (yp + 2y¢h) cot
24. The foregoing expressions can be obtained in a
different manner.
Thus if u and v be the component velocities,
weos 0+ 000s = 5 (aw cos O-+y cos $),
usin d-+vsin = 4 (sin 8 + ysing),
and if f, f’ be the component accelerations,
foosd+f’cosp= 5 (a cos @ + y cos ®),
2
f sin @ +f’ sin = Llesin 6 +ysin 4).
The solution of these equations will give the expressions
for u,v, f and f’.
25. Particular illustrations of the use of the principle of
relative velocities and relative accelerations.
(1) A point P describes an equiangular spiral with
uniform angular velocity round O, and a point Q describes an
equal spiral with the same angular velocity round P; tt is
required to find the path of Q.
Since r = ae®ets, we have
$=seca.r=r6 cosec a,
so that, if ~OP be the velocity of P, in the direction PT,
pPQ is the velocity of Q relative to P in the direction QF,
the angles OPT, PQF being equal and constant.
Hence OQ is the actual velocity of Q.
Further if QE, QF represent the component velocities in
direction and magnitude, the resulting velocity of Q is
represented by QG@ the diagonal of the parallelogram, and the
angle OQG = PQG — PQO=PQOF+ FQG — EGQ= PQF;
hence it follows that the path of Q is an equal spiral.
23
KINEMATICS.
s
ane ona R
ty
a
oO
A circle rolis uniformly inside a circle of double its
(2)
radius; it is required to find the acceleration of any carried
pownt.
ed
r
If P be the carried point on the radius CB, and if OB
produced meet the circle in A, it follows, since the angle
QCB = 2 COB, that the arcs QA, QB are equal.
24 KINEMATICS,
Therefore A is a fixed point and B moves along the line
AOA’.
Since OC, CB make equal angles with OA it follows
. that the angular velocities of the lines OC, CP are equal.
Hence, if w be this angular velocity, the acceleration of C
is in the direction CO and =o’. CO, and the acceleration of
P relative to C is in the direction PC and = w*. PC;
therefore, by the triangle of accelerations, the resulting
acceleration of P is in the direction PO and = w’. PO.
(3) A circle rolls on a straight line ; it is required to find
the acceleration of the point of the circle in contact with the
line.
If 6 be the angle through which the circle has rolled
from any assigned position, and a the radius of the circle, a9
is the linear space traversed by the centre C and therefore a6
is the acceleration of the centre.
The accelerations of the point of contact P, relative to the
centre are a” in direction PC, and a parallel to the line and
in the direction opposite to that of the motion.
Compounding these with the acceleration of C, it results
that the acceleration of P is in direction PC and is equal to
a6’, or to aw’, if w be the angular velocity.
This result, may otherwise be obtained as follows:
Let # and y be the coordinates of the point initially in
contact ; then
2=a0—asin 6, and y=a—acos 0,
from which #=a0—a(cos0.6—sin@. @),
ij =a(sin 0.6 + cos 0. &),
and, putting @=0, #=0, and 7 = a6’,
we hence infer that if p be the radius of curvature, at the
point of contact, of any curve rolling on a straight line, the
acceleration of the point of the curve in contact with the line
is w’p in the direction perpendicular to the line.
KINEMATICS. 25
Or we can give a proof directly from the definition of
acceleration.
wy
77 a
_ Let the curve P@ roll on a straight line, the point P
rising from the point A.
When at A, P has no velocity, and when Q is the point,
of contact, and is therefore the instantaneous centre, the
velocity of P is w. PQ perpendicular to PQ.
Taking PQ as an infinitesimal arc, and £# as the centre of
curvature, the velocities of P parallel and perpendicular
to the line are w. PQsin oO and w. PQ cos 66, if PHQ = 80.
Hence if 5¢ be the time the accelerations are the limits of
wo PQ se and w PQ ay , and, as PQ = pd8, the first of
these ultimately vanishes, and the second = op.
(4) A circle of radius b rolls on a circle of radius a; tt
is required to determine the acceleration of the point of
contact.
Taking the are BP equal to the arc AP, and o as the
angular velocity,
a+b,
o=(¢+d)=——9,
26 KINEMATICS.
and the accelerations of P relative to C, in the direction PC
and perpendicular to it, are
bw’ and bo.
The accelerations of C, in the direction CO and perpen-
dicular to it, are
; (a +b) @ and (a+ d) 6,
2.2
or DB aa be
at+6
Compounding these with the relative accelerations of P,
it results that the acceleration of P is in the direction PC
and is equal to
ab ,
arb”
Replacing a and b by radii of curvature this expression
gives the acceleration of the point of contact of any curve
rolling on a fixed curve.
26. We have considered in Art. (7) the angular velocity
of a line moving in a plane; we shall now find it necessary to
consider the angular velocity of a rigid system of lines
and points in space.
KINEMATICS, 27
The angular velocity of a rigid system about an axis is
the rate of increase of the inclination of a plane fixed in the
system, passing through the axis, to a plane passing through
the axis, fixed in space.
Parallelogram of angular velocities.
Imagine that a rigid system has two coexistent angular
velocities , @ about two axes OA, OB. Construct a
P,
iN
O MI A.
parallelogram AOBC such that OA and OB are in the
ratio of the angular velocities, and take a quantity Q such
that
OA: OB: OC :: 0: 0': 0.
If P be any point in the plane AOB, the velocity of P,
due to the two angular velocities, is equal to
oPM+o'PN,
perpendicular to the plane.
Now, OACB being a parallelogram, we know that
PL.OC=PM.0A+PN. OB;
oe 0O.PL=a.PM +0’ PN,
and therefore the velocity of P=.PL, which is the
velocity due to an angular velocity about OC.
The line OC therefore represents the resultant angular
velocity.
28 KINEMATICS,
Hence it follows that angular velocities are subject to the
parallelogrammic law, and can be compounded and decom-
posed in the same way as linear velocities.
In other words, an angular velocity is a vector.
27. If a rigid system be in motion about a fixed point,
there is always one line in the system which has no motion
and about which the system is turning.
It is clear that the motion of the system is completely
determined by the motions of any two given lines OP, OQ of
the system. Now, at any instant, OP must be moving in
some plane and therefore must be turning round some
straight line in the plane through OP perpendicular to the
plane of motion of OP.
Similarly OQ must be turning round some line in the
plane through OQ perpendicular to the plane of motion
of O@.
If then OC be the line of intersection of the two planes
through OP and OQ, perpendicular respectively to their
planes of motion, the motion of the system is completely
represented by a state of rotation about OC.
Any state of motion of a rigid system about a fixed point
can therefore be represented by a single angular velocity, or
by three coexistent angular velocities about three lines
through the fixed point.
28. Velocities and accelerations of a point referred to
three moving axes at right angles to each other.
Let 6, 0, 6, represent, at any instant, the angular
velocities of the system of axes about the axes themselves, or
rather, about the lines fixed in space with which the axes
are, at the instant, coincident.
If u, v, w be the component velocities,
u=velocity of P relative to K+that of K relative to V
+ that of V relative to O
=a—y9, + 20,,
KINEMATICS. 29
and similarly
v=y—20,+20,,
w=s— 20,4 0,
xz
K; | PL
/O “TL xv
‘M
y
For the accelerations,
let OL=u, OM=», ON=w
represent the component velocities ;
then the accelerations parallel to the axes are, on this
scale, the velocities of P, and are therefore
u— v0, + w8,
19 — wi, + U8,
w—ud, + v0.
Or, the acceleration of P relative to WV, in the direction
Ox, being w#—v6,, and the acceleration of N in the same
direction being w@,, the acceleration of P parallel to Ow is
the sum of these two, and the accelerations parallel to Oy
and Oz are obtained in the same manner.
29. If the position of a moving point P be defined
by the length r of the tangent PQ to a given curve, and the
deflection ¢ of the tangent,
30 KINEMATICS,
the acceleration parallel to PQ relative to Q = #— r¢’,
and that of Q in the same direction = 5, if the are OQ =s,
.. acceleration of P in the direction QP=7—r¢? +8
Ce
and, similarly, acceleration perpendicular to PQ
=rgét+ anb+ oe
if p be the radius of curvature at Q.
30. A point moves on a given curve, while the curve
turns round a fixed point in its plane: it is required to
find expressions for the accelerations of the point.
KINEMATICS. 31
If OP=r, the accelerations of the point P of the curve
are wr and r@ in the direction PO and perpendicular to
PO.
If the moving point be passing over the point P its
accelerations are those of P compounded with its accele-
rations relative to P.
These relative accelerations are due to the angular
motion of PY and to the motion on the curve, and, in
the respective directions of the tangent PZ’ and the normal
at P, are, if s be the are AP measured from a given point A
of the curve,
3?
§ and 2os + p ,
in accordance with the observation of Art. (10).
It is an instructive exercise to obtain these expressions by
taking a consecutive position of the moving point on the
curve, when twisted through a small angle wdt, and actually
resolving its velocities, relative to P, in the directions PZ’
and perpendicular to it.
EXAMPLES.
1. A railway train is moving at the rate of 30 miles an
hour, when it is struck by a stone moving horizontally and at
right angles to the train with the velocity of 33 feet per
second. Find the magnitude and direction of the velocity
with which the stone appears to meet the train.
2. Assuming that the earth describes a circle uniformly
about the sun in a year, that the distance of their centres is
240 radii of the sun, and that the radius of the sun is 100
times that of the earth, find the measure of the velocity of the
vertex of the earth’s shadow, taking the sun’s radius as the
unit of length and a year as the unit of time.
32 EXAMPLES,
3. If one point move uniformly in a circle, and another
move with equal velocity in a tangent to the circle, what are
their relative paths ?
4. The radius of the earth being 4000 miles, the latitude,
r, of a place at which a train travelling westward at the rate
of 1 mile per minute is at rest in space is given by
cos A = 507
5. Acircle revolves with uniform velocity about its centre.
The centre moves with varying velocity along a straight line.
Find the velocity parallel to this line at any instant of a point
on the circumference, and deduce the acceleration of the centre
necessary for this point to be always moving at right angles to
the line.
6. A point moves in a curve in such a way that its direc-
tion of motion changes at a rate varying as the velocity directly
and the whole space described inversely. Prove that the cur-
vature varies inversely as the are.
7. A wheel revolves uniformly about its centre C, which
is fixed, and a particle A moves uniformly in a straight line
through the centre; describe the path of a point # in the
wheel relative to A, (1) when CA is in the plane of the wheel,
(2) when CA is perpendicular to that plane.
8. Ifthe resolved parts of the velocity of a moving par-
ticle perpendicular to its distances from two fixed points are
constant, and equal to one another, its velocity varies as the
square root of the product of its distances from these points.
9. Aparticle A moves ina straight line, a second particle
B always moves towards A and keeps at a constant distance
from it. Find the path of B, and shew that its velocity is a
mean proportional between the velocity of its projection on
the path of A and the velocity of A.
10. df a point be situated at the intersection of the per-
pendiculars, drawn from the angular points of a triangle to
the sides respectively opposite to them, and have three com-
EXAMPLES. 33
ponent velocities, represented, in magnitude and direction, by
its distances from the angular points of the triangle, prove
that its resultant velocity will tend to the centre of the circle
circumscribing the triangle, and will be represented by twice
the distance of the point from the centre.
11. The tangent at a point P of a parabola meets the
tangent at the vertex in Y and the axis in JT. If Y move
with uniform velocity, shew that 7’ moves with uniform ac-
celeration: if 7’ move with uniform velocity, the velocity of ¥
varies inversely as AY.
12. If the velocity of a point be resolved into any number
of components in a plane, its angular velocity about any fixed
point in the plane is the sum of the angular velocities due to
the several components.
13. A point moves in a plane curve and sounds as it
moves. At a fixed point 0 in the plane the whole sound
produced is heard simultaneously. Shew (i) that if the point
moves uniformly, the curve is an equiangular spiral—(ii) if
the velocity of the point vary inversely as the distance of C
from its line of motion, the curve is a reciprocal spiral.
14, A point moves in the are of a cycloid so that the
tangent turns uniformly; prove that the acceleration of the
point is constant.
15. If the axes Ow, Oy revolve with constant angular
velocity w, and the component velocities of the point (xy)
parallel to the axes are
; a—b 2p?
a+b oy, e+e wx,
prove that the point describes relatively to the axes an ellipse
in the periodic time
aw a+b
@° ab
Prove that the locus of the points about which the angular
velocity of a point moving in any manner is, at the same
instant, the same, is a circle,
RT 3
34 EXAMPLES.
16. If the acceleration of a falling body be the unit of
acceleration and a velocity of 60 miles an hour the unit of
velocity, find the units of length and time.
17. Ifthe angular velocity of a particle about a given
point in its plane of motion be constant, prove that the trans-
versal component of its acceleration is proportional to the
radial component of its velocity.
18. If the acceleration of a falling body be the unit of
acceleration, and if a velocity of a yard per minute be the
unit of velocity, find the units of space and time.
19. Ifa lamina move in its plane so that two fixed points
in it describe straight lines with accelerations f, /’, shew that
the acceleration of the centre of instantaneous rotation is
JP FP HF 05 0
sin 0
3
-@ being the angle between the lines.
20. A lamina moves in its own plane so that two points
fixed in the lamina describe straight lines with equal accelera-
tions; prove that the acceleration of the centre of instan-
taneous rotation is constant in direction.
21. A point P moves with uniform velocity in a circle;
@ is a point in the same radius at double the distance from
the centre, PR is a tangent at P equal to the are described
by P from the beginning of the motion; shew that the
acceleration of the point # is represented in magnitude and
direction by RQ.
22. In two different systems of units an acceleration is
represented by the same number, while the velocity is
represented by numbers in the ratio 1 : 3. Compare the
units of time and space.
23. If the time is a quadratic function of the space
described, prove that the tangential acceleration is propor-
tional to the cube of the velocity.
_EXAMPLES. 35
24. A point moves in an ellipse so that the velocity
varies as the square of the diameter parallel to the direction
of motion: prove that the resultant acceleration at any
instant will be in direction of the line joining the point with
the middle point of the perpendicular from the centre on the
tangent at the point.
25. A point moves in a plane in such a manner that
its tangential and normal accelerations are always equal, and
its velocity varies as ec, s being the length of the are
of the curve measured from a fixed point; find the path.
26. Ifacurve roll in contact with a straight line with
uniform velocity, shew that the acceleration of the point in
contact with the straight line varies inversely as p, but if
with uniform angular velocity directly as p; p being the
radius of curvature of the curve at the point in contact,
27. A curve rolls along a straight line, the point of
contact moving uniformly along the line. Shew that the
acceleration of the centre of curvature of the rolling curve at
2
the point of contact is proportional to Be in the curve at the
8
point.
28. If the motion be referred to two axes one of which
is fixed, and the other revolves about the origin in such
a way that the line joining the origin to the particle is
equally inclined at an angle $@ to the axes, shew that the
component acceleration parallel to the fixed axis (€) is
& — (26 + £0) cosec 0,
What is the other component ?
29. Ifthe radial and transversal accelerations of a particle
be each proportional to the velocity in the direction of the
other, the path of the particle is given by the equation of
the form
2) -2 ir 2 C
(8) Gleave anares
3—2
36 EXAMPLES,
30. If the perpendiculars from a point Pon axes Ox, Oy
of which Ox is fixed, and Oy revolves uniformly, are & 7
respectively, prove that the accelerations of P parallel to
the axes at the instant when they are perpendicular
are j—2Ew +7’, and £; the angular velocity of Oy
being o.
31. The centre C of an elliptic wire is moved with
uniform velocity along a fixed line CY in its own plane
whilst the wire is in contact at P with a fixed line PY
perpendicular to CY; shew that the acceleration perpen-
dicular to PY of the point of the curve in contact at
Po x’ yp’, where CY =p, and a, y are the co-ordinates
of P referred to the axes.
32. A point moves in a plane with an angular velocity
w, and the plane is turning round the radius vector with an
angular velocity w’; prove that the accelerations in the plane
are #— o'r, and ro + 2rw, and that the acceleration perpen-
dicular to the plane is raw’.
33. A point P moves on a straight line OP which is
made to describe uniformly a right circular cone about an
axis OA, while OA sweeps out uniformly a right circular
cylinder ; find an expression for the acceleration of the point
P in the direction OP. ;
34, A point P moves so that its velocity is compounded
of two constant velocities, one of which is in a fixed direction
and the other is perpendicular to the line joining P to a fixed
point. Find the orbit described by P.
35. A plane is moving about an axis perpendicular to it,
and a point is moving in a given curve traced on the plane;
in any position w is the angular velocity of the plane, v the
velocity of the particle relative to the plane, r its distance
from the axis, p the perpendicular on the tangent, s the arc
described along the plane, prove that the acceleration along
the tangent to the curve is
dv dw 2 ar
0 (Greg) oe a
EXAMPLES. 37
86. The velocity of a point moving in a plane is
the resultant of two velocities v and v along two radii
vectores 7 and r’ measured from two fixed points at a
distance a apart. Prove that the corresponding accelera-
tions are
du ve’ 2 2 2
dit apy + oF),
ba ate (r?—r? +0’).
and dé * Qrr®
37. 4)
al x ¢ COS 4, wa ‘
58 RECTILINEAR MOTION.
This shews that the particle descends through the space
2a <8, and then rises again to its initial position and
continues to oscillate, the time of a complete oscillation being
n/m,
The range of oscillation can be obtained at once by
the principle of energy, for the particle will fall until the
gain of potential energy developed by extension is equal to
the loss of potential energy due to the fall.
Now the potential energy of a stretched elastic string
=} (Tension) (Extension),
and therefore, if z be the total fall,
eee = 94 oe
$(a2)e mgz, or z 2a >
62. Fall of a heavy particle in a resisting medium
when the force of resistance 1s proportional to the velocity.
Measuring w downwards the equation of motion is
c= —ke,
which gives é+ ka = gt,
if the particle fall from rest,
and.’ : ae” = [gte™ dt, [Chap. 11.]
t kt
or L= ¢ - q + fe ee
taking «= 0, when ¢=0.
Hence & = - t er"
and, if ¢ increase indefinitely, ¢ = f ‘
This is called the terminal velocity.
63. Fall of a heavy particle in a medium, the resistance
of which varies as the square of the velocity.
RECTILINEAR MOTION. 59
Measuring x downwards the equation of motion is
dv _ ty OP aa
oe 0 ke? or + 2h = 29,
from which ve = . e+ 0, [Chap. 11]
and, choosing the origin so that v=0 when 2 = 0,
v= (l-e«™).
In this case the terminal velocity is a ‘.
Ms ice ang
dz gNe*—1’
“ OTs Py Sea 1,
from which we obtain,
kx = log (
Further,
ele =)
5 :
Or we may use the equation,
0 =9g- ke’,
which leads to
ie ; gvtt. = Net a
gg) Nw 41 Nae NER
and gives the same value of x as before.
64. Motion of a heavy particle projected vertically up-
wards in the same medium.
In this case, measuring # upwards,
dv
v——=—g—kv’.
dc
Integrating and taking w as the initial velocity,
g + ky? hens et
gtk
2
6U RECTILINEAR MOTION.
shewing that the ak rises to the height
ap loe (1 + ew a
g
Further il = o A ku’) * — 9g,
bo o
wodkg .t = sin
Ju 1+ — pe 14+—
which gives _
Zp k
a a/ a .usin (hg. t) + cos (J/kg)
Or, starting from the equation 9 =— g — kv’, we obtain
- Jgkt= tan*(v J = tan”? (u J)
and therefore
— sin™
w/t
on/s= tan./kg.t uk cos Jlig.t—s/g sin Jig.t. t.
Tt ua/* tan vig t ~ J/g cos Jkg- ttuJksin Jig.t”
giving the same value of « as before.
65. A particle moves from rest, in a medium the resistance
of which varies as the square of the velocity, under the action of
a force to a fimed point varying as the distance.
In this case
dv
= = ky’ — px,
and therefore _
ees oe = oe aie—a) ai (1 — ea), [Chap. 11]
observing that v= 0 when =a.
66. Motion of a piece of uniform chain in a straight line,
under the action of forces in that line.
Taking a fixed point O in the line, let x be the distance
from O of one end A of the chain and take r as the distance
from A of a point Pof the chain, —
RECTILINEAR MOTION, 61.
The motion of the element PQ (ér) depends upon the
tensions at P and Q and the acting force.
Oo A PQ B
If m be the mass of unit length, the mass of the element
is mér, and if mérX be the force acting upon it, the equation
of motion is
mor .@=8T' + mor. X,
taking 7 as the tension at P, and observing that the accele-
ration of every point of the string is the same as that of the
point A.
Integrating this equation over the length of the string we
shall obtain an equation for determining « in terms of the
time.
Suppose for instance that the force is repulsive and varies
as the distance from the point O, or that
A=p (a+r).
Integrating,
r
2
mrié= T+ mp (re + 5) + C,
and, observing that 7’'= 0, when r=0 and when r=a,
so a
cL=p (2 - 5) 5
the solution of which is the same as in previous cases,
Substituting for # we find that
T=impr (a—-71).
67. Direct impact of elastic balls on each other.
If two elastic balls impinge directly on each other, that is,
if the line joining their centres be the line of motion of each
ball, the effect of the impact is an immediate change in the
momentum of each ball.
But, since action and reaction are equal and opposite the
momentum added to one ball is equal to that which is lost
62 RECTILINEAR MOTION.
by the other so that the total momentum remains un-
changed.
This gives one equation of motion.
For another we appeal to experiment; and assume the ex-
perimental law that, if e be the coefficient of elasticity, the
relative velocity of the two balls after impact is reversed in
direction and is to the relative velocity before impact in the
ratio of e to unity.
Hence if. the ball m impinge with velocity u on the ball
m’ moving in the same direction with velocity w', and if
v and v’ be the velocities after impact, both measured in the
same direction as before, we have the equations,
mvt+ my = mu+m'w,
vw —v=e(u—v),
from which we obtain
(m+m’) v' = u(m+em) + wu (m' — em),
(m+) v = u(m— em’) +u' (m' + em’).
It is worth mentioning that, in all cases of the impact of
elastic bodies, energy is lost by impact; if the elasticity be
perfect, that is, if e = 1, no energy is lost.
If two elastic balls impinge obliquely on each other, all
that is necessary is to resolve the velocities parallel and
perpendicular to the line of centres; the motions perpendi-
cular to the line of centres are unchanged, and the preceding
equations determine the changes of motion along the line
of centres,
68. In the case of Art. (55), it is required to examine
the effect of suddenly attaching a weight, mass p, to any point
of the ascending string.
The mass », having no momentum before it is attached,
acquires momentum instantaneously, and if m be the
descending body its motion is suddenly checked, while the
portion of string between mw and m’ is slackened and m’ rises
freely.
RECTILINEAR MOTION, 63
_ Aft be the velocity with which the two are moving at the
instant before mw is attached, and uw’ immediately afterwards,
(m + p) u’ = mu,
since the momentum in the direction of motion is unchanged.
The impulsive tension @ of the string is given by the
equations
m (u'—u)=~ Q, pu'= Q,
the effect of the impulse on each body being change of
momentum.
Subsequently, if ¢ be the time which elapses before the
lower string becomes tightened,
m — pb
t—ho? =wt+4——" gt’;
Bm tg = ait h ae}
this determines ¢, and therefore determines the velocities of
m’ and of « and m at that time.
A jerk then takes place, and the momentum of the
system in direction of motion remaining unchanged the new
velocity is at. once determined and the subsequent accele-
ration is
m-h—m
m+p+m I
69. A straight piece of uniform chain lying on a smooth
horizontal table recewes at one end a given impulse in direction
of its length ; it is required to determine the motion and the
umpulsive tension at any point.
B p 2172
Let m be the mass of the chain, and a its length; then if
v be the velocity produced by the impulse,
Q=m,
and, if 7’ be the impulsive tension at a point P,
eae
a
for the mass of BP is set in motion by the impulse 7.
64 RECTILINEAR MOTION.
70. A heavy uniform chain is suspended by one end above
a horizontal table, its lower end being just above the table; of
it be allowed to fall, it is required to find the pressure on the
table.
We have seen that force is measured by the rate of pro-
duction, or destruction, of momentum.
As the chain falls, the table receives an infinite number
of infinitely small impulses, and the result is that a finite
varying pressure is produced, which, added to the weight of the
portion coiled up at the instant considered, gives the pressure
on the table at that instant.
When a length z has been coiled up, the velocity is J 29a,
and therefore the portion coiled up in a small time 6¢ is
5¢ /2gx, and the momentum of this portion, which is de-
stroyed in the time 6¢,
MEM Nigam uy
M being the mass of the chain and a its length.
Hence momentum is being destroyed at the rate of 2Mg -
per unit of time; and therefore, adding the weight of the coil,
the pressure on the table is three times the weight of the coil.
71. One end, B, of a heavy uniform chain hangs over a
small pulley A, and the other 1s coiled up on a table at C; of
B preponderate it 1s required to determine the motion and the
tension at C.
It is easily seen in this case that all internal tensions
neutralise each other, and that the momentum of the system
in the direction of motion is due to the external forces acting
on the system in that direction, that is to gravity, and the
reaction of the table.
This reaction is equal to the weight of the coil on the
table, and the resulting force in direction of the motion is the
difference of the weights of the two straight portions of
chain.
oO
RECTILINEAR MOTION, 6
If AC=a, and AB=za, and if v be the velocity, the
momentum = 4 (w+a)v, w being the mass of an unit of
length ; therefore
d
5 (eta) 1} =9 (ea),
or, since dao dy P= (
i den tare v=g(x—a),
the integral of this equation is
3
(a + a)? t= 29 (Gata) + C,
the constant being determined by initial conditions.
If for instance # = a, initially, that is, if # be just greater
than a, C= ga’,
(w+ aot = 2 (@— a) (e+ 20).
Also, (the tension at C) x t= momentum generated in the
time é¢ by the action of the tension
= (uvdt) v;
therefore tension = pv,
Or, we might have arranged the process thus :
calling the tension 7,
di
p(e+a) 05" = pg (w—a)—T
is the equation of motion of the portion of chain CAB,
and, as above, 7'= pv’.
\
72. A spherical raindrop, as tt falls, receives continually
by precipitation of vapour, an accession of mass proportional
to ws surface; neglecting the resistance of the air, it is re-
quired to determine its motion.
If a be the initial radius, and e the thickness of the shell
deposited in the unit of time, the radius (r) at the time ¢
=at+e.
B. D. 5
66 RECTILINEAR MOTION,
Hence the momentum at the time ¢
= mp (a+ et)? 2,
and © (4mp ar ell 0) =9.4mpate ,
dv 3ev
and therefore i + a 9:
am pee
and = ate asa:
This article and the two preceding were published in 1873,
in a paper in the Mathematical Journal for that year.
73. Fall of snow down a sloping roof.
Imagine the snow to be just supported by friction or
adhesion, and that a very slight downward impulse is given
to the top line of the snow just below the ridge of the roof.
In that case the snow will slide down from the top and
gradually set the whole in motion.
Take 6 as the breadth in motion, and mas the mass of
unit area ;
then, neglecting the friction on the mass in motion which
is practically very slight, the equation of motion is
. (mbxé) = mbag sin a,
or xt + a = gx sina,
which gives &* = 2 gxsina,
and shews that the acceleration is one-third of that of a mass
sliding freely.
74. The equilibrium and motion of a heavy ball, supported
by a vertical jet of sand.
We shall consider the case of a cylindrical homogeneous
jet, supporting the ball symmetrically, and assume that the
reflected particles of sand do not interfere with the ascending
particles,
RECTILINEAR MOTION. 67
The weight of the ball will be equal to the rate at
which momentum is being destroyed, or created in a reversed
direction, when resolved vertically.
In other words the weight will be equal to the resultant,
which is clearly vertical, of the negative time-fluxes of the
momenta.
We shall assume that the velocity of the jet is consider-
able, so that we may neglect the changes in the velocities of
its particles due to the action of gravity.
If m be the mass of the unit of volume of the sand, and u
its velocity, the quantity which impinges on an elementary
zone in the time 6¢ is
m. 2aasin 8. acos 056. ust,
and the normal component of the momentum of this quantity
of sand is
2arma’u’ sin @ cos’ 6606E.
Multiplying this by 1+e, where e is the coefficient of
elasticity between the ball and the sand, we shall obtain the
quantity of motion created in the normal direction outwards
round the zone, and, dividing by &, we then obtain the
negative time-flux of the momenta, which is the pressure on
the ball.
5—2
68 RECTILINEAR MOTION.
The last result, when multiplied by cos@, will be the
resultant vertical pressure on the zone, and, if the breadth of
the jet subtend an angle 2a at the centre of the sphere, and
M be the mass of the sphere, it follows that
Mg =} wma’? (1 +e) (1 — cos*a).
If the ball be in motion, suppose that, at any instant its
vertical velocity is v; then the equation of motion of the
ball is
Mo = } wma? (u— v) (1+) (1 — cos* a) — Mg,
or 07 =a as (Qu — 0’).
Integrating we obtain
ge
Qu —v = Ce”;
and, if we suppose the ball to start upwards with a velocity
v, it will have its velocity destroyed after ascending through
the space
uw 2u
om ee Qu—v'’
and will then be under conditions consistent with equi-
librium.
The time in which this takes place is obtained by inte-
grating the equation
b= — 7, Quo —'),
and the theoretical result is that an infinite time must elapse
before the ball absolutely loses its velocity.
The simplest method of illustrating the idea of this article
is to employ a jet of water. The ball rises and falls inter-
mittently, and is occasionally at rest for a sensible time. As
in the case imagined of a jet of sand, the pressure is due to
the rate of destruction, and of creation in the contrary direc-
tion, of the momenta, in directions perpendicular to the
surface of the sphere, of all the elementary cylindrical shells
which constitute the impinging stream.
RECTILINEAR MOTION. 69
EXAMPLES.
1. A smooth wedge on a horizontal plane is moved from
rest with an uniform acceleration; find the direction and
amount of the acceleration that a heavy particle placed on
its inclined plane surface may be in equilibrium relative
to it.
If the acceleration be given, find the motion of the
particle, supposed initially at rest, upon the inclined surface.
2. Particles slide from a fixed point down rough planes
to points in the surface of a cone, whose axis, passing in
direction through the point, is vertical, and vertex upwards.
Shew that, if the vertical angle of the cone= 2 tan ,
the particles will all have the same velocity on arriving at
the cone.
3. Give a geometrical construction for determining the
straight line of quickest descent of a heavy particle from a
given point to a given curve.
If the curve be a conic, with its vertex upwards, the
length of the line of quickest descent from the focus to the
curve is equal to the latus rectum.
4, Determine the motion of a particle, initially at rest,
under the action of a force to a fixed point varying inversely
as the cube of the distance.
5. A train goes from one station to another a mile off,
being uniformly accelerated from rest in the first two-thirds
of the distance, and being brought to rest by uniform
retardation in the remaining one-third of the distance, and
taking 3 minutes to perform the journey. Find the ac-
celeration and retardation and the maximum velocity ac-
quired.
6. A hyperbola is placed in a vertical plane with its
transverse axis horizontal; prove that when the time of
descent down a diameter is least, the conjugate diameter is
equal to the distance between the foci.
70 RECTILINEAR MOTION.
7. Find the locus of points from which inelastic particles
may be let fall on a smooth inclined plane, so as always to
have the same velocity on arriving at the same horizontal
line in the plane.
8. Two equal weights are fastened to the extremities of
a string and are then hung over two small smooth pullies
A, B which are in the same horizontal line. If a third
equal weight be fastened at the middle of the horizontal
portion AB of the string, shew that it will descend a distance
equal to two-thirds of AB, and find the velocity in any
position.
9. Two bodies, 2P and P, are connected by an in-
extensible string, which passes over a fixed smooth pulley;
determine the motion and the tension of the string.
If, after the motion has gone on for one second, another
body P, having no velocity, be suddenly attached to the
descending body 2P, determine completely the subsequent
motion of the system.
10. Two elastic balls impinge obliquely, so that their
directions of motion are interchanged: prove that the
product of their velocities is unaltered, and that if their
masses be equal their directions make equal angles with the
line of impact and that their velocities are unaltered.
11. In an Atwood’s machine, if the string can only bear
a strain of one-fifth of the sum of the weights at its two ends,
shew that the larger weight is not less than 13 times the
smaller weight, and that the least acceleration possible is
V3
57
12. If two elastic balls impinge on each other with
equal and opposite momenta, their kinetic energy will be
reduced in the ratio e”: 1.
13. ee gs ee
2e 22 * gS
2
and only two if it be > —
RECTILINEAR MOTION. 73
23. A weight P hanging vertically just supports a
weight W in that system of pullies in which there is only
one string. Shew that, neglecting the masses of the pullies,
if P and W be interchanged their centre of gravity will
descend with an acceleration
CW = Py
We WP+ Ps
24. If the weight (P), on a wheel and axle, suspended
from the wheel preponderate over the weight (W) suspended
from the axle, prove that the acceleration of P is
aP—abW
IVW+@P ’
where a and 6 are the radii of the wheel and axle, the inertia
of the wheel and axle being neglected.
If an additional weight (w) be suddenly attached to W,
find the impulsive tensions of the two strings.
25. Two trains of equal weight are being drawn along
smooth level rails by engines, one of which exerts a constant
tractive force, while the other’s rate of working is uniform.
Prove that if their velocities at two instants are equal, the
second train moves through the greater distance during the
interval between the two instants, and that they are working
at the same rate, at the end of half this interval.
26. Two given points are in the same vertical line;
shew that the locus of the points in a vertical plane through
them, from which the times of descent to the two points are
the same, is a rectangular hyperbola.
Shew also that, if two equal circles be in the same
vertical plane, the locus of the points from which the times
of shortest descent to the circles are the same is a rect-
angular hyperbola.
27. A particle moves in a straight line under a centre of
attractive force w’r in that straight line ; if it be initially at a
distance c from the centre of force and be projected in the
(4 RECTILINEAR MOTION,
straight line with velocity V, shew that it will arrive at
the origin in a time equal to
pe
- I +__/.__. ,
B 10. af 7p? + pc
28. A cycloid has its base horizontal and vertex up-
wards; prove that the time of falling down any radius of
curvature is constant.
29. The mean time of descent down a given inclined
plane of unknown roughness is equal to twice that down
an equal smooth plane, all coefficients of friction, for which
motion is possible, being considered equally probable.
30. A heavy particle is attached by an elastic string to
a fixed point on a smooth horizontal table; the particle is
drawn out along the table till the string is double its natural
length (a) and it is then let go; find the velocity of the
particle in any position and shew that it will return to
the starting point after a time = 2y/ (7 +2): the modulus
of elasticity of the string being equal to the weight of the
particle.
31. Two equal particles which mutually repel one an-
other with a force varying as the distance between them are
connected by a light elastic string; find the condition that
the motion may be oscillatory; and assuming that the par-
ticles would rest in equilibrium with the string stretched to
twice its natural length find the amplitude of the oscillation
if the particles just meet.
32. Two particles start simultaneously from the same
point and move along two straight lines, the one with
uniform velocity, and the other from rest with uniform
acceleration. Prove that the line joining the particles at any
time is always a tangent to a fixed parabola.
33. An infinite number of particles are arranged along a
curve; they move normally to the curve with velocities
which are always proportional to the perpendicular from the
RECTILINEAR MOTION, 75
origin on the tangent to the locus at any instant. Prove
that they will always lie in a similar curve with the origin
for a centre of similitude; and that if they move so as to ap-
proach the origin, they will reach it together after an infinite
time.
34, ABCD is a smooth tube in a vertical plane bent up-
wards at Band C, BC being horizontal, and the angles ABC,
BCD, being equal and obtuse. An inelastic particle slides
from a given point in AB. Find the time it will take to
reach its highest position in CD; and if this time be equal to
that of the next similar stage of motion, and angle ABC = 135°,
shew that the original vertical height of the particle above
BOC=2 BC.
35. A smooth circular hoop, radius a, rests on a smooth
horizontal table; a small spherical mass is projected in any
direction from the centre of the circle with velocity v: prove
that the whole time that elapses until the nth impact is
a 2 — et sas e”
. v grt gh
where ¢ is the coefficient of elasticity.
Also find the ultimate velocity of the ring and sphere
after an infinite time.
36. An elastic string is extended between two fixed
points to double its natural length, and a particle of mass m
is fastened to the middle point of the string. If the particle
be drawn towards one of the fixed points through half its
distance from that point, and then let go, find the greatest
velocity which it subsequently acquires.
If a be the natural length of the string, prove that the
time of a complete oscillation is m/ma “af
37. A particle is placed initially at a distance a from a
centre of force the attraction to which varies inversely as the
distance; prove that the time of arriving at the centre of
. Tv
force is a a,"
be
76 RECTILINEAR MOTION.
38. The upper extremity of a piece of chain, hanging
vertically is made to move upwards, with a given acceleration ;
find the tension at any point of the chain.
39. An endless elastic string, modulus A and natural
length 27, is placed in the form of a circle on a smooth
horizontal plane, and is acted upon by a force from its centre
equal to wr per unit mass of the string. Shew that its
radius will vary harmonically about a mean length
2adc + 2arr— mpc,
m being the mass of the string, if 273A > mpc.
Examine the case when 27 = myc.
40. o, P will oscillate with period 27/,/u — o”.
41. A rod revolves about its middle point with uniform
angular velocity a and has at its extremities two centres of
force varying as the distance one attractive and one repulsive
of the same absolute intensity; supposing a particle placed
in the plane of rotation in a line perpendicular to the rod
through its centre, shew that its path will be cycloidal, the
time from one cusp to another being 27/a.
42. A smooth horizontal disc rotates with angular velo-
city J about a vertical axis at which is placed a particle
attracted to a certain point of the disc by a force whose
acceleration is sx distance; prove that the path of the
particle on the disc will be a cycloid.
43. A particle moves under the action of two constant
forces in the ratio of nine to one, whose directions rotate in
opposite directions with uniform angular velocities in the
ratio of three to one: prove that, under certain initial con-
ditions, the path of the particle will be a closed curve, of the
same form as that represented by the equation, r =a cos 20.
44, The two ends of a smooth weightless rod are move-
able on two fixed straight wires intersecting each other at
_right angles. A particle can move on the rod and is attracted
to the point of intersection of the wires by a force varying as
the distance. Prove that if the particle have initially no
motion the angular velocity of the rod is given by an equation
of the form
ow” = n? {1 —sin? 2a cosec” 26}.
CHAPTER VII.
RADIAL AND TRANSVERSAL ACCELERATIONS.
90. Havine discussed, in the previous chapter, the use of
the components of acceleration parallel to two coordinate
axes, we now take into consideration the expressions for
radial and transversal components, leading to the equations
of motion, 7
, f¥—-7rP=P, rO4+ 2d=Q,
mP and m@ being the radial and transversal forces acting
on a particle of mass m.
For our first illustration we take the following case.
Motion of a particle in a smooth straight tube which
revolves uniformly, in a horizontal plane, about a fimed point
in the axis of the tube.
In this case the only force acting on the particle is the
pressure R of the tube, and, if w be the angular velocity, the
equations are
r—owr=0, 2mro = R.
If the particle start from the distance @ with no initial
velocity along the tube, we obtain from the first equation,
r= 5 (e*# + e-°*) =a, cosh. ot,
and from the second,
R= 2mae’ sinh «ot.
ROTATING TUBES. 105
We can also obtain the velocity and pressure in terms of
r, for the first equation gives
Pr (Cd = a’),
and therefore R=2Ime’ Jr — a.
If b be the length of the tube, the direction in which
the particle flies out is inclined to the tube at an angle 0
such that
be b
t 6 = —___ = ——— 5
si o /P-a Je —a'
If the tube revolve in a vertical plane the equations are
*— o'r =— sin wt, 2mrw = R— mg cos ot.
From these equations,
= aoe sin wt + Ac? + Be Chapter IL),
2 P
and R= 2mqg cos wt + 2mo* (Ae** — Be-**),
the constants being determined by initial conditions.
91. Motion of a particle in a straight tube which revolves
uniformly in a horizontal plane about a fied point at a
distance c from tts axis.
If OA (c) be the perpendicular from the fixed point on
the axis of the tube, and, P being the position of the particle,
if AP =r, the acceleration of P relative to A =7— o'r, in the
direction AP, and 27 perpendicular to AP; and the accele-
ration, wc, of the point A is wholly in the direction AO.
Hence the equations of motion are
F¥—w'r=0, m(2Qrw+o’c) = f,
and the solution is similar to that of the preceding case.
Motion of two particles,m and m’, connected together by an
inelastic string, in a straight tube revolving uniformly in a
horizontal plané about one end. is
106 ROTATING TUBES.
If r be the distance of m from the origin, J the length of
string, and 7’ its tension, the equations are
m(#— o'r) = T, m' {F- ow (r+ )}=—7,
from which we obtain
(m +m’) #— o (m+ m') r — mol = 0,
tthe 1 = Aevt + Be-t,
and therefore r+
m+m
92. Motion of a piece of uniform chain in a straight tube
revolving in the same manner.
Let r be the distance from O of G, the centre of gravity
of the chain, GP =p the distance from G@ of one end of an
element PQ, (6p) of the chain, m the mass per unit of length,
T the tension at P, 7'+ 67 at Q.
The equations of motion of the element are, since p is
2
independent of the time and therefore (OP) equal to #,
mép {i — wo" (r+ p)} =8T, 2mdprw = Rp,
R being the rate of pressure at P per unit of length.
Integrating the first of these equations, or, in other words,
taking the sum of the equations of motion of all the elements,
we obtain
m{G—o'r)p-a GL = T+ 0,
ROTATING TUBES, 107
Observing that 7=0 when p=—I and when p=1, 21
being the length of the chain, there results
m (¥— o'r) 21=0, or #— o'r = 0,
shewing that the motion of the centre of gravity is the same
as that of a single particle.
Taking account of this result, 7’= 4mo’ (I? — p?).
93. Motion of a bead on a smooth circular wire revolving
uniformly in its own plane about a fixed point.
If O be the fixed point, and @ the angle PCA, the accele-
rations of P in the directions PZ’ and PC, obtained by
compounding the accelerations of P relative to C with that
of C relative to O, are respectively,
a q (6+ ot) + a%csin 6, and a(6 +)? +0°c cos 8,
taking OC =c, and CP =a.
If the plane be horizontal, and & be the pressure of the
wire on the bead, the equations of motion are
ab + wcsin@=0, and m {a(6+a)*?+’c cos 6} = R.
108 CENTRAL ORBIT.
If the bead be originally attached to the wire at the
angular distance a from the line CA, and be set free, the first
of these equations leads to
a” = 20° (cos 6 — cos a),
shewing that the bead oscillates through the angle 22, and
the second determines the pressure.
CENTRAL FORCES.
94. If a particle move under the action of an attractive
force mP to a fixed centre, P being a function of r, the
equations of motion are
¢#—7rP=—P, 164+ 270=0.
From the second equation we at once obtain
76 =h,
h being a constant.
Hence t= 79= 5 pa ap if “=
p= nt gai pe
and the first equation becomes
eae Pe
dé Y
du P
or ap Ya
This equation, if the law of force be given, determines
the path, and, if the path be given, determines the law of
force.
95. If A be the area swept over by the radius vector,
A=}r6=hh,
CENTRAL ORBIT. 109
and therefore A = ht, shewing that the area is proportional
to the time, and that 4h is the area swept over in the unit of
time.
If ds be an:element of the arc of the curve, and p the
perpendicular from the centre of force upon the tangent,
$A = Lpés,
and therefore: h=2A =pi=pv,
shewing that the velocity is inversely proportional: to the
distance of the centre from the tangent to the path.
96. We have shewn,.ix. Art. (17), that the normal accele-
ration, in any curvilinear path, is equal to v°/p, where p is
the radius of curvature.
If mF be the resultant of the forces acting on a particle
m,and ¢ the inclination to the normal of the line of action of
this resultant, it follows that
2
m i = mF cos $,
and therefore, if g be the chord of curvature in direction
of the force,
v= 489.
That is, the velocity of a particle at any point of an orbit
is that which the particle would acquire if it were to move
from rest under the action of a constant force, equal to the
force at the point, through a space equal to one-fourth of the
chord of curvature in direction of the force.
97. Since — and cos =f,
P r
Ve dr
we have pre PPT
2
and therefore P= z 7 ;
an expression which is frequently useful in determining the
path for a given law of force, or the law of force for a given
path. :
110 ° CENTRAL ORBIT.
We can also obtain the same expression for P by employ-
ing the expression for the tangential acceleration.
; dv dv.
Thus —Psin =z =v | sing;
__ hd /(h\ _h'dp
therefore Pa~ oo (S)-p ae
The two expressions for P are deducible, each from the
other, by help of the equation,
i sy (S).
o dé)"
98. Another expression for the velocity is found by
utilizing the expression for the tangential acceleration; we
thus obtain
dv dr
ta? ae
and therefore y=y?—2 | Pdr,
shewing that v is a function of the distance.
Further, since
h? 1. 1 /dr\?
2 pa SS ge
- p t {a+ (G5) f>
: dé. ‘ :
it follows that r dr 8% function of the distance, and therefore
that at all points which are at the same distance from the
centre of force the angle between the radius vector and the
tangent is the same.
We now proceed to apply these formule to some particu-
lar cases.
99. To find the law of force to the focus under the action
of which a conic section can be described.
CENTRAL ORBIT. 111
Taking as the equation of the conic
cu=1+¢ cos 8,
eet 6. and du lak
de: ecos Vv, an det Y=
2,2 2
so that pore ate)
¢c uh6UcclUr
and therefore varies inversely as the square of the distance.
If «w be the absolute force, that is the force at the unit of
; 2 2
distance on a particle of unit mass, yu =* = * , if LZ be the
latus rectum.
To find the law of force to the centre under which a central
conic can be described.
2
Employing the equation, P= 3 a we know that in
this case,
p (? + Gb? peas *) ace a’b*,
272 2
and therefore — no =— an so that P= e Tr;
ip p ab
and therefore varies as the distance.
2
If « be the absolute force, w = ore
100. To find the law of force to the pole under which an
equiangular spiral can be described.
From the definition of the curve, p=rsina,
and therefore P= .4=35)
and the velocity =
112 CENTRAL ORBIT.
To find the law of force when a particle describes a circle
under the action of a force to a point in the circwmference.
In this case Pe 5 , or 7° = 2ap,
2 2 2
and therefore P=" : “ = sl =4
: Qah_ 1 i”
and the velocity Soe Sal g:
101. Motion of a particle under the action of a force to a
fixed point varying inversely as the square of the distance.
In this case, P = pu’, and we obtain
du be
rT i
the integral of which is
u— =A cos (0-4),
or u =F {1 +ec0s (0 —y)},
which is the equation of a conic section, of which e is the
2
eccentricity, and x is the semi-latus rectum.
To find the constants, let c be the initial distance, v the
velocity of projection, and 8 the inclination to ¢ of the initial
direction of motion ; then,
‘ - au :
h=ve sin 8; and, since a ~i esin (@—y),
+ =H (1 +6 0089) and “cot @=—Hesiny,
or vesin’ 8 =p (1+ecesy), v’csin @ cos 8 = — pesiny ;
CENTRAL ORBIT. 113
whence = (v’e sin? 8 — p)? + v'c* sin’ B cos’ B = pe’,
vic’sin®B 2v*c sin’ B
2 ?
pb
ve
sod Enis Does.
p—ve sin’ B
or e=1+
It follows that the conic is an ellipse, parabola, or
hyperbola, according as v? is less than, equal to, or greater
Qu
than —.
c
If 2a and 2b be the axes when the curve is an ellipse,
2
hi
—=a(l—e’);
naa (L=e)
and therefore
ve* sin® B * (= sin’B a vc’ sin? 8)
2
a be ie
2
or foe
c a
Since any point may be regarded as the point of projec-
tion, the velocity at the distance r is given by the equation
pale _b
ra
In the same manner, if the conic be a hyperbola, we
find that 2
2 2p + & :
r
We can also solve this question by the use of the equation
h' dp _p_
pdr to #
leading to t _ 7H +6,
por
which is an ellipse, parabola, or hyperbola, according as C is
negative, zero, or positive.
B.D. 8
Vv
114 CENTRAL ORBIT.
: Qu
If C=0, the velocity = tage :
p r
If the curve be an ellipse or hyperbola, the axes of which
are 2a and 2b, we find by comparison with the equation
fe 2atr
p —- r >
2 2
that w= aoe , if Z be the latus rectum, and that
AP Dye _
v= = - + .
102. The case in which the force varies as the distance
has already been dealt with in Art. (81), but we can also use-
fully employ the equation
h? dp
Pp aia
2
leading to a =C-— pr’,
which is the equation of an ellipse.
Comparing with the equation
p(a@+h—r*)=a'b’,
‘we find that C= pu (a’+ 0°), and h? = pa)’, and that
aR ane +i *) = pw. OD",
if CD be conjugate to r.
103. Motion of a particle under the action of a repulsive
force from a fixed point varying inversely as the square of the
distance from that point.
The equation of motion is
a
CENTRAL ORBIT. 115
therefore ut ii =A cos(0—y),
? 1
or Be eee
Introducing the initial conditions, we find that
2 sae 2 5
ve sin Bat =a cay Aq BS sn BoP _ osin -
2 Sn 4A? gtd
therefore e=1+ ae ene + — ;
shewing that the conic is a hyperbola.
As in the previous case,
h 3
— =a(e’—-1
- (—1)
egaae ve? sin? B a (7 sin? 8 4 ve ste e .
be Be
2
and therefore fama,
a ¢
Hence, any point being a point of projection, we have at
the distance r
2u
=
als
104. Path of a particle projected at the distance a with
the velocity Ju--a in the direction at right angles to the
imitial distance, and subject to the action of a central force
which on unit mass is equal to
pe {2 (a? +B”) w’ — 30°0u'}.
In this case h = ae a=,/, and therefore
= $u=2 (a 4d) uv — Babe,
116 VELOCITY IN AN ORBIT,
Multiplying by 2 S integrating and observing that when
Uu= E og we find
a’ ao
(3) = u! (au? — 1) (1— Bu’),
restoring r this becomes
dé r
dr ~ I@—r ') (® — B)
Putting 2 = 7° —b’, and oe we obtain
7 — b? = (a? — b*) cos’ (9 —y).
But r=a when 6 = 0, and therefore y = 0, and
7 = a? cos* 6+ 6 sin’ 0
is the orbit, which is the pedal of an ellipse with regard to its
centre.
VELOCITY IN AN ORBIT.
105. If the orbit be central, the velocity is given by the
equation
r=,
a
In general, whether the orbit be central or not, the
velocity is given by the equation,
v=3% Ky,
where g is the chord of curvature in the direction of the
resultant force.
For instance if the orbit be an ellipse, the force being
directed to the centre C, and if v be the velocity at P,
v= $ nOP. “CO ncDe
VELOCITY IN AN ORBIT. 117
For an ellipse, when the force is to the focus,
Gat, 2 ee
sr Ay SP UAC
For a parabola, force to the focus,
2 2
v =1 gm 4SP=-
For a hyperbola, force to the focus,
2_y & 20D? Mw, pw
=t9p- 407 spt ac:
_ For a hyperbola when the force is repulsive from the
ocus,
Patt Pe ae
2" 3p” AC AC SP
For an equiangular spiral, force to the pole,
=p hora.
For the orbit,
v= a" cos?@ +b’ sin? @, Art. (104),
> will be found that
r
‘ ali _
P= TEER rage Od 9 AE METI,
106. If a particle move in a conic section under the
ction of a force to the focus, the velocity at any point can be
scomposed into two constant velocities, one perpendicular
' the radius vector, and the other perpendicular to the aais of
1@ conte.
The sides of the triangle SPG are perpendicular to the
rection of the actual velocity, and to the directions in
iestion. Hence the velocity, and its components are in
.e ratio of the sides of the triangle. GZ being drawn per-
118 TIME IN AN ORBIT.
pendicular to SP, the component perpendicular to SP
ce eg ee eee
“SY°' PG PL 4L oh
, Art. (101).
and, since SG=e.SP, the component perpendicular to the
axis = + :
It will be noticed that the latter component is in the
direction PN, or NP, according as the body is moving
towards, or away from, the vertex.
TIME IN AN ORBIT.
107. The time of passing from one point to another of
a central orbit is in all cases determined by the equation,
7? 6 =h, that is by the fact that the area swept over by the
radius vector is proportional to the time.
Time of traversing an arc of a parabolic path, when the
force is to the focus.
TIME IN AN ORBIT. 119
The parabola being’
eee
T+cos9) 78°" 9°
dt r at 10 aé. , s 2
dé = Pua Jan? “3 = 75, ( es 5) 6 a
and therefore t=a* ff a (tom e a tan® 5) ’
B& 2° 3 2
measuring from the vertex.
we have =
108. Time in an ellipse when the force is to the centre.
The equation of the ellipse being
cos’@ sin’? @ 1
oe TR
dor or | ab
dd h abdu Jp arsin 0+ 0 cos 0”
ab sec’ 0
az ar 6? + a* tan’ 0’
and therefore the time from the end of the transverse axis
1 atan 0
= —-tan’———_..
Ju 6
The Periodic time is equal to the area of the curve divided
by 4h, and
_ mab — Qr
daby/p
It will be noticed that this is independent of the size of
the orbit.
1
109. Time in an ellipse when the force is to the focus.
120 TIME IN AN ORBIT.
Taking <= 1+ecos@ as the equation of the curve, we
have
i a a
dO h Juc Jp’ (k+ecos 6)"
ee I dé _ [_cos@ te _ [cos 6d
(1+ecos 6) J(1 +e cos 6)’ (1 +e cos 6)
__sin@ =A) 2... ff | a,
l+ecos@ e/|1l+ecos@ (1+ecos 6)’ ”
therefore
0-6) [ape ret ico
=~ ot | rang
and the time from the vertex is therefore, since c=a/1—e’,
i Loa i
S- {otax (4/7 *tan 8) ead ée’ sin 6)
Ju l+e 2 l+ecos@ $
The total area being crab, the periodic time
= Qrab Qrrab Qrat
ho pale) Vp
This of course can be obtained from the preceding
expression by taking @=7, and doubling the result.
110. Time in a hyperbola, when the force is to the
Focus.
The process is exactly the same, only that, e being
greater than unity, the result of the integration appears in
the form
APSES AND APSIDAL DISTANCES, 12]
e— = no |
esin 0 1 [il St maar at
(-vf -
(1+ecos 6)? I+ecosO ,/e yi ” | hn
111. Time in the orbit, r? = a? cos? 6 + B sin? 6.
In this case h=,/u, /ut = [a0
therefore /ut=4(a? +b°) 044 (a? 0’) sin 20,
2
and the periodic time = ~ (a+ m (a + 68)
a
APSES AND APSIDAL DISTANCES.
112. An apse in a central orbit is a point at which the
tangent is perpendicular to the radius vector, and the length of
the radius vector at the point ts the apsidal distance.
We have shewn that, if the central force be a function
of the distance, the velocity at any point and the inclination
of the tangent to the radius vector are also functions of the
distance, and from these facts it follows that if the motion at
any point be reversed in direction, the particle will retrace
its path in the opposite direction.
For, supposing the particle projected from P with a given
velocity v to arrive at the apse A with a velocity wu, the
value of r _ is a function of v and r, and therefore if
Bas), =] Fodder
4
and if ASP =a, a =[ FO dr.
122 APSES AND APSIDAL DISTANCES.
Now, suppose the motion reversed at A; then the values
of 6 and a are the same as before, and the orbit is therefore
retraced.
p
S P
We hence see that any apsidal line dimdes the orbit
symmetrically.
For on arriving at A the particle is under the same
circumstances with regard to the direction AP’ as it was
when reversed with regard to the direction AP.
Hence it is obvious that, at an apse, the radius vector has
a maximum or minimum value, and further that, in a central
orbit in which the force is a unique function of the distance,
there can only be two different apsidal distances, although
there may be any number of apses.
113. It follows that we cannot ensure the complete
description of an orbit by placing a centre of force at any
assigned point. Take for instance the case of an ellipse, and
trace its evolute.
The centre of force may be at the centre O, or at any
point of each of the four limited lines AC, DB, EA’, FB’.
If a centre of force be placed anywhere else, as at K, the
normal KP does not divide the orbit symmetrically, and
APSES AND APSIDAL DISTANCES, 123
although a particle, projected from A, may describe the arc
AP, it will not proceed in the ellipse, but will describe the
are PA turned over to the other side of KP.
8 P
D
Al |A
EB KE Cc
Fr
B’
The same remarks apply to an orbit of any form.
114. If the law of attraction be inversely as the nth
power of the distance, that is, if P =u", the equation of
motion is
aw ut?
t dé 6 3 +u= rw ,
leading to
2
(35) += oH aa +¢.
Hence the apsidal distances are given by the equation
ee +0,
which cannot have more than two positive roots, a result in
accordance with that of Art. (112).
U
124 APSES AND APSIDAL DISTANCES.
If however the moving particle be so projected that
i= cer and C= mae ,
du\? ._Ac™ Su n—8
(i) Tad, tee
and the equation for the apsidal distances takes the form
(n—1) cu? = 2 (cu)"* + n — 3.
It is easily seen by taking the derived function that this
equation has two equal roots, that is, that there is really only
one apsidal distance, of length c.
we have
Taking n= 5 for example, we find that
(ae) "a
dé\? 2c"
and therefore (5) a (-r} .
Integrating we find that the equation of the orbit is
ge Qe op
e~ ted 7"
a curve which has an asymptotic circle of radius c.
Hence it appears that, when projected in the manner
described, the particle will make an infinite number of re-
volutions before arriving at the apsidal distance of its path.
If for another example we take n= 2, the equation of
the path is
(@) += 25-3
" (za) + (#-3) -0
shewing that o =0, and w= s
APSES AND APSIDAL DISTANCES. 125
or that the only possible path, under the conditions stated, is
a circle having the centre of attraction for its centre.
In fact it will be found impossible to satisfy the conditions
for any angle of projection which is not a right angle.
115. The peculiarity of the preceding case is that the
velocity of the apse is that which is suitable for circular
motion round the centre of attraction as a centre. /
For 0 = I’ {(36) + wh
dé
= anne {2 (cu)"* + n — 3}
=o when 7 =c,
116. A particle describes a nearly circular orbit about a
centre of force ; it is required to find approaimately the equa-
tion of the path and the apsidal angle.
If $(r) be the force, and if the particle be projected at
the distance c, perpendicularly to the distance with the velo-
city wf cd (c), it will describe a circle.
We shall suppose the particle projected perpendicularly
with the velocity 4/ c@ (c) at the distance c++, y being a very
small quantity.
We have then h? =(c + 7)’ cd (c), and if we suppose that
r=c-+ a, where a is very small,
_1l_1 @
7 6 Cc
a b(r)_ b(c+2) (c+2) (¢+y)?
es hae co (c)
1 Qa, ah’ (c) vy
=i(l4 e+ ee)”
if we neglect the squares of the small quantities.
126 APSES AND APSIDAL DISTANCES.
The differential equation then becomes
de of)
Bete B+ SS fam
and the ea equation of the path is
ore + Aeos{y/34 2 {) o+ah,
at the apses, - = 0, and therefore the apsidal ‘Angle is
3 + “i (c)”
Js+38
If (r) =r the apsidal angle is 3 , and if $ (r) =5 it is
equal to 7.
It will be seen that if the force vary as the nth power of
the distance n must not be less than — 3.
In other words if n is greater than — 3, a circular orbit
possesses the characteristic of stability.
If n= 3, the apsidal angle is infinite. In this case if the
particle be describing a circle about the centre of attraction
as centre, any slight divergence of path, without change of
velocity, will cause the particle to describe an equiangular
spiral.
117. Case in which $ (r)=r", where n is a positive
integer, the particle being projected from an apse at the distance
¢ with the velocity Juc™,
In this case the equation of motion is
du 1
dee t= Gare yi
leading to
(n+ 1) (cu)"? + 2—(n +3) (cu) _
(3) as (n+ 1) ot yt
=0.
RESISTING MEDIA. 127
Now if we take
F(a) = (n +1) a”? +2 — (n+ 3) v™,
we find that the equation, f(x) =0, has two roots equal to
unity, and, further, that for positive values of w, the function
J (a) is always positive.
Hence it follows, from the equation of motion, that
du
dé
or that, with the assigned conditions, a circle is the only
possible path.
=0, and r=c,
If in this case a slight disturbance of path take place, a
nearly circular orbit will be described, the apsidal angle being
a)din + 3.
118. Motion of a particle under the action of a central
Jorce, in a medium the resistance of which varies as the square
of the velocity.
Taking the transversal acceleration, we have
a ae
rd = FS as ksré,
1 ae ihe. gs
or andi (7°60) = — ks,
and therefore 76 = he-™, h being a constant; or, if p be the
perpendicular on the tangent,
ps =he-®,
Taking the normal acceleration,
# aa 5p he —iks — P) dr
= pe = Pap"
By help of the equation
: ieee al
po +(33 )
128 RADIAL AND TRANSVERSAL
this is transformed into
d*u P
qe t= Bye
119. 6, and is projected from an apse at a distancea+b
with velocity ./~ + (a+b): shew that its orbit is
r=a+bcosé.
36. If the parabolic orbits of two comets intersect
the orbit of the earth, supposed circular, in the same two
given points, and if ¢,, ¢, be the times in which the comets
respectively move from one of these points to the other,
prove that
4\3
¢+yi+¢-o8=(5),
the unit of time being a year.
37. The pedal of a curve with respect to a point is
defined to be the locus of the foot of the perpendicular drawn
from the point on any tangent to the curve, and the pedal of
the pedal with respect to the same point is called the second
pedal, and so on; a particle describes the n'™ pedal freely
under the action of a force tending to that point; find the law
of force.
If the curve be a rectangular hyperbola, and the pedals be
formed with respect to its centre, prove that the n™ pedal
will be the orbit of a particle moving under the action of
6nt+1
a force varying as r*", where r is its distance from the
@
centre of force.
138 EXAMPLES,
38. A particle is projected with velocity v from the
vertex of a cycloid and describes the curve under an attraction
to a centre of force situated on the axis at a distance from the
vertex greater than the diameter of the generating circle and
less than twice that diameter; prove that the particle will be
again at an apse after a time
a 2a’ cosa+ 3asin2+ 3 sin*a cos «
o° acosa+sin a
a being the radius of the generating circle of the cycloid, and
a the apsidal angle.
x
39. A particle P describes a central orbit, centre
of force 8, and through P is drawn a straight line at right
angles to PS, which line touches its envelope in @: prove
that the velocity of Q
1 /d’r
o ? (Gat) 5
and is constant only when the path of P is a parabola, whose
focus is 8S.
40. 2ga and <4ga, the highest point is given by
_ uw—2ga
cos 6 = — Iga?
and the pressure vanishes, and changes sign, when
2
cos =— ™ =e
3ga
(4) If w’>4ga and < 5ga, the particle rises to A and
passes over and the pressure vanishes when
2
deg 2 ee
3ga
(5) If w= 5ga, the pressure vanishes at A.
‘ (6) If w?> 5ga, the pressure never changes sign.
Oscillation of a Pendulum.
126. A heavy particle, suspended by a string from a
fixed point, and oscillating in a vertical plane, forms a simple
pendulum.
Measuring @ from the vertical, and observing that if a be
the length of the string, s =a, the equation of motion is
a =—g sin 8.
If the amplitude of oscillation be very small, the approx-
imate equation is
6+26=0,
a
and therefore 6=Acos (4/2 t+a ) oa
PENDULUM. 149
This represents isochronous vibrations, the time of
a complete vibration being 2a yi F é
Finite motion of a Pendulum.
Recurring to the equation, ad =—g sin 6, and supposing
the pendulum to start at an inclination @ to the vertical,
we obtain
a? = 2g (cos 6 — cos a),
and therefore if + be the time of oscillation, from one side to
the other,
rae ei jones vi; | Jaojnmt
Panag ¢ sin ; =sin 5 sin yy, this transforms into
ravi Tuan ae
=2/2F (sin$.5)
If 6 be the angle at the time ¢ from the lowest point,
~M Qglq ./cos@—cosa g ai ae & sin’ ‘
0
nf
= Js F (sin 5%) ‘
sin? = 5 sin! =
150 MOTION ON
or, in the notation of Jacobi and Guderman,
vnm(y/).
and the height of the bob of the pendulum = 2asin’® #
2
wasnt wt (4/21), sind
=2asin?§ ont ( at) 2 mod. sin 5.
127. Motion of a heavy particle on the arc of a smooth
cycloid, having its vertex downwards, and axis vertical.
Measuring ¢ from the tangent at the vertex, the intrinsic
equation of a cycloid is
s= 4a sin ¢,
and the equation of motion is
§=—gsin ¢, or 8+ 2 5 =0;
1.8=A.c0s ( Lita),
4a,
shewing that the motion is an isochronous vibration, the
period of a complete vibration being
tr 4/2.
g
128. Motion of a particle in a smooth circular tube under
the action of a force to a fiaed point varying as the distance
Srom that point.
Take a as the radius of the circle, and c as the distance of
the centre of force S from the centre C.
Resolving along the tangent, the equation of motion is
© = ur cos SPL = pr
v at
SMOOTH CURVES. 151
and therefore 0° = yw {(c + a)* — 7°} = 2uac (1 — cos 6), supposin
the particle to start from A. Leepe ), Supposing
If R be the pressure on the particle, measured inwards,
2
a= mur cos CPS +R = mpPN + R,
or mal? = mp (atc cos 0) +R,
therefore 2 = mp (2c —a-— 3c¢ cos 0).
129. Motion of a particle on the arc of a smooth equi-
angular spiral under the action of a force from the pole.
If mP be the force from the pole, and & the pressure
measured inwards, we have
ne
v oF pie me Sin 4 = mP sina — R.
ds r
Tn the case in which P= y/r’ these equations give
dv p ‘ 1 1
oe ae or, =u (5-2),
if the particle start with no initial motion from the distance
a, and the second equation determines the pressure.
152 -MOTION ON
We also have
o- v COS 4 = COS % pees
and therefore the time from the starting point to the distance
b is equal to
I & Jar dr
a C084 /9u (r—a)
130. Motion of a particle on the are of a smooth hypocy-
cloid, under the action of a force to the centre varying as the
distance.
Taking BAB’ as the arc of the hypocycloid, of which A is
the vertex, measure the arc from A.
In the figure C’ being the centre of the rolling circle of
radius 6, Q is the instantaneous centre, and HP, PQ are the
tangent and normal to the hypocycloid at P.
D
The angle YOA being ¢, we see that
ad
a . o_ 2b¢
p+O= 5, and ae Oa or!
and p=OY=(a—-26) cos OF = (a~ 2b) cos —2F ,
SMOOTH CURVES. 153
The curve being convex to the point O,
ds__ dp _4b(a—b) ad
dp? ag a— “a —2b"
ie _ ab
and therefore s=4 a (a —b) sin an 2b"
The equation of motion is
. dp
§=— pOPcos OPY=—pPY=p ds:
% par =
or, oS gee)
shewing that the motion is oscillatory and isochronous.
A geometrical proof of the isochronism of the hypocycloid
will be found in the Principia, Book 1., Section x.
If we make the radius of the circle infinitely large, and
the quantity » infinitely small, and take ua =g, we fall upon
the case of cycloidal motion, and the above equation becomes
s+ is = 0, as in Art (127).
131. Motion of a particle sliding on a rough curve.
The equations of motion are, if BR be the pressure,
measured inwards, and pw the coefficient of friction,
du
mv ds =mT — wR,
v
m - =mN+4+ Rf.
Taking the case, for instance, of a heavy particle sliding
upwards on the arc of a curve in a vertical plane, we have
dv .
my 7 = — mg sin p — whi,
v
a
where ¢ is the inclination of the tangent to the horizon.
154 ROUGH CURVE. RESISTING MEDIUM.
dv vw ‘
Hence Seti ony HECee),
2
om oS + 2yo* = — Qgp (sin $ + cos $),
and, the intrinsic equation s=/() being given, p=/' (4),
the equation is that of Chapter II. (1).
132. Motion ofa heavy particle in a medium the resistance
of which varies as the square of the velocity.
Measuring ¢ downwards from a horizontal line, the
equations of motion are
dv : a e
07, = 9 sin b — ke’, and 3 =9 cos ¢.
The second equation shews that for a given velocity the
curvature is independent of the resistance, a theorem which
is true for motion in any resisting medium under any forces.
Eliminating v we obtain
cos of- 3p sin @ + 2kp* cos ¢ = 0,
d *) 1 :
or, =, |—])+8tan ¢.-— = 2k, leading to
dg (; ? p -
sec’ dh
=k {tan ¢ sec d + log (tan $ + sec ¢)} + C,
and this is the intrinsic equation of the path.
133. The question sometimes arises whether a given
curve can be described by a particle under the action of forces
to two or more fixed points. In such cases we obtain equations
2
for v - and — , and the value of v? obtained by integrating the
first must be identified with the value of v* obtained from.
the second.
If for instance the curve be an ellipse and the forces
Kw
2 to the two foci, we have
S and
TWO CENTRES OF FORCE. 155
From these equations,
pags 4
r
, , 2
d A ae :
an v = ae since p sin d AG’
134. Motion of a particle fastened to a string which is
wound round a fixed curve.
Suppose that when the string is completely wound up,
the particle is at A, and measure s and ¢ from A and the
tangent at A.
Then PQ=s, and the path of P is an involute of the
curve, its radius of curvature being PQ.
Taking mS and mN as the forces perpéndicular and
156 PARTICLE ON A STRING.
parallel to the string, and 7’ as the tension, the equations of
motion are
modv
do
o being an arc of the path, or
ve
=m8, i es
mode _
sdb
If there are no acting forces, v is constant, and the tension
varies inversely as PQ.
mS, m= =T+mN.
Ex. Let the curve:be a circle and the acting force a
repulsive force from the centre varying as the distance.
In this éase v a = pa,
do
so that the motion is uniformly accelerated, and
a = T—muys,
so that, if the particle start from rest at A,
T = 2mps.
135. Motion of a string or fine chain inside a smooth tube
of any shape under the action of given forces.
Taking AB as the chain, we let s represent the length
OA of the axis of the tube, measured from a fixed point 0,
and let o represent the length AP of the chain.
. Then if 7 be the tension at Pand 7+ 687 at Q, and Réc
be the pressure of the tube on the element PQ, the equations
of motion of the element, the mass of which is méc, are, ob-
serving that the velocity and the tangential acceleration of
every point of the chain are the same,
mobo .8 = 81 + méc8,
and mda : = re +m8oN + Ric,
MOTION OF A CHAIN, 157
where S and W are the tangential and normal forces per unit
of mass.
O
Taking J as the length of chain and integrating the first
equation from A to B,
l
w= Sdo,
0
and the second equation gives
- +2
R=m= —7— mW,
As a particular case consider the motion of a heavy chain
inside a smooth circular tube in a vertical plane.
Measuring from the vertical radius, and from OA, take
COA=6, and AOP = ¢.
The equation of motion of the element PQ, or madd, is
mad .ad = mads.g sin (0 + ¢) +67,
and therefore taking a as the angle subtended by the string,
mahé = T — mga cos (0 + ¢) + mgacos 6,
158 MOTION OF A CHAIN,
a
and aa6=g {cos 0 —cos (6 +a)} = 2g sin (0+5) sin 5,
i Opin * @ g
whence aad? = 29 sin 5 {eos 3 — 008 (8 + 5) :
if the end A start from C.
eae
For the rate of pressure at any point,
mad. ab? = mad}>.g cos (0 +) + TS¢ — Radd,
or Ra = mga cos (6+ 6) + T— mae.
136. Motion of a piece of fine chain inside a smooth
circular tube which is revolving in its own plane about a point
in its circwmference.
AB being the chain, let ECA =06, and ACP =¢.,
The acceleration of the point P with regard to C, in
direction of the ve is
af, (0+¢), or a8,
MOTION OF. A CHAIN, 159
and the acceleration of C is w’a in the direction CO; there-
fore the equation of motion of the element PQ is
madp {ab + wa sin (6 + ¢)} =87,
and, integrating from A to B, that is from ¢=0 to =a,
a0 = {cos 0 — cos (6 + a)} = 207 sin (0 + 5) sin 5°
and therefore «a6? = 0 — 40 sin 5 cos (6 + 5) ‘
the constant being determined by initial conditions.
137. The equations of motion of a free string in a plane
under the action of given forces in the plane,
If, at any instant, w and v be the tangential and normal
velocities of point P of the string, and ¢ the angular velocity
of the tangent, the accelerations of P are
io — vp, and t+ ud.
Hence the equations of motion of an element PQ are
més (%— vd) =8T + més. 8,
més (i + ud) = 72 +mos.W,
160 MOTION OF A CHAIN.
p being the radius of curvature of the string at P and mS,
mV the forces per unit of length,
or m (ig) = + mS, m (itu) == + mW,
The string being inextensible, the geometrical condition
is that the motion of Q relative to Pis ultimately perpen-
dicular to PQ, and leads to the equations, ,
(uw + 8u) cos Sp — (v + dv) sin dp =u,
86 _ (v+ Sv) cos bp + (wu + du) sin dy — 9
a 8s :
Sy being the angle between the tangents at P and Q; or
ultimately
du_v
dsp’ andy “ast p’
138. A particular case is that of an endless chain originally
at rest under the action of conservative forces, and the
reactions of smooth curves, and set in motion in such a
manner that each point of the chain begins to move in the
direction of the tangent at the point.
In this case the chain will retain its form.
For, if v be the velocity of each point of the chain,
the equations of motion of an element ds are,
2
0=més. P +687, mBs més. Q + =;
or 0=mP+© (P—mi), O=mQ-+e (2— mai),
leading to P+ = (Qp) = 90,
as the equation giving the form of the curve when there is
no motion, and it therefore follows that the chain retains its
form, but that the tension at each point is increased by mv’.
MOTION OF A CHAIN, 161
This question is discussed in the solutions of the Tripos
. ° Questions for 1854 by, Mr Walton and the late Bishop
Mackenzie.
Mr W. Froude, in a letter in Nature, in November 1875,
described the experimental fact that a heavy endless chain,
placed over a drum, and made to revolve rapidly, retains
unchanged the catenary form which it assumes when not
in motion; and further that if an indentation in the form
be made by a blow from a heavy hammer, the inden-
tation, if the rotation be very rapid, remains for a considerable
time.
In the latter case the tension becomes so great that the
action of gravity is unimportant, although of course, the
action of gravity will, in time, remove the indentation and
restore the catenary form.
139. The equation for determining the initial tension of
a@ string.
The problem to be considered is that of a string on the
point of motion, under the action of given forces, as for
instance a string which being in equilibrium is cut at any
point.
Let PQ (8s) be an element of the string, and més.8,
mésN the tangential and normal forces acting upon it.
Take a, 8, a+8a, @+68 as the tangential and normal
accelerations at P and Q respectively, and 7, 7+ 67 as the
initial tensions at P and Q.
Then, 56 being the angle between the tangents at P
and Q,
mos .a=87' + més. 8, and més. 8 = (T+ 67) sindd + mésN,
ds
where p is the radius of curvature.
T
or, ultimately, m2z= ae +mS, mB= a +mN,
We have also the geometrical condition that the accele-
rations of Pand Qin the direction PQ are the same; and
B. D. 11
162 MOTION OF A CHAIN.
hence, 8¢ being the angle between PQ produced and the
tangent at @, we obtain
(a + 82) cos dp — a — (8 + 68) sin 86 = 0,
or, ultimately, 7 -& =0,
and, therefore, from the mechanical equations above,
@T aS T,mN
ds* biel a a p-
If one end of the string be fixed, we have, in determining
the constants resulting from integration, to introduce the con-
dition that the tangential acceleration at the fixed point is
zero, and, if either end of the string be moveable on a fixed
curve, the condition thereby introduced is that the accele-
ration of that end of the string in the direction of the normal
to the curve is zero.
Mathematical Journal, 1864.
For example suppose that a catenary, the upper ends of
which are fixed, ts severed at the vertex.
We have s=ctand, ee ¢, N=—g cos ¢,
and therefore a8 —g cos
2 1
The equation is i =o or, transforming,
gnc 2a psig Tcosf=0.
Integrating a cos $ — 7'sin d = C,
and therefore T cos = C+.
If ¢=0, 7=0, and T’cos ¢ = Co.
MOTION OF A CHAIN. 163
If a be the value of ¢ at the upper end,
dT :
wee sing =0, when ¢=y,
which gives i ae
cosy+ysin y
For another example take the case of a catenary the ends
of which, held apart, can slide on a smooth horizontal rod, and
umagine the ends let go.
In this case, as before,
Tcos$=Ch+C’,
but the geometrical conditions are that the tangential accele-
ration of the vertex is zero, and the vertical acceleration of
each end zero.
Therefore =0, when $= 0, which gives C=0, and
T=C'sec ¢,
and asin y+ cos y=0, when ¢=y,
leading to O'=mge and T =mgc sec ¢.
The vertex has no initial acceleration, and the horizontal
acceleration of each end is g siny (1 —sin ¥).
140. A heavy chain, lying on a smooth horizontal plane,
receives tangential impulses at one or both ends; it is required
to find the impulsive tension at any point, and the direction of
the initial motion.
Taking u and v as the tangential and normal velocities of
a point P of the chain, and 7’as the impulsive tension at P,
the equations of motion of an element PQ are
mos.u = dT, mis.o= 0;
aT T
or mu=—, and mv=—;
ds p
11—2
164 MOTION OF A CHAIN,
and we have besides the equation of continuity expressing the
fact that in the limit, the velocity of Q in direction of the
tangent at P is the same as the velocity of P in that
direction.
This condition gives us
(u + du) cos 86 — (v + bv) sin 86 = u,
on dp’ dsp
We hence obtain for the impulsive tension, the equation,
rT :
ds* ~ p .
If the chain be heterogeneous, that is, if m be a variable
quantity, the equation is
aT 1ldmdT T
ds* mds ds p*
As an example take the case of a piece of chain in the
form of a portion of a catenary, bounded by a chord parallel
to its directrix, and suppose that equal tangential jerks are
applied simultaneously at its two ends.
Since s=c tan ¢, we obtain
2
cos pS? sing TAT T cosh =0,
and therefore T cos¢ = 064+C,
At the vertex, u=0, and at each end, 7 =P, if P be the
tangential jerk; and we obtain, y being the extreme
deflection,
Tcos 6 = P cosy.
Moreover meu = P cosy sin ¢, and mcv = P cosy cos ¢,
and therefore v=ucot d,
shewing that every point of the chain begins to move in the
direction parallel to the axis of the catenary.
MOTION OF A CHAIN. 165
Ex. (2). Ifa chain in the form of a quadrant of a circle,
the density at any point of which, measured from one end varies
as e°, receive a tangential jerk at the other end, we have
1dm_1
mds a’
and our equation is
&@T dT
de ap 7 = 9
the integral of which is given in Chapter II., and the geome-
trical conditions are that .
T=0, when 6 =0, and that 7’ = P when 0=4;
these conditions determine the two constants of integration.
EXAMPLES.
I. A lamina, in the form of a regular polygon, is placed
flat on a smooth horizontal plane, and fastened to the plane ;
a string, the length of which is equal to the perimeter of the
polygon, is wound round it, one end being attached to an
angular point, and the other end carrying a particle; if the
particle be projected horizontally, at right angles to the
string, find the time after which the string will be wound up
again, and its greatest and least tensions. If the lamina be
held in a vertical plane, and the particle be projected in the
same plane, with an initial velocity sufficient to keep the
string always stretched, find its velocity at the instant the
whole string becomes straight, the side of the lamina-with
which the particle is initially in contact being horizontal and
downwards.
2. A small bead is projected with any velocity along a
‘circular wire under the action of a force varying inversely as
the fifth power of the distance from a centre of force situated
in the circumference. Prove that the pressure on the wire is
constant,
166 ‘ EXAMPLES,
3. A particle is placed at the extremity of the vertical
minor axis of a smooth ellipse and is just disturbed. Shew
that if it quit the ellipse at the end-of the latus rectum the
eccentricity must satisfy the equation e°+ 5e*+ 3e"= 5.
4. Ifa particle hanging vertically by a string be pro-
jected horizontally, and rise to a point P, and there leave the
circular motion, shew that if it recommences circular motion
at Q, PQ and the tangent at P to the circle will make equal
angles with the vertical,
5. If a particle move under the action of forces F, F’,
to any number of fixed points, and if g, q’,... be the chords of
curvature of the path in directions of these forces,
2mv? = & (FQ).
6. A uniform circular ring rotates uniformly in a hori-
zontal plane about its centre. Shew that the greatest possi-
ble linear velocity of its particles is independent of the radius
of the circle and of the cross section of the ring.
Find the breaking tension in pounds per square inch
in the case of a uniform ring of radius a feet which is on the
point of breaking when it makes » revolutions a second,
the weight of a cubic inch of the material of the ring being
that of c ounces.
7. Two equal particles which repel each other with
a force = pu (distance) * are placed on the inner surface of a
smooth sphere (rad. a), and their initial distance subtends
an 422 at the centre: shew that they will perform isochro-
nous oscillations in intervals = 27ra?,/2 sin a/./u.
8. A particle descends the arc of a smooth cycloid whose
axis is vertical from the base to the vertex.
If a horizontal line through the particle meet the circle
described on the axis of the cycloid in @, the velocity of
approach of the particle to Q is constant and equal to half the
velocity of the particle at the vertex of the cycloid.
9. 34, where p is. the coefficient of friction,
168 EXAMPLES,
Between what limits must yw lie in order that the particle
may come to rest at the end of its m™ semi-oscillation ?
16. A fine parabolic groove has its axis vertical and
vertex downwards, an elastic string has one extremity at-
tached to the focus, and the other to a particle in the groove;
the natural length of the string equals one-fourth the latus
rectum, and the weight of the particle is such as to stretch
the string to twice its natural length ; determine the position
of equilibrium, and shew that the time of a small oscillation
about it is 27 /2a/g.
17. If a particle, mass m, be acted upon by equal
constant forces mf in the directions of the tangent and normal
to its path, and if the resistance be mfv"/k’, prove that the
intrinsic equation of the path is
2fe
ie fe Me 1) =u? (e—1),
u being the velocity of projection.
18. Two elastic strings the natural length of each of
which is 47ra, are fastened at a point P in a circlar tube
(radius a) of small bore; the strings are stretched in opposite
directions, and their other extremities fastened to a particle
of given weight. If the plane of the tube be horizontal, and
the particle be displaced from its position of equilibrium
through an angle less than 7/2, shew that the time of an os-
cillation is independent of the extent of the displacement,
19. A heavy particle is projected upwards from the
vertex, within a smooth parabola whose axis is horizontal,
with the velocity due to a fall down the latus rectum (4a).
Investigate the subsequent motion, and shew that the particle
impinges upon the parabola again, at a distance 3a./13 from
the vertex, with a velocity that bears to the velocity of pro-
jection the ratio /5 : /2.
20. A particle describes a circular arc under the action
of a constant force not tending to the centre; shew that it
will oscillate through a quadrant.
EXAMPLES. 169.
21. A particle is moving on the convex side of a rough
equiangular spiral towards the pole, under the action of a
force to the pole =«v, where v is the velocity at distance r.
If V be the velocity at distance a, and ¢ the time of moving
from distance r to distance a, shew that, « being the coeffi-
cient of friction,
ta 1
at 22V cosa+psina y — ¢(-cosartwsinaat}
pitetana _ itp tana — =
K cOsa— msInz
where « is the angle of the spiral.
22. Having given that the normal acceleration varies as
the square of the velocity parallel to the axis of a, find the
path; and prove that if this path be described under the
action of a force parallel to the axis of y, then the whole
acceleration at any point is proportional to the velocity.
23. If the curve whose intrinsic equation, referred to a
horizontal tangent, is s* sin ¢=a’ be described by a particle
under the action of gravity, find the time of descent from any
point of the curve to the horizontal tangent.
24, A particle, mass m, moves in a smooth circular tube
of radius a, under the action of a force, wm (distance), to a
point inside the circle at a distance ¢ from its centre; if the
particle be placed very nearly at its greatest distance from
the centre of force, prove that it will pass over the quadrant
ending at its least distance in the time
Ja log (\/2 + 1)//ue.
25. a. If V be the velocity of the
particle when at its greatest distance from O and 1 its velocity
after describing an ¢ @ from that position, shew that
v= V?—-2f {e+a— Ve +a? + 2ac cos G}.
Find also the tension of the string and shew that
y’ + 5fa.
170 EXAMPLES,
26. A heavy particle is projected in a resisting medium ;
if » be the velocity at any time, @ the inclination to the
vertical of the direction of motion, and f the retardation,
prove that
\
1 du fo
a ae
If f=’, find v in terms of ¢.
27. Prove that the curve possessing the property that
the product of the distances of any point on it from two fixed
points is constant, may be described with uniform velocity
under the action of two forces, each tending to one of the
fixed points, and varying as the distance from the other, the
absolute intensities of the forces being the same.
28. Prove that a particle can describe a parabola under
a repulsive force in the focus varying as the distance and
another force parallel to the axis always of three times the
magnitude of the former; and that if two equal particles
describe the same parabola under the action of these forces,
their directions of motion will always intersect on a fixed
confocal parabola. ‘
29. Find the time of a small oscillation of a particle
suspended from a point by a string of length J, when the
square of a, the angle of oscillation, is neglected ; and shew
that the time will be r (1 + ia) sf 7 if the approximation
include the square of a.
A weight is drawn up uniformly and slowly with velocity
u by means of a crane; shew that the times of small oscilla-
tions will decrease at first in arithmetical progression, the
‘common difference being m*u/2g.
30. Two equal particles, connected by a fine string, are
placed in a circular tube, to one point of which they are
attracted with a force varying inversely as the distance; one
of the particles being initially at its greatest distance from
the centre of force, and v, v' being the velocities with which
EXAMPLES. 171
they successively pass through the point whose distance from
ee yt
the centre of force is 90°, shew thate “te “=1.
31. Two equal particles are connected by a string passing
through a small hole in a smooth horizontal table, one
particle hanging down, and the other held on the table; if
the latter be projected along the table at right angles to the
string with the velocity V2gc, prove that the initial radius of
curvature of its path is 4c.
32. Within a smooth circular tube of radius a held fixed
“in a vertical plane lies a light string of length greater than
half the circumference of the tube. The string carries equal
weights at its ends, which balance within the tube, and the
string subtends at the centre an angle 2 (w—a). If they be
slightly disturbed, shew that the time of a small oscillation
is the same as that of a simple pendulum of length a sec a.
33. A particle moves under the action of a central force
which is such that the normal acceleration on the particle
is constant: find a differential equation of the first order
to the path of the particle, and shew that 7° sin30=a’ is
a particular integral.
34, A heavy particle moves on a smooth curve in a
vertical plane, the form of the curve being such that the
pressure on the curve is always m times the weight of the
particle: prove that the time of a complete revolution is
2am/a/./g (m?—1)*, and that the length of the vertical axis
of the curve is 2ma/(m? —1)*, the whole length of the curve
being ma (2m? +1)/(m?—1)4.
35. A small smooth heavy bead runs on a string
fastened at two points in the same vertical line: the string is
originally vertical and the bead in its lowest possible position,
the bead is then projected so that it proceeds to describe
a portion of an ellipse, the string being at first tight; prove
that if the string becomes slack when the bead is at the
extremity of one of the equi-conjugate diameters of the
172 EXAMPLES,
ellipse, then the free path of the bead will pass through the
other extremity of the same diameter, and the latus rectum
of its free path will be to that of the ellipse as 1: 2/2.
36. On a wire in the form of a parabola with axis
vertical and vertex downwards is a bead attached to the
focus by an elastic string whose natural length is one eighth
of the latus rectum and whose modulus is equal to the
weight of the bead. Prove that the time of a small oscillation
is 27,/a/g, where 4a is the length of the latus rectum.
37. A particle slides down the arc of a vertical parabola ,
with vertex downwards starting from rest at a height h
above a horizontal line through the vertex. Shew that the
time of descent to the vertex is equal to
VES Wea).
where E£' (k) denotes the complete second elliptic integral to
modulus k.
38. <), if
projected from a point in the line CS distant a from C with
Je @ +e)
2a (a? —c’)
39. A smooth wire is bent into the form of a circle
radius a, and rotates with uniform angular velocity w abouta
then taking each force to be
a velocity perdendicular to CS.
EXAMPLES, 178
vertical axis through the centre which makes an angle a with
the plane of the circle. If a smooth bead slide on the wire,
shew that the equation of motion of the bead along the
wire is
ad’ eos gs. 8 #8
dp 7 2@ 008" a cos = sin = —g cos asin
where s is measured from the lowest point, Hence find the
position of equilibrium of the bead, and the time of a small
oscillation about that position.
40. A heavy particle hanging by a string from a fixed
point O is projected horizontally and describes a portion of a
circle greater than a quadrant until when it arrives at a point
P the string slackens and it begins to move in a parabola:
shew that the circle is the circle of curvature of the parabola
at P, and that if OP be produced to meet the directrix the
locus of the intersection 1s a circle concentric with the given
one.
41. A heavy bead slides on a smooth fixed vertical
circular wire of radius‘a: if it be projected from the lowest
point with a velocity just sufficient to carry it to the highest,
prove that the radius through the bead will, in a time ¢,
turn through an angle
= (sin /f
2 tan (sink A a t)
42, Ifa particle move on an ellipse under a force to the
centre = mr — nr log a . where c?=a’+6’, and N be the
-pressure on the curve, p the radius of curvature, prove
Np = 2ner + constant.
'
If the velocity vanish at an extremity of the major axis
and ~ = log = , then
n c—a
Np = 2ne (r —a).
43. Snow is uniformly spread over the surfaces of a
conical pinnacle and of the hemispherical dome of a building.
174 EXAMPLES,
It begins to slide off, starting at the highest point and
clearing a path as it goes. Prove that the motion in the
two cases is the same as that of a free particle moving on the
surfaces under the action of a vertical acceleration equal
to one-fifth and one-third the acceleration of gravity re-
spectively.
44, Ifa heavy particle be projected with a given velocity
and in a given direction prove that the initial curvature of
the path is independent of the resistance. Shew that, if the
resistance = p (velocity)’, the radius of curvature (p), at the
point where the tangent is inclined at an angle ¢ to the
vertical, satisfies the equation,
sin g $f + 8p.cos $+ 2up'sing = 0;
and that, if 1/p’ be the curvature at the other point where
the inclination to the vertical is the same, the curvature at
the vertex is
Lod
2 sin’ ( + 5) :
45. or mg cos a, and that
2v" cos a < ag sin? a,
If the particle be slightly disturbed in direction of the
string, find the time of a small oscillation.
3. A point describes a rhumb line on a sphere in such a
way that its longitude increases uniformly; prove that the
resultant acceleration varies as the cosine of the latitude, and
that its direction makes with the normal an angle equal to
the latitude.
4. A material particle rests on a rough plane inclined at
a given angle to the horizon, the plane begins to rotate round
an axis perpendicular to it, with a velocity commencing from
zero and continually increasing. Determine the velocity at
which the particle will commence to move on the plane, and
the condition that the commencement of the motion is
simultaneous with that of the plane.
5. 2ag, it may do so, and find the
additional condition necessary.
15. ,
the particle will pass from the inner to the outer surface, and
back again, and so on, when ¢, its angular distance at any point
from the lowest point of the cross-section through that point,
takes the successive values given by 3 cos 6 = 2 cos 8.
EXAMPLES, 201
20. There are two points P and Q which move so that
the line of motion of each relative to the other is always
parallel to a given direction. If the motion of P, and the
initial position of Q be given, shew how to determine the
surface on which it must move. If the orbit of P be plane,
prove that this surface is a cylinder. If the motion of P be
that of a projectile in vacuo, and the relative velocity of
P and Q constant, determine the motion of Q.
21. A smooth hollow ellipsoid of revolution is fixed with
its axis (2a) vertical, and a particle is projected from a point
in the horizontal plane through the centre and on the inside
surface with a velocity /2ga and inclination « to the horizon.
Find « in order that the greatest depth below the centre may
be 2a/3, and find in that case the greatest height reached.
22. A smooth cylinder, whose transverse section is a
cycloid generated by a circle of diameter a, is placed with its
axis horizontal, the axis of the cycloidal section being vertical
and its vertex downwards. A heavy particle is allowed to
fall from rest at any point of the surface and is attracted by
a perfectly elastic plane perpendicular to the axis of the
cylinder, with a force varying directly as the distance from the
plane, whose absolute intensity is 2g/a. Shew that the path
of the particle will be such that if the cylinder be developed
it will develope into successive portions of a parabola.
23. A smooth surface is generated by the revolution of
the curve z*y=c® about the axis of y which is vertically
downwards, and a heavy particle is projected along the sur-
face with velocity due to the depth below the horizontal
plane through the origin: prove that its path intersects all
the meridians at a constant angle.
24, A surface of revolution is such that if it be held with
its axis vertical, and a heavy particle be projected along it
with suitable velocity at any point in any direction, its path
will cut every meridian of the surface at a constant angle.
Shew that the surface may be generated by the revolution
round the axis of y of the curve
h (a? — a”) + ay =0.
202 EXAMPLES,
25. A parabolic wire, axis vertical and vertex downwards,
rotates about its axis with uniform angular velocity. A ring
slides down it under gravity ; prove that it may descend with
constant velocity.
26. A heavy string of given length is enclosed in a
smooth straight tube, which is made to revolve uniformly
about a vertical axis, so as to describe a right circular cone;
determine the motion of the string and the tension at any point.
27. A surface is of the form traced out by the revolution
of the curve z=ccosa/c about the axis of z: the surface
being placed with its axis vertical, a particle is projected
upon it in such a manner that it describes a horizontal circle
in a given time ¢. Prove that the number of possible circles
is even, except in that case in which the time of revolution
satisfies the equation
gt a
1+ dete * ©°8 J (Se 1) = 0.
28. A heavy particle moves on a curve which revolves
uniformly about a vertical axis; prove that the time of an
oscillation of the particle about a position of relative equi-
librium will be
Qa psina \
@ (=n aeate ;
p being the radius of curvature at the point of equilibrium,
a the angle made by the normal at that point with the
vertical, & the distance of the point from the axis of revolu-
tion, and w the angular velocity of the curve.
29. An anchor ring is formed by the revolution of a
circle of radius (c) about an axis in its own plane, distant (a)
from the centre of the circle. A particle is projected along
the equator, of smaller radius with velocity (v), and is acted
on by a centre of attractive force in the centre of the axis,
and equal at distance r to ur"; shew that if the particle be
slightly displaced it will continue to return to its original
path at equal angular intervals (9), where
GaSe
EXAMPLES. 203
30. c
2
where ¢ is their initial distance apart.
3. Two bodies, the masses of which are m and m’, are
projected from the points A, B, and attract each other
according to the Newtonian law. The body m is projected
from A in the direction BA with a velocity i oa and
m’ is projected from B in a direction BP with a velocity
2 / ttm cos PBA;
determine completely the path of either with regard to the
other.
4. The co-ordinates (a, y), (a, y,), of the simultaneous
positions of two equal particles are given by the equations
x=a0 —2asin 6, wx, =a,
y=a—acos 8, ¥,=—-a+acos6;
prove that, if they move under their mutual attractions,
the law of force will be that of the inverse fifth power of the
distance.
EXAMPLES, 227
5. Two particles move under the action of their mutual
attractions, one of them being constrained to remain on a
fixed smooth wire in the form of a plane curve: if the path
of the other be an involute to this curve and the two particles
be always at corresponding points, the curve has for its
intrinsic equation
m2
S=ae 2,
where ™m is the ratio of the masses of the particles.
6. Two equal bodies attract each other with a force
varying inversely as the fifth power of the distance, and they
are projected with equal velocities, in opposite directions, at
right angles to the line joining them; prove that there are
two velocities, in the ratio of 1 : /2, for each of which the
relative orbits will be circles.
7. Two masses m, m’ are connected by an inextensible
string of length a. The extremity A to which m is attached
is compelled to move with uniform acceleration in a straight
line under the action of a force P in the straight line, and the
extremity B to which m’ is attached, is compelled to describe
a circle round A with uniform angular velocity » under the
action of a force @ perpendicular to AB, Find P and Q, and
prove that the least value of Pis
m'arw*
mf — 47 provided aw’ be < 2f.
8. Two smooth circular rings (of radius a) are placed in
a vertical plane with their centres in the same horizontal
line at a distance 3a. Two equal beads (of mass m) slide on
these rings and are connected by a thin elastic string, of
which the natural length is 3a and modulus of elasticity
3amg. They are held as far apart as possible and then let go.
Find when they come to rest.
In the particular case in which 7 =1, find the whole time
of the motion.
9. Two equal particles can move on a fixed smooth
circular wire and attract each other with a force varying as
15—2
228 EXAMPLES.
the distance between them. Prove that their centre of
gravity moves with uniform angular velocity, and that the
relative motion of one with respect to the other is the same
as the motion of a simple pendulum.
10. Two beads of equal mass repelling one another with
a force varying inversely as the square of the distance are
free to slide on a parabolic wire. If they are initially at the
extremities of the latus rectum, prove that if properly
projected the line joining them will always pass through the
focus of the parabola.
11. The attraction between two equal particles, each of
mass m, is wm?/r*, when r is the distance between them, and
they are projected with equal velocities on the same side of
the line (c) joining them in directions not parallel but
equally inclined to that line; prove that the path of each
will be an ellipse, parabola, or hyperbola, according as the
initial component of each velocity in direction of the line ¢
is less than, equal to, or greater than /2um/c’*.
12. Two small rings, each of mass m, which attract each
other with the force mw* x distance, are placed on smooth
wires Ox, Oy, inclined to each other at a given angle, which
commence to move in their own plane with angular velocity
w, and continue to move uniformly. Determine the motion
of the rings.
CHAPTER XII.
ENERGY AND MOMENTUM.
177. It is intended in this Chapter to illustrate the use
of the principles of momentum and energy which were laid
down in Articles (40), (48) and (48) of Chapter IV.
In many cases problems of motion are very rapidly and
easily solved by the aid of these principles, and in all the
cases to which they are wholly or partially applicable, the
problem of determining the motion of a body or a system is
reduced to the solution of equations containing differential
coefficients of the first order, or simple time-fluxes of the
co-ordinates of the system.
178. Motion of two spheres which attract each other
according to the law of nature, of given masses m and m', and
given radii a and a’, placed originally without kinetic energy
with their centres at a gwen distance c from each other.
Supposing that the configuration of zero potential energy
is when the spheres are in contact the potential energy of
the initial configuration, which is the work done in separating
the spheres,
& mm mma mn’
mf? dean SO
ata 7 a+a c
During the subsequent motion let u and w’ be the
velocities of the two balls when their centres are at a
distance r from each other.
230 PENDULUM.
The principles of momentum and energy give the two
equations,
mu =m'w,
' ’ ’ ,
; i mm’ mm mm mm
mu mur + Sea a wee
gmu +3 ata r ata’ c’
Dp ed
or 3 (mu? + mu”) = mm ( = 5) ;
from which u and u’ are at once determined in terms of the
distance.
179. Motion of a simple pendulum.
If a simple pendulum of length / start from the inclination
a to the vertical, the work done by gravity as the pendulum
falls to the inclination 0 is mg (J cos @ —J cosa), and the kinetic
energy is 4ml’60?,
Equating these we find that
P= 7 (cos @— cosa),
a. ft 1
dd V' 29 (Joos 8 = cos a”
If « is very small, this is approximately
dt fi 1
d~N 9 Tea
from which we obtain 6 =a cos eS ¢ tas in Art, (126).
and
180. Motion of two equal heavy particles, fastened to the
ends of a rod without weight, and oscillating in a vertical
plane inside a smooth sphere.
Taking a for the radius and 2c for the length of the rod,
the equation of energy is
2 {4ma?6"} = 2mg ./a* —c? (cos 0 — cos a),
PENDULUM. 231
6 being the inclination of the rod to the horizon,
: 2 —
or P= anes (cos 8 — cos a).
Comparing this with the first equation of the last article
we see that the length of the equivalent simple pendulum
is
e+ /a—c.
‘181. Motion of a compound pendulum, that is, of any
rigid body, or connected system of bodies, about a fixed
horizontal amis.
G being the centre of gravity of the system and GO its
distance from the axis, let @ be the inclination of GO to the
vertical at any time during the motion.
If P be the position of a particle mass m of the system,
and if OP =r, the kinetic energy of the particle m.is $mr’6”’,
for the angular velocity of OP is the same as that of OG.
Hence the equation of energy gives
> (mr°6") = Mga (cos 6 — cosa),
if OG =a, and M= the total mass.
The expression = (mr’) is called the moment of inertia of
the system about the axis, and is generally represented by the
expression Mk’, so that .
C= = (cos 0 — cosa).
Comparing this with the first equation of Art. (179), we
see that the length of the equivalent pendulum is k’~a, so
that if J be the length,
la = k’.
The point in OG at the distance J from O is called the
centre of oscillation of the system, the point O being the
centre of suspension.
232 MOMENTS OF INERTIA.
182. The evaluation of the expression & (mr’) for
particular cases is an exercise in the Integral Calculus.
In the performance of the calculation two facts are of
great utility; these are
(1) That the moment of inertia of a rigid body about any
axis is equal to the moment of inertia about a parallel axis
through the centre of gravity together with the product of the
mass by the square of the distance between those. parallel
axes;
(2) That the moment of inertia of a plane lamina about
any axis perpendicular to the plane is equal to the sum of the
moments of inertia about any two axes in the plane, per-
pendicular to each other, drawn through the foot of the axis.
For the first let r’ be the distance of any particle from the
axis, aud r its distance from the parallel axis through G.
Then if h be the distance between the axes,
= (mr) = Xam (r° + 1? — 2hr cos 6) = & (mr*) + Mh.
For the second, if x and y be the distances of any particle
of the lamina from the axes in a plane
= (mr?) = Dm (a? + y?) == (ma®) + & (my’).
For convenience afew simple results may be stated, taking
in all cases Mas the mass of the body, and Mk’ as representing
the moment of inertia.
For a straight rod of length / about an axis through one
end perpendicular to the rod, k*= 41’; and hence, if the axis
pass through the middle point, k? = 7°.
For a circular ring, about the line through its centre
perpendicular toits plane, k?’=7°. For acircular lamina about
the line through its centre perpendicular to its plane k’ = 47”.
For a parallelopiped of edges a, b, c, about the edge c,
KP =4 (a? +0’).
MOMENTA. 233
For an elliptic area about the transverse and conjugate
axes, kK? = 40°, and k’ = 4a’,
and about the line through its centre perpendicular to its plane
(k? = 4a? + 0°).
For a sphere about a diameter, k? = 2r”,
For a solid ellipsoid about the axis c,
M=1(@' +0’).
183. Hzpressions for linear and angular momenta.
Considering motion in one plane, if « and y be the
co-ordinates of a particle m of the system, the linear
momenta parallel to the axes, are &(m#) and > (my), or, if &, 7
be the co-ordinates of the centre of gravity, ME and M7.
The moments about the origin of the momenta md and my
being — méy and my#, the angular momentum of the system
is
Xm (ay — ye).
In polar co-ordinates mr6 is the part of the momentum
perpendicular to the radius vector, and therefore the angular
momentum is ;
= (mr’é).
If A be the area swept over by the radius vector,
2A = ay — ye = 7°,
so that the angular momentum is
22mA.
Again, if p be the perpendicular on the tangent to the
path of the particle m, the angular momentum of the system is
S (mip),
and, since = pds = r°d0, and p= a -y = ;
this expression at once transforms itself into either of those
preceding.
234 MOMENTA.
In the case of a single rigid body, revolving about an axis
with which it is rigidly oanncaton. 6 is the same for all the
particles, and the angular momentum is
Mk, or Mito.
184, For motion in three dimensions the expressions for
the linear and angular momenta are
% (ma), & (my), 2 (mé),
im (ys — 2y), Sn (2 — #2), Um (ay — ye).
If we take £, y, € as the co-ordinates of the centre of
gravity, and a, y, z as the co-ordinates, relative to G, of a
particle m, the angular momentum about the axis of z
= {m (E+2) (+9) —(9+y) (E+ 4)},
= M (£4 — nf) + Em (ap — ya),
since = (ma) = 0, and & (my) =
Hence it follows that the angular momentum of a system,
about any assigned axis, is the sum of the angular momentum
due to the motion of the particles of the system relative’ to
the parallel axis through the centre of gravity, and of the
angular momentum due to the mass of the system supposed
to be concentrated at, and moving with, the centre of
gravity.
It may be instructive to present the proof of this state-
ment in another form.
Let O and G be the projections of the assigned axis and of
the centre of gravity on a plane perpendicular to the axis,
GA the projection of the line of motion of G, and FK the
projection of the line: of motion of a particle.
Taking m as the mass of the particle and wu as the
component in the line FK of its velocity, and taking EG
parallel to FK, j
The angular momentum about the axis O
== (mu. OF) = (mu.O£) + % (mu. GK).
MOMENTA. 235
If & be the velocity of G in the direction GA, the first
term, which is the sum of the moments about O of a number
of momenta in lines through G, is equal to the moment of
their resultant, and therefore
= Mu. ON.
een
The second term
= % {m(u— cos 6) GK} + a (mGK cos 8).
But = (mGK cos 0) => (m. KL) =0,
and therefore the second term represents the angular mo-
mentum ‘due to the motion of the particles of the system
relative to the centre of gravity.
185. In the case of a single rigid body, when the motion
is entirely in two dimensions, an expression for the angular
momentum is
Mp'd + Mio,
if p and ¢ be the co-ordinates of the centre of gravity.
Take, for instance, the case of a number of rigid bodies,
rotating about the sume fied axis with given angular velocities,
and becoming suddenly, or gradually, connected together.
236 ENERGY.
In this case the total angular momentum is unchanged,
and therefore, if mk’w be the original angular momentum of
one of the bodies, and © the final angular velocity of the
system,
2.3 (mk*) = & (mk'o).
186. Expressions for kinetic energy.
For motion in two dimensions, the expression in rect-
angular co-ordinates is
2m (4° +9’),
and in polar co-ordinates,
43m (7? + 7°68).
For the case of a rigid body in motion about a fixed axis,
the kinetic energy is
£3 (mr°6") or LMBO.
For motion in three dimensions the expression for the
kinetic energy in rectangular co-ordinates, is
fim (#@ +742);
in cylindrical co-ordinates,
435m (7? + 7°@ + 2);
and in polar co-ordinates,
42m (? + °F + 7° sin? 06°).
_ Other modes of expression can also be given and will be
employed when necessary.
If 2, y, z be co-ordinates relative to the centre of gravity
the kinetic energy
=h.2{m(E+ar tty? + (b+,
= 4M (49+ 0) +42m (+7 +2).
So that the kinetic energy is the sum of the energy due to a
mass M at the centre of gravity and of the energy due to the
motions of the particles of the system relative to the centre
of gravity.
ENERGY. 237
187. In all cases in which no external forces are in
action the linear momenta and the angular momenta remain
constant.
The principle of the conservation of energy of a mechanical
system, that is to say, the assertion that the sum of the
potential and of the visible kinetic energies is constant,
applies to all those cases in which the potential energy
depends on the configuration of the system, and in which
the change of potential energy, due to a change of con-
figuration, is independent of the manner in which that
change is made.
There is no doubt that, in any system, the total energy
remains unchanged, unless extraneous force act on the
system, but, as in the case of impacts taking place between
bodies of the system, there may be an apparent loss of kinetic
energy, which is fully accounted for by the development of
invisible kinetic energy in the form of heat, or in some other
form.
Or again, kinetic energy may be created by explosions,
but in this case, the visible kinetic energy, together with the
heat added to the system, are the equivalent of the potential
energy which was lying dormant in the explosive matter
while in its quiescent condition.
Internal friction, if due to the sliding of two surfaces on
each other, is destructive of visible kinetic energy, while, on
the other hand, visible kinetic energy may be created by the
action of live things, as for instance in the case of a man
walking on a rough plank, or a rough ball, or climbing a
moveable rope.
In such cases the system is said to be not dynamically
conservative, although it is really conservative rf all the
transformations of energy be taken into the account.
* 188. If an elastic string form part of a system, the gain
of potential energy due to its extension from its natural
length is
4 (Tension) (Extension) ;
238 ENERGY.
for the work done in pulling out the string
° TH, x -
=] Tax = | * (@-1) de=y* (rl)
u U
as may also be shewn by a simple geometrical figure. In
such a case the contraction or extension of the string implies
a transformation of energy, the loss, or gain, of potential
energy due to the contraction or extension, being represented
by a change in either, or both, of the kinetic energy, and of
the potential energy due to configuration, irrespective of the
string.
nergy imparted to a system by the action of an extraneous
couple.
Any state of motion of a plane can be represented by a
state of rotation about an instantaneous centre in the plane,
IP
If a small displacement, 56, be made round the in-
stantaneous centre H, the work done by the force of the
couple
=P. EBs$¢—P.EAi$=P . ABSh= Gd,
G being the moment of the couple.
Hence, if @ be the total angular twist of the couple, the
work done
*
0
= i: Gdd = GO, if G be constant.
We now proceed to illustrate these general statements by
their applications to some particular cases,
ENERGY. 239
189. Motion of a heavy rod placed with its lower end in
contact with a smooth horizontal plane, and let go.
If a be the initial inclination to the vertical, and @ at any
subsequent time, the work done by gravity is
mg a (cos a — cos 8),
and the kinetic energy is
4m (7 +k6), where y = a.cos 6.
Hence we obtain
2
= (sin’6 + 4) 6’ = ag (cos a — cos @),
4. 6g cosa — cos 8
2 —_— —“ sacs: noma
- os 3sin’?A+1 °
190. Motion of a heavy rod, constrained to slide in a
vertical line, with its lower end on the curved surface of a
smooth hemisphere, the hemisphere sliding on a smooth hori-
zontal plane.
If @ be the inclination to the vertical of the radius to the
point of contact, and a its initial value, the work done by
gravity is mga (cosa —cos@),m being the mass of the rod.
If M be the mass of the hemisphere the kinetic energy of the
‘ system is
on eee eee ce sin 6),
7 ) (G4 :
and therefore
(m sin6 + M cos*6) @ = a (cos a — cos 8).
191. Motion of a heterogeneous sphere rocking on a rough
horizontal plane, the whole motion being parallel to one vertical
plane.
Taking O as the point of contact of the end of the radius
CG through G when it is vertical, x, y, as the co-ordinates
of G, CG =e, and the radius = a, the equation of energy is
dm {a + 9° + k°6} = mge (cos 0 — cos a),
where xz=a0—csin @, and y=a—ccos@;
@ {a? +c? — 2ac cos 6 + k?} = 2gc (cos @ — cosa).
240 ENERGY AND MOMENTUM.
192. Motion of two equal rods, AB, BC, jointed at B and
moving, on a smooth horizontal plane, about the fixed point A.
In this case the angular momentum about A and the
kinetic energy are both constant.
Taking 6 and ¢ as the inclinations to a fixed line on the
plane, the velocity of the centre of gravity, G, of BC is com-
pounded of its velocity relative to B,
that is, ag perpendicular to BC, and of the velocity of B,
which is 2a6 perpendicular to AB;
4a?
a
m a6 + mad {a + 2a cos ( — 6)} + m2a8 {2a + a cos (b — 6)};
hence the equation of momentum is
6 (48. + 2 cos h — 6) +(£+2cos $—6) = 0.
Again, the square of the velocity of G
=a? + 40°6" + 40°66 cos 6 — 0,
the angular momentum of ABis m — 6, and that of BC is
2
the kinetic energy of AB is m me
— j2
3 Be
2
and that of BC due to rotation is ms ¢? :
ENERGY AND MOMENTUM. 241
.. the equation of energy is
18 P+4¢4' +4466 cos p—0 =C",
C and C’ being constants given by the initial conditions.
These two equations determine 6 and ¢.
193. If a solid body is rotating about a fixed axis, and
is changing its shape and size, without the action of any
external force, its angular momentum remains constant, and
this determines the change of angular velocity.
If for instance a sphere rotate about a fixed diameter,
changing its size, but retaining its shape and its homogeneity,
the angular momentum, which is 2 Mr*w, remains constant.
If the radius change to 7’, the change in the kinetic
energy is
2
£M (ro —1o*) or $M (FP — 7) of
194. Motion of a heavy rod swinging about its upper
extremity which is freely jointed to a fimed support.
If 6 be the inclination of the rod to the vertical, and ¢ its
azimuthal velocity, the angular momentum about the vertical
through the fixed end and the energy are respectively,
& (mr? sin’ . 6}
and = 4S {mr + mr*sin’O . "| + Mg (a— aco 8),
if we assume that the configuration for zero energy is when the
rod is vertical and at rest.
Each of these expressions being constant, we obtain for
the determination of @ and ¢ the equations,
¢ sin’é = O sin’a,
2 a (& + g* sin’O) + g (1 — cos 6)
= 2a(o + 0’ sin’a) +9 (1 — cos a),
w and Q. being the initial values of 6 and ¢.
B.D. 16
242 ENERGY AND MOMENTUM.
Eliminating ¢ and taking the time-flux of the resulting
equation, we obtain
4a0 — 4a.0? sin‘ a cosec’@ cot 6 + 3g sin 8 = 0.
The condition that the rod may revolve uniformly, so as
to describe a right circular cone of vertical angle 22, is
4aQ7cos a = 3g.
If while thus revolving the rod receive a slight displace-
ment, not disturbing this relation, the small vibrations in 0
will be determined by putting 6=a +, when w is small in
the above equation.
The result is the approximate equation,
‘ 4a cos ap + 8g (1438 cos *a) fp =0,
so that the period of the oscillation is
4er,/a, cos a / 4/3g (1 + 3 cosa).
195. Motion of a heavy horizontal ring, fitting on a
smooth vertical cylinder, and supported by a number of verti-
cal strings fastened to its upper edge.
If the ring, when in equilibrium, be started with a given
angular velocity w, it will rise until the potential energy.
stored up by the elevation is equal to the original kinetic
energy, that is to a height A such that ,
mgh =4 maw’,
a being the radius.
As the ring rises the strings will form helices on the
surface of the cylinder, and, taking / for the length of each
string, and @ the angle through which the ring turns in
rising through the height z, we have the geometrical.
equation
P =(l—z)? + 0°6, and .*, a°06 = (1-2) 2.
The equation of energy is
£m (# + a6") = } ma’a* — mgz,
and these equations give 6 and 2 in terms of z.
ENERGY AND MOMENTUM. 243
If, instead of starting the ring with an angular velocity,
it be set in motion by a horizontal couple G, twisted through
an angle @, the energy imparted to the system is GB.
Part of this energy appears in the form of a change of
potential energy due to change of configuration, and its
amount is
mg {l— J? — a6".
The difference, G8 — mg {l—./l* — a®B}, is represented by
the kinetic energy with which the ring starts off in its new
configuration.
196. If a heavy elastic ring, in the form of a horizontal
circle, be placed on the surface of a smooth sphere and allowed
to slip down, we can determine the motion by observing that
the kinetic energy is increased by the fall, and diminished
by the extension of the rings If a be the radius of the
sphere, 27rasina the initial length of the ring, and @ be
the angular distance of each point of the ring from the
vertex at any subsequent time, the equation of energy is
ae ro _X (sin 8 — sina)
4ma’é? = mga (cos a — cos 6) 5° 27a ee
The condition that the string should just slip over the
sphere is that
Tv
6=0 when Gas:
which gives mg sinacosa=) (1 —sina)’.
197. A circular wire ring of mass M, carrying a small
bead of mass m, lies on a smooth horizontal table, and is
capable of turning about a fixed point in its circumference.
An elastic thread the natural length of which 1s less than
the diameter of the ring has one end fastened to the bead
and the other end to the fixed point. It 1s required to
determine the motion when the initial position of the thread
coincides very nearly with the diameter of the ring,
16—2
244 ENERGY AND MOMENTUM.
The angular momentum is always zero, so that if OP the
thread be inclined at an angle ¢ to the initial position of the
diameter OA, ;
M .2a°0 = mr'd,
where r = 2a cos (p + 6).
P
Again the equation of energy is
M206" + m (i# + 096%) = ¥ (Ba — 0? — (r — 1),
and these equations theoretically determine 6 and ¢.
When the string contracts to its natural length the kinetic
energy retains a constant value until by the motion of the
bead the string is again put into a state of tension.
198. If an elastic thread, in the form of a circle on a
smooth horizontal plane, be set rotating with a given angular
velocity, the principles of angular momentum and energy give
the equations }
mr? = maa,
dm (77? +7°6) = dmato® — = (r — a)’;
and those equations determine # and 6 in terms of r.
ENERGY AND MOMENTUM. 245
199. Motion of a wire ring on a smooth horizontal plane
produced by an insect alighting upon it and moving uniformly
round the are of the ring.
As the insect starts with a finite motion there must be an
impulsive-action, that is, of the nature of a kick, between the
insect and the ring in direction of the tangent.
Take M, m, as the masses and w as the velocity of the
insect relative to the ring.
If V, uv be the actual initial velocities, in contrary directions,
of the centre of the ring and of the insect,
MV=mv.
If be the initial angular velocity of the ring, we have
the geometrical condition,
V+ao+v=u.
Again the angular momentum about any vertical line is
equal to zero.
Taking the angular momentum about the vertical line
through the initial position of the centre of the ring,
Me’o = mua,
and these equations determine V, » and v.
During the subsequent motion, G remains at rest, and
the angular momentum about G is zero, so that if ¢ and @ be
246 ENERGY AND MOMENTUM.
the angles turned through by the ring and the radius to the
insect, ; ;
mPG’6 + MCG"6 — Ma’d =0,
or mO =(M+m)d.
This equation, and the geometrical condition, a (6 + é) =u,
determine @ and @..
200. Aremarkable application of the principle of energy
has been made by Professor C. Niven in discussing the
motion produced when a heavy elastic string, suspended
from one end, is cut at-any point*.
To illustrate this application we take a simple case, in
which the action of gravity has no effect.
An elastic string has one end fastened to a fixed point on a
smooth horizontal plane, and the other end is drawn out to
any assigned distance, and is then let go; it is required to
determine the subsequent motion.
Taking a as the natural length and 7 as the stretched
length of the string, the tension 7’ is ) (J—a)/a, and if dx be
the natural length of an element at the end of the string, its
potential energy, before the end is let go, which is half
tension x extension,
T° t—a\?
=45- de=3.0(=*) dx.
When the end is let go, this energy is set free, and is
immediately converted into kinetic energy.
Taking m as the mass of unit’ length, and V as the
instantaneous velocity of the end of the string, the kinetic
energy is 4mdzV”, and therefore,
ry oe
mr ma
The first element being started with this velocity the
next element will be under the same initial conditions, and
* On a case of Wave motion, by Professor C. Niven, Messenger of
Mathematics, Vol. VIII.
ENERGY AND MOMENTUM. 247
will acquire the same velocity, and all the elements in
succession will acquire the same velocity, so that a wave
like motion will be propagated from the free end to the
fixed end of the string.
To find the velocity of transmission of the wave, we
observe that when the wave is passing over the element PQ,
A Pg B
the tension at P is 7 and the tension at Q is zero, and
Coo in the time dé the momentum generated in PQ ‘is
dt.
But this momentum is mdz. V, and therefore
sam =s/%
so that the velocity of transmission is constant with regard
to the natural length.
Hence the time in which the wave travels from B to
A=al/ m/JX, and in this time the free end B will have:
traversed the space Vax/m/,/X which is equal to J—a.
It follows therefore that, when the wave reaches A, the
string is In its unstretched condition, and every element has
the same velocity V in the direction "BA,
If we assume that Hook’s Law holds for compression as
well as for dilatation, the kinetic energy will be gradually
converted into the potential energy of compression, which
will in its turn be reconverted into the original kinetic
energy.
If Hook’s law does not hold for compression or if the
string is so constituted that it is reduced to rest on arriving
at its natural condition, the kinetic energy, which is ap-
parently lost, is really converted into heat.
201. We can explain from first principles why it is that
the release of the end of the string instantaneously repulis 4 in
the production of a finite velocity at that end.
248 EXAMPLES.
Considering a small element at the end B, at the moment
of release, the force on the element is 7’ and its mass is mda,
so that we have a finite force acting on an infinitesimal
mass.
Now if, by means of a mental microscope, we imagine
the mass magnified so as to become a finite mass, and the
force T magnified in the same proportion, we shall have the
case of a very large force acting upon a finite mass, the result
of which is, as we know, the production of a finite velocity in
a very small time, and the smaller we take the element at
the end B, the more closely do we tend to the ultimate
form, which is the instantaneous production of velocity at
the end.
EXAMPLES.
1. A heavy particle slides down a chord of a vertical
circle to the lowest point of the circle, and then ascends the
curve; prove that in no case can it rise through more than
one-sixth of the total are.
2. A and B are two pegs very near together and in the
same horizontal line. A perfectly flexible string of length
Lis fastened at A and hangs over B, the portion between A
and B hanging down; the loose end begins to descend from
the position of equilibrium: prove that the final velocity of
the string is ,/291/3.
3. If a system of bodies initially at rest be acted on by
no forces but the attractions of its several parts, and at any
subsequent time become united as a single solid body, shew
that this body will be at rest.
4, A particle is attached to a smooth string which passes
over a rough circular arc in a vertical plane; the particle,
initially at the end of a horizontal diameter, is drawn up
with constant acceleration g/m; prove that the work expended
in drawing it to the vertex of the circle is to the work which
would be done in lifting it through the same height in the
ratio 6+44—mp : 4.
t
EXAMPLES. 249
5. The two ends of a homogeneous rod are moveable on
the arc of a fixed smooth conic, having its axis vertical and
vertex downwards; if the length of the rod be greater than
the latus-rectum, and if it be placed in a horizontal position
and slightly displaced, find the greatest kinetic energy which
it acquires.
6. A small heavy ring, moveable on a smooth circular
wire fixed in a vertical plane, is attached by an elastic string
without weight to a point at a distance below the lowest
point of the circle equal to its radius, and when the ring is at
the lowest point of the circle the string is unstretched. If
the ring be drawn along the wire till the string becomes a
tangent to the circle and then let go, determine the velocity
with which it will reach the lowest point of the circle.
7. (me),
and the angular momenta, about these axes, are
2m (yz— zy), Lm (ze — 22), Lm (ay — ya).
Hence it follows that the mathematical forms of the
statements (1) and (2) are as follows, .
(1) ¥ (mi) =X, (mj) = Y, 3 (mi) =Z,
(2) Sm(yz—2i) =L, Sm(2# — 22) =M, Sm (xy — ye) =N.
Or these equations can be obtained, as in Art. 53, from
the principle, Art. 46, that the system of the time-fluxes of
momenta of the several particles of a system is the exact
equivalent of the system of acting forces, and therefore that
the sums of the components of the one system and their
moments about the axes are the same as those of the other
system.
17—2
260 - EQUATIONS OF MOTION.
Tn the case in which impulses are applied to a system,
the mathematical forms of the statements (3) and (4) are
(3) Sm(u'—u)=P, Sm(v'-v)=Q, Ym (w’—w) =R,
(4) Sm fy (w’—w) —2(o'-v } = G,
im {z(w’ —u) —a (w’—w)} =H,
Sin {ee (o' —0) —y(w'—w) =K,
where P, Q, R, are the sums of the applied impulses in
directions of the axes, and G, H, K the moments about the
axes of those impulses,
205. Independence of the motions of the centre af gravity
and of the system relative to the centre of gravity.
If & 7, € be the coordinates of G, the centre of gravity,
the equations (1) become
EX (m)=X, 2 (m)=Y, $3 (m)=Z,
shewing that the motion of G is the same as if the whole
mass were concentrated into a particle at that point, with
all the extraneous forces acting upon it.
Again, if we take a, y, 2 as the coordinates, relative to the
centre of gravity, of a particle m of the system, its accelera-
tions are #+ & +4, 2+ and, if L, M, N’ be the moments
about the axes through G, of the acting forces, the equations
(2) are replaced by
Xm {y (2+ 6) —2(9 + %)} =L, &e,
or, since & (my) = 0, and & (mz) = 0,
Sm (yz— 27) = L, &e.,
shewing that the motion relative to the centre of gravity is
independent of the motion of the centre of gravity itself.
206. In the case of impulses being applied to the
system, if the velocities of the centre of gravity change from
a, 6, c to a’, b,c’, the equations (3) become
M(a'—a)=P, M(B -b)=Q, M('-c)=R,
If being the mass of the whole system.
MAN ON SPHERE. 261
Again, taking the instantaneous position of the centre of
gravity as the origin, and taking u, v, w as the velocities of
m relative to the centre of gravity, so that the actual
velocities of m-are u+a,uv+b, w+c, the first of the equations
(4) becomes
Sm {y (w' + —w—e)—2(v +b'-v —b)} = &,
os Sn {y (w' —w) —2 (v' — 0)} = G.
These results shew that the changes of motion of the
centre of gravity, and the changes of angular momentum
about axes through the centre of gravity, due to impulsive
actions, are independent of each other.
207. To illustrate at once the use of these principles,
consider the case of
A man walking on a large rough sphere, so as to make
the sphere roll in a straight line on a horizontal plane, the
man keeping himself at a constant angular distance (a) from
the highest point of the sphere.
Take M, m as the masses of the sphere and the man, and
let w be the angular velocity of the sphere at any instant.
The velocity of the man is aw parallel to the plane, and
the time-flux of his momentum is therefore maw.
For the sphere the time-fluxes of the linear momentum,
and of the angular momentum about the centre of gravity
are
Mae and M20’,
Hence taking moments about the horizontal axis, perpen-
dicular to the motion, through the point of contact, we
obtain
Mo’ + M20’ + mash = mga sin a,
or ® (7Ma + 5mh) = 5mg sin a,
where h is the constant height, above the plane, of the centre
of gravity of the man.
We may also solve this problem by finding the rate of
change of the angular momentum, at any time, about the
262 MAN ON SPHERE,
axis fixed in space which passes through the point of contact
at that time.
To do this we observe that, at any time, the angular
momentum of the system about the point of contact is equal
to
£ Mao + mah.
After the lapse of an interval 6¢ of time, the angular
velocity is » + dw, and the linear velocity of the centre of the
sphere and of the man is a (w+ do).
Observing that the distances from the assigned axis of
the lines of acceleration of the centres are the same as at the
time t, the angular momentum at the time ¢ + 6¢ is
Ma? (w + 8) + 2Ma? (w + 8) + ma (w+ bw) h,
and the rate of change is therefore
2Ma’o + maho,
which is equal to the moment mga sin a of the acting forces.
If the reactions and frictions be required, we observe that
the time-fluxes of the linear momenta of the sphere and the
man are
Mae and mas,
so that, if 2” be the friction between the sphere and plane,
and R, F the reaction and friction between the man and the
sphere,
Mao + mao =F’
maw = Rsina— F cosa
0=Reosa+Fsina—mg,
and these equations determine F, F” and R.
208. This system is not, from a purely mechanical point
of view, a conservative system.
The work done by friction upon the sphere is not equal
and opposite to the work done by friction upon the man, and
the energy of motion at any time is due to the difference
between the amounts of work done upon the two bodies.
Thus if the figure represent two consecutive positions,
P being the point of contact, the horizontal distance
MAN ON SPHERE, 263
PP'= 86, and if P’C'Q=80, the point P of the sphere is
carried to Q.
L\Q
Cc’
Hence, if P’L, QN be perpendiculars on the tangent at P,
the work done by friction upon the sphere is /’. PN, and the
work done upon the man is f’.(—PL). The sum of these
=F. LN = Fa8é, and the work done upon the system
z | Fad6.
But, the acceleration of the man in the direction of the
tangent at P being a® cos a, it follows that
Mae cosa = mg sina — F,
and therefore the work done
= | (mga sin a —ma’o cos a) dé.
This is transformed into energy of motion, or kinetic
energy, the measure of which is
$M.2a’o’ +4 ma’o’.
Equating these two expressions, we find that
ta’o ($M+m+mcosa) =mgasina. 8,
and, taking the time-fluxes of each side of this equation, we
obtain the same equation for @ as before.
The fact that kinetic energy is produced and increased is
264 CHAIN ON PULLEY.
a proof that potential energy is being lost somewhere. The
explanation is that the man’s power of exerting himself is
diminishing; he is getting tired, or, in other words, the man
is a machine which has acquired potential energy by being
wound up, and is running down.
209. A heavy chain passes over a rough pulley, moveable
about a horizontal axis through its centre, and the portions:
hanging down, which are of different lengths, are coiled up and
held close to the ends of the horizontal diameter ; if both coils
be let go at the same instant what ts the subsequent motion ?
The coils will fall freely, each leaving behind a straightened
portion, and, at the time ¢, each will have fallen through the
space 4gt’.
Take a for the radius of the pulley, b and ¢ for the lengths
of the portions coiled up, b being greater than c. Then if 0
be the turn of the pulley in the time ¢, the lengths 0’, ¢’ of
the pieces in the coils at that time will be
b— (4gt? — a6) and c — (49? + a6).
The velocity of each point of the straight pieces and of
the portion in contact with the pulley will be a6, and the
velocity of each coil will be gt.
Let Mk’ be the moment of inertia of the pulley, m the
mass of the whole chain, and J its length, so that
l=b+c+ 7a.
Then the angular momentum of the system will be
Mi6+™ (g# + ma) a+ gta — ne a,
or Mio + 7 (g@? + a) a6 + mgt —c+2a8).
Taking the time-flux of this expression and equating it
to the moment of the acting forces which is
mb’ _ me’
ge
or mI" (b —¢ +206),
i
SLIDING ROD. 265
we obtain the equation
2 oe 2. =
{ue 4 (ot +a) 8 4. mga bp x0),
from which, by integration and the introduction of initial
conditions, 6 can be determined.
210. Motion of a heavy rod sliding between a smooth
vertical plane and a smooth horizontal plane in a vertical
plane perpendicular to both.
The angular velocity in any position is at once deter-
mined by the principle of energy, but the question is intro-
duced for the sake of further illustrating the meaning of the
phrase angular momentum. ° ;
|
oo
2
of
oe
-
oer
If AB be the rod, and # the instantaneous centre of the
motion, the velocity of Gis aw, and the angular momentum
about # is ma’o + mk’w, or 4 ma’.
After a time 6¢, the rod having turned through an angle
60, the perpendicular distance from # of the line of motion
of G’ is 2a.cos 89 —a, which to the first order of infinitesimals
is equal to a.
Hence the new anguldr momentum about F is
ma? (w + Sw) + mk? (w + So),
and therefore the rate of change of the angular momentum
about EF is 4ma’# which is equal to mga sin 0;
; y+ 39 . a __ 39 =
G=7 sin 8, and 0 = 9, (cose cos @).
266 FIXED AXIS.
This is one view of the case, and another is to observe
that aw? and aw are the accelerations of G in the direction
GO and perpendicular to it, so that the time-fluxes of
momenta are maw’, maw, and mk’s, and the moments of
these about £ are equal to mgasin 0.
The reactions R, #' in the directions AH, BE are given
by the equations,
R= ¢ (mab cos 6) = ma (6 cos 6 — 6° sin 6),
R—mg=4 (-mad sin 0) =— ma (6 sin 0 + 6° cos 6).
It will be seen from these equations that R’ vanishes and
changes sign when
3 cos 0 = 2 cos a,
shewing that the rod will then leave the vertical plane.
If it should be required to take moments about 0, it will
be seen that the angular momentum is maw — mk’o and
therefore that the equation of motion is
2ma’o = mga sin 6 + R'2a cos 6 — R2a sin 6,
but then the preceding equations must be employed for the
elimination of R and £&’.
211. Motion of a rigid body about a fined axis.
If w be the angular velocity of the body at any instant,
its angular momentum is M (k’ +h’) w, h being the distance,
OG, of the centre of gravity from the axis and Mk’ the
moment of inertia about the line through G parallel to the
axis.
Hence if V be the moment of the acting forces,
M(? +h’) o=N,
or, if @ be the inclination of the plane through G and the
axis to a fixed plane through the axis,
Me +h) O=N.
FIXED AXIS. 267
If r be the distance of a particle m from the axis, its
accelerations in the directions of r and perpendicular to it
are respectively — wr and ra.
Taking the fixed axis as the axis of z and OG as the axis
of x, the components of these parallel to # and y are
— o's — oy and — wy + ox.
Hence the time-fluxes of the momenta and their moments
about the axes are respectively
2m (— wa — ay), Um (— wy + wz), 0,
and Ym (w°yz— wz), Xm (—w'xz— wyz), ZS {me (a? +4},
or, — Mah, Moh, o,
and Dw’ — Eo, — Ew — Do, M (kh? +1’) @,
where D and £ represent the quantities, Smyz, and Ymzz.
The first three of these expressions are equal to the sums
of the acting forces and of the reactionary stresses of the axis,
and the next three are equal to the sums of the moments
about the axes, of the same quantities*.
Suppose that the body is connected with the axis at two
points at distances c and c’ from O, and that U, V, W, and
U’, V', W’ are the stresses upon the axis at these points.
Then, if X, Y, Z, L, M, N be the sums and moments of
the acting forces, we shall have the equations
—~Mo*h=X-U-U’,
Moh=Y-V-—V’,
o=Z—-W-W',
Dow — Es = L — Ve —V'e’,
— Eo? — Da = M+ Uc+ U'e'.
212. Impulses applied to a body in motion about a fixed
ants.
* It will be seen in the next chapter that these expressions can be
also obtained by first writing the expressions for the angular momenta and
then employing the general expressions given in that chapter for the rates
of change of the angular momenta,
268 FIXED AXIS.
If w'—w be the change of angular velocity due to the
application of impulses, and K the moment of the impulses,
the change of angular momentum is given by the equation
UM (i? + h’) (o’ —@) = K.
Taking the axes as in the last article, and observing that
m (#’ —w)r is the change of momentum of the particle m in
the direction perpendicular to r, of which the components
are —m(o'—@)y, and m(w’—) #, we find that the sums
and moments of the changes of momenta are respectively
o, M (w' — w)h, 0,
and —E(#'—w), -—D(w'-—o), UM (k’ +2’) (o’ —@).
Equating these expressions to the sums and moments of
the applied impulses, and of the reactionary stresses, we can
calculate the latter quantities.
The right-hand members of the equations in the preceding
article will be the expressions for the sums and moments, if
the symbols employed be supposed to represent the applied
impulses and the impulsive stresses on the axis at two
points. .
213. We have defined, in Art. 181, the centre of oscilla-
tion of a compound pendulum.
We can shew that the centres of oscillation and suspension
£ and O are convertible.
For OL. OG=04 +2,
whence OG. EG=R,
shewing that O and EF are convertible.
214, Centre of percussion.
If a single impulse can be applied to a rigid body which
is capable of motion about a fixed axis, so as to produce no
impulsive stress on the axis, the line of the impulse is called
the line of percussion, and the point in which it meets the
plane through G perpendicular to the axis is called the
centre of percussion.
‘ILLUSTRATIONS. 269
If w be the angular velocity produced the sums and
moments of the changes of momenta will be
0, Moh, 0, — Ho, — Do, M (kh +h)o;
OG being the axis of 2, and Oz the fixed axis as in Art. 211.
The single impulse P must therefore be in the direction
of the axis of y, and, if &, be the coordinates of the point
in which its line of action meets the plane wy, we must have
— Ew =— Pi, —-Do=0, M(h +2’) w= PE
Hence it follows, as a necessary condition for the existence
of a centre of percussion, that D, or & (myz), must vanish,
and that, if there is a centre of percussion, its distance from
the axis is the same as that of the centre of oscillation.
When £, or & (mz), vanishes, the centres of oscillation
and percussion are coincident.
215. Motion of two heavy rods AB, BC jointed at B, and
swinging in a vertical plane about the end A which 1s jointed
to a fixed horizontal axis. ,
If 6 and ¢ be the inclinations of AB and BC to the
vertical, the angular momentum of the system about A, 2a
and 2b being the lengths of the rods, is
4q? . 9 OG. er
m 3 O+m x > +m'bd {b + 2a cos (6 —4)}
+ m'2a6 {2a +d cos (db — 6)},
and the time-flux of this expression
=— mga sin 0 — m'g (2a sin 6 + bsin @).
Next, the accelerations of G being compounded of bf and
bf? perpendicular and parallel to GB, and of 2a8 and 2a6"
perpendicular and parallel to BA, we obtain by taking
moments about B for the rod BC, and dividing by m’
0b + 5 $+ 2a b cos (p— 6)
+ 2a6°b sin (b — 0) =—gb sin ¢,
or. 4bh + 2a [6 cos (b — 6) + sin ($ — 6)} =—gsing.
270 ILLUSTRATIONS.
Or for a second equation we might have expressed the
constancy of the energy which is
3ma?O? + 4m'd'd? + 5 {B'? + 4a°6? + 4abd6 cos (f — 6)}
— mga cos 6 — mg (2a cos 6 + b cos ¢).
In either case we obtain two equations for the determina-
tion of @ and ¢.
The horizontal and vertical components of the momentum
of the system are respectively
maé cos 0 + m'bd cos ¢ + m’2a8 cos 6,
and ma sin 0 + mb sin b + m’2a0 sin 8,
The time-fiux of the first of these is the horizontal com-
ponent of the stress at A, and the time-flux of the second
increased by the weight of the rods is the vertical com-
ponent.
In the same manner the stress at B is determined by
writing down the horizontal and vertical components of the
momentum of the rod BC.
216. Motion of a heavy sphere, the centre of gravity of
which is eccentric, on a smooth horizontal plane.
If the sphere have no initial kinetic energy, the centre of
gravity G moves in a vertical line GO, and if OG =y, the
equation of moments about C or about any point in the
vertical line CP through the point of contact P is, with the
notation of Art. 189,
mijc sin 0 + mk*6 = — mge sin 8,
where y =a—ccos 6.
Substituting, multiplying by 26 and integrating we obtain
6 (k? +c? sin?0) = C+ 29c cos 6,
which is the equation of energy.
The reaction, &, at P is given by the equation
R- mg = mi.
MOTION OF LAMINA. 271
If the plane be rough so that the sphere Tolls, the equation
of moments about P is
mie + méy + mije sin 0 = — mg.c sin 6,
where 2=a0—csin#, and y=a—ccos6,
making the substitutions and integrating we obtain the result
of Art. 189,
The horizontal and vertical reactions at P are given by
the equations mé=—F, mij= R— mg.
217. Motion of a plane lamina, of any given shape, on a
smooth plane, when a given point of the lamina is made to
move in a given manner, and the lamina is besides acted upon
by known forces.
If A be the given point, and G the centre of inertia of the
lamina, take 0 as the inclination of AG to a fixed line in the
plane, so that 6 is the angular velocity of the lamina.
If f and f’ be the accelerations of the point A in the
direction AG and perpendicular to it, which are known
functions of the position of .A, or of the time, the accelera-
tions of G in the same directions are f— a6’, and f’ +a,
and the time-flux of the angular momentum about G is
MO.
Hence, if V be the moment about A of the acting forces,
M(f' +06) a+ MO =N,
the equation which determines the angular motion of AG.
If P, Q be the requisite constraining stresses at A, and
X, Y the resultant forces, in the direction AG and perpen-
dicular to it,
M(f-a6)=X+P, and M(f’ +a6)=Y+Q.
218. Motion of a plane lamina, bounded by a curve,
rolling on a fiaed curve under the action of given forces.
We have first to solve the kinematical question of the
time-flux of the angular momentum about the point of
contact.
272 “MOTION OF LAMINA.
The angular momentum being the sum of the angular
momenta due to the rotation and the motion of the centre of
gravity, the first part is Mk’w. :
&
Gg’
AY
For the second, taking as the angular velocity when the
point P of the rolling curve is in contact with the point A of
the fixed curve, and @ as the consecutive point of contact, the
angular momentum at A = Mr’a, if
AG=PG =r,
In the consecutive position, when the motion of G' is”
perpendicular to QG’, the angular momentum about A
= M (r+ 6r) (w+ 80) 7,
remembering that AP is an infinitesimal of the second
order, and the difference
= Mr (réo + wor).
Hence the time-flux of the angular momentum due to
the motion of G
= Mr’ + Morr,
MOTION OF LAMINA, 273
and consequently the equation of motion is.
M (+7) 0+ Morr =L,
L being the moment about P of the acting forces.
If p, p' be the radii of curvature at P of the rolling curve
and the fixed curve, and if the are AQ=6s,
oot = as + ae i
pp
and, if @ be the angle between the line AG and the normal
at A,
,
err =— or sin 6s = — wr sin 8 = 3
p
so that the equation of motion takes the form
Mk +9°) @— Mo'r sin 0—PP— = 1.
pt p
If the fixed curve be a straight line
pee,
p
and the equation is then
M (k? +7") a — Mo’pr sin 0 = L.
219. The result of the preceding article may be other-
wise obtained.
In Art. 25, it is shewn that the acceleration of the point
P, when at A, in direction of the normal at A is
o'pp'/(p +p’).
The acceleration of G relative to A, in the direction
perpendicular to AG js rw, and therefore the actual accelera-
tion of G perpendicular to AG is
ro — opp’ sin 6/(p +p’).
Hence, equating momenta about A,
Mia + Mr {re — opp’ sin O/(p + p’)} = L.
B. D. 18
274 MOTION OF LAMINA.
220. The investigation of the two preceding articles is
the infinitesimal case of the following general statement.
@ @f
If Q be the linear momentum of a body, in motion in one
plane, when P is the instantaneous centre, and Q’ at a
subsequent time when P’ is the instantaneous centre, G
being the centre of inertia, the change of the angular
momentum about P is
Mi? (o' — w) + Q' (r’ + PP’ cos 4) — Qr.
221. Asa particular case consider the motion of a heavy
uniform circular disc of radius ¢ rolling on the curve,
s=of (), starting from the highest point, from which s and
are measured.
In this case, 9=0,
1 1 " Se r
and o= ff + ate (9) ¢=(1+f'9) ¢,
and the equation of motion becomes
30° ; Pah ia IS 5
MEL +f GIb+S" () 4b} =Uge sin $.
Suppose the curve to be a cycloid, s=csin ¢;
then cos f—sin § f= 3.2 sin$,
MOTION OF LAMINA. 275
the integral of which is
ihe ohn. aie
3cp cost 5 = 2g(1 cos 5)
and therefore ait (1 — cost $ ) .
3c 2
To find the pressure we have the equation,
ew M
e. g cos p— Rh,
shewing that & vanishes, and therefore that the disc flies off,
when 5 cos ¢ = 3.
At the instant of flying off, w” = 249/25c, and the velocity
of the centre of the disc is 2/6gc/5.
222. Change of motion produced in a lamina, moving in
any manner in its plane, produced by its impact on a rough
curve.
We suppose the roughness to be so great that there is no
sliding, and we have simply to express the fact that the
angular momentum round the point of contact is unchanged.
P being the point, let v be the component perpendicular
to GP of the velocity of G, w and w’ the angular velocities
just before and after the impact; then
M (kh +17") 0 = Mk’o + Mor.
' Suppose for example that the disc of the preceding
article, just after flying off the cycloidal arc impinges on a
fixed rough peg just beneath its lowest point.
In this case
So «se ‘
7? =5 o+c’a cos ¢,
from which we obtain 150’ = 11.
The disc will then turn round the peg as a fixed point,
and the equations of motion will determine the angle
through which it turns before leaving the peg.
18— 2
276 BREAKING OF RODS.
223. In general if a rigid body, or system of any kind,
be in motion, and if a straight line of the system suddenly
become fixed, the angular momentum of the system about
the axis is unchanged.
In the case of a single rigid body this at once determines
the angular velocity about the axis.
Thus, if Q be the linear momentum of a rigid body
perpendicular to the axis which becomes fixed, p the distance
from the axis of its centre of inertia G, and H the angular
momentum about the line through G parallel to the axis,
the angular velocity is given by the equation
Mio = Qp + H,
Mi? being the moment of inertia about the axis which
becomes fixed.
224, Tendency of a rod in motion to break at any assigned
point.
Imagine a rod of small section and of any shape, its axis
however being a plane curve, to be in motion in that plane
under the action of forces in the plane.
Taking any cross section, through any point P of the axis,
the stress at this section, that is, the action and reaction
between the two parts of the rod separated by the cross
section, may be represented by two forces Z'and NV at P in
directions of the tangent and normal to the axis, and a couple
G in the plane of the axis.
The velocities and accelerations of the various points of
the axis having been previously determined, the quantities
L, N, and G can be found by writing down the equations of
motion of either of the two parts of the rod, including 7, N,
and G amongst the acting forces.
Now a rod may break in three ways; the internal
molecular forces may not be sufficient to withstand the force
T in direction of the tangent, or they may give way in
direction of the normal, or the moment about P of the mole-
cular forces may be overpowered by the couple G.
BREAKING OF RODS. 277
In other words the rod may break by tearing, by shearing,
or by snapping, and the quantities 7, NV, and G are, respec-
tively, the measures of the tendencies to break in these three
ways.
To illustrate, take the case of a heavy straight rod swing-
ing in a vertical plane about one end, and examine the
tendency to break at the middle point.
Writing down the equations of motion of the lower half
of the rod, and taking ras the distance from the axis-of a
point in the rod, we obtain
2a 6dr 5 3 2a dr
[ m 578 = N— ging sin 0, [ m5
a
76? = T — kg cos 0,
2 .
[omer @-a) d= G — mga sin 8,
where 6 and @ are known functions of 6, and these equations
determine the values of 7, NV, and G at the middle point of
the rod.
225. If arod have its state of motion suddenly changed
by impulsive action, impulsive stresses are created at all
points of the rod, and the method of determining them is the
same as in the previous case.
If for instance the free end of the swinging rod, supposed
inelastic, be suddenly stopped by impinging against a fixed
surface, and if 7, N, and G then represent impulses, the
equations are
2 ‘
T= 0, [m= N-P
i 2a
2a .
| — mF r(r—a)b= G —4Pa,
a
where P, the impulse at the free end, is given by the equation,
mab = BP.
226. Determination of initial stresses, and initial accelera-
tions, when some of the constraints of a system, previously in
equilibrium, are removed.
278 INITIAL STRESSES.
In such cases the equations of motion should be written
down for the configuration ofthe system at the instant of
release from constraint,
These equations, in combination with the kinematical
relations of the system, will be sufficient for the determination
of the required stresses.
The equations are simplified by the fact that the linear
and angular velocities are zero, so that radial and transversal
accelerations take the forms 7 and 76, and normal accelerations
are evanescent*.
Exampies. (1) wo rods AB, CD, of lengths 2a and
2b, are connected by equal strings AC, BD, of length c, and the
system 1s supported, with the rods horizontal, by a fixed hori-
zontal axis through the middle point of AB; if one string AC
be cut, at is required to find the initial tension of the other.
Let w, w, and w be the initial angular accelerations, in
the directions figured, of the two rods and the string.
/)
wo
A
Sp) manne neneen ened
The vertical acceleration of G, the centre of gravity of CD,
= ba’ + cw” cos a+ aw,
and its horizontal acceleration = cw” sin a.
Hence the equations of motion are
a
mx @ = Ta sina,
* Some illustrations of the method of finding initial stresses are given in
an article in the Mathematical Messenger for 1866.
INITIAL CURVATURES. 279
m’ (bw' + co” cosa + aw) = m'g— T'sina,
m'cw” sina = T cos a,
Bg.
ms wo = T.bsina,
which determine the tension and the angular accelerations.
(2) A heavy rod, of length 2a, is supported against a
smooth fixed sphere by a horizontal string fastened to its upper
end A, and also to the highest point of the sphere; if the
string be cut it is required to find the initial pressure on the
sphere.
If « be the angular distance of the vertex from P the
point of contact, it will be found that PG =asin’a. Observ-
ing that the acceleration of P is wholly tangential, and taking
as the initial angular acceleration of the rod, it follows
that wPG is the acceleration of G perpendicular to the rod,
and therefore taking moments about P
a
3
We have also moP G=mgcosa—R,
and we obtain R(1+3sin*a) =mg cosa.
m= o + mPG’o =,mgP G cos a.
227. Determination of the initial radit of curvature of
the paths of assigned points of a system, when the system is set
in motion in any given manner, or, being in a state of equi-
librium, has some of tts constraints removed.
If the velocity and direction of motion of an assigned
point of the system be known, the expression for the normal
acceleration, v’/p, determines the curvature, 1/p, for the
acceleration of the point in the direction of the normal to its
path is obtainable from the equations of motion of the
system.
EXAMPLES. (1) Two particles, m and pu, are connected by
a string passing over a smooth fixed horizontal rail, and, the
portions of string, of lengths a and b, being vertical, the
particles are projected horizontally, in opposite directions
perpendicular to the ratl.
280 INITIAL CURVATURES,
The initial equations of motion are
m (# — 76°) = mg — T, m (rb + 276) =0,
ub — pd) =n9 —T, w (pb + 264) = 0.
If u and v be the velocities of projection, then, initially,
r=a, p=b, r=0, p=0, aG=u, bp =2,
and therefore 6=0, d =0,
uw vw
m(i#-F)=mg-F, »(6-F)=ng- 7,
and these equations, with the equation *+ p= 0, determine
*, p, and T.
The initial radii of curvature R, R’ of the paths of m and |
p are given by the equations
uw
vw
m= T—mg, mm = T — ug,
assuming the concavities to be upwards.
If Tis less than either mg, or yg, the concavity in that
case will be downwards.
(2) A rod AB is moveable in a vertical plane about the
end A, and a string BC carries a heavy particle at C; the
particle is held in a given position in the vertical plane through
the rod, and is projected in the direction perpendicular to BC’
in the vertical plane.
If 6 and ¢'‘be the inclinations of AB and BC to the
vertical at the moment of projection, the initial equations of
motion are
ue b+ mbp {b + 2a cos (f — 6)} — mb? 2a sin (d — 0)
+ m2a6 {2a + b cos (¢ — 6)} + m2a6’ b sin (¢ — 6)
= Mga sin 0+ mg (2asin 6 + bsin ¢),
and b+ 2a6 cos (f — 6) + 2a6* sin (6 — 0) =—gsin ¢,
where 2a and 6 are the lengths of AB and BC.
INITIAL CURVATURES. 281
Initially, if u be the velocity of projection,
6=0, and u=dd, :
and the preceding equations determine @ and ¢.
The acceleration of the particle in the direction CB is
initially bd? — 2a0 sin (f — 9), and this is equal to u*/p if p be
the initial radius of curvature of the path of C.
228. Ifasystem have initially no motion, and. we wish
to find the initial curvature of the path of any assigned
point of the system, we must first find the initial direction
of motion, and then, observing the small displacements which
take place in a very short time, we can sometimes obtain the
curvature by an immediate application of the Newtonian
expression for the diameter of curvature, viz. (arc)” + perpen-
dicular subtense. Sometimes however it is necessary to take
the analytical expression, in Cartesian or polar co-ordinates,
or in some other system, and to expand, in ascending powers
of the time, the various terms contained in these expressions.
An illustration of each case will be sufficient to explain the
methods.
(1) Two rods, AB, BC, freely jointed together at B, and
moveable about the end A, are held in a horizontal position so
as to form a straight line ABC, and are then let go;
it is required to find the initial curvature of the path
of C.
Let uw, m be the masses and 2a, 2b the lengths of AB
and BO, then, if w and ’ be the initial angular accelerations
of AB and BC, it can be shewn, by taking moments about A
for the system and about B for the rod BC, and combining
the equations, that
a @
Now supposing that, after a short time ¢,@ and ¢ are
the inclinations of 4B and BC to the horizontal, it follows
that the horizontal and vertical displacements of C are
2a + 2b'— 2a cos 6 — 2b cos ¢, and 2a sin @ + 2bsin ¢,
or, approximately, ;
ab? + bg? and 2a0 + 2b4.
282 INITIAL CURVATURES.
The initial tangent to the path of C is vertical, and
consequently
5 ~ ., 4 (a8 +b)"
< 2o = Limit of oo = we .
The first approximations to @ and ¢ are
0 = ot’, 6=ho't’,
and we hence obtain
i EE
2ab--b (m+ 2u)* +ap""
(2) A plane lamina, which is moveable about a horizontal
axis on its plane, is inclined to the horizontal at an angle a,
and a heavy particle m is placed upon tt at a distance c from
the axis and below the ams; it is required to determine the
initial curvature of the path of the particle.
If @ be the inclination at any time, the equations of
motion are
Mk’6 + mr (r6 + 276) = mgr cos 6,
¢—7r6=gsin 0.
The expression for the radius of curvature is
(r°6* + 5)8
PO + 27°6 — r (6% — 76)’
and we have to expand in powers of ¢, the various terms of
this expression, which can be effected by Maclaurin’s
Theorem.
Taking m? to represent Mk’ + mc’, we obtain, from the
equations of motion,
pe Shay x gcocos a
F=gsina, 6, = E
» g'ecos? Qc? ~ g' 8in a COSa 7c
=f F ae Fr) 6 = (1-+).
, #,=0, 6,=0,
VIRTUAL WORK. 283
Now G=8 E+... PHPEL
. as se s, wee. 3
and 6 —7O= Birt #8) BF ene
and therefore
G2+0d2)!
C03 + 2128, 2 (Bs — 78)
Po =
and, making the requisite substitutions, we obtain p, in terms
of a, J, and ¢.
If a=0, it will be found that
3c 3inc®
Po= FB Ue
the negative sign shewing that the concavity of the initial
path is outwards-from the axis.
229. Application of the principle of virtual work.
If at any instant the geometrical configuration of a
system be contemplated, and if a geometrical displacement
be imagined, the virtual work of the time-fluxes of momenta,
or of the effective forces, and of the acting forces will be the
same,
We must however include in the phrase acting forces
any internal forces such as the tensions of elastic strings,
or sliding frictions, by means of which. work is done on the
system.
Considering a single rigid body, i.e. a material system of
invariable form, if #’ be the time-flux of the linear momentum
in any direction, and és the displacement of the centre of
gravity in that direction; and if K be the time-flux of the
angular momentum about an assigned axis through the
centre of gravity, and 5¢ the angular displacement about the
axis, then the corresponding portions of the virtual work
are Fés and Ké¢.
(1) Consider for example the case of the two rods in
Art. 215. ‘
284 VIRTUAL WORK.
Taking « and y as the horizontal and vertical co-ordinates
of G, we obtain
2 2
m = 680 +m’ hdd + m'#d2x + m'ijdy = m'gdy — mga sin 88.
Now «=2asin6+bsin ¢, and y= 2acos 6 +b cos ¢,
from which dx and éy are obtained in terms of 5@ and 8d,
and observing that 8? and $¢ are arbitrary quantities and
independent of each other, their coefficients must each
vanish, and we thus obtain the equations for the determina-,
tion of 6 and ¢.
ExampiLe. (2) Motion of an extensible circular ring,
placed horizontally over a smooth surface of revolution the aats
of which ts vertical.
Let s represent the distance along a meridian are from a
fixed level to the ring, 7 its radius and z the depth of its
plane. The accelerations of any point of the ring down the
meridian are and perpendicular to it are § and s’/p, and there-
fore, if we imagine a displacement by slightly shifting the
ring downwards on the surface the equation of virtual work
is, m being the mass of the ring,
ms8s = mgdz — TS (207),
or mi= mg — 2D S,
an equation which can also be obtained by considering the
meridional motion of an element of the ring.
Observing that Z=2(r—a)/a, and that r=f (z);
this equation determines the acceleration along any
meridian.
(3) Four equal rods, of length 2a, are jointed together in
the form of a square OADB, and suspended from the joint
O, the square form being maintained by a string OD;
of ae string be cut it 1s required to find the change of stress
at O.
_ Take as the expression for the initial angular accelera-
tion of each rod; then if G and H be the centres of gravity
VIRTUAL WORK. 285
of OA and AD, the initial vertical accelerations of G and H
are aw/,/2 and 3aw/,/2 ;
and the initial horizontal accelerations are each awn! 2, also
the time-flux of the angular momentum of each rod is
mew/3. .
_ If we imagine D pulled through a small space, so as to
displace each rod angularly through the small angle @, the
linear displacements of G and H are, vertically, «6//2,
3a6/,/2, and horizontally each is a0/,/2; also the vertical dis-
placement of the centre of gravity K of the system is a0,/2.
Hence we obtain
awd 9a?wd vod awd =
at 2m = + dm SS + dm <= dng /2,
from which 10a = 39/,/2, and therefore the acceleration of
K is 39/5, shewing that the pressure on the point of support
is instantaneously diminished by three-fifths of the weight of
the system.
If P be the horizontal stress at D, it can be determined
by giving the rod AD a small arbitrary twist, 0, about 4,
breaking the connection at D.
2m
The equation of virtual work will be
& 38maw a0 maw af ae
= 50 — oe ae ee eee —— + Paé 2,
ME ae gale
awh! _ _ mg
from’ which P = io°
If Q and R be the actions at A upon OA in the directions
DA and OA, these quantities may be found by giving DA a
twist about D, and OA a twist about O, breaking in each
case the connection at A.
The equations obtained are
maw 6 3mao a maw ad
aé
es — .—— = R?2 6- Fe
3 oo we ge
286 VIRTUAL WORK,
ao maw a0 maw ad aé
al o° fe ere 2. 6— ==;
mee 8 i
and from these we find that
R=3,mgJ2 and Q=y5mg,/2.
In solving this question our object has been to illustrate
the use of the principle of work, but the same result may be
obtained from the initial equations of motion of the rods,
which are 4maw mga
3 ~/e — 2aQ,
ate gh mab Vd _ pp
J/2 J2 * f2 fh ,
mara Pa
3 noes
EXAMPLES.
1. A smooth sphere is at rest on a smooth horizontal
plane, and an equal sphere is placed gently upon it, so as to be
in contact very nearly at the highest point; prove that the
centre of the upper sphere will describe a portion of the arc
of an ellipse, and that when @ is the inclination to the
vertical of the line of centres,
a6? (1 + sin? 6) = 2g (1 — cos 6)...
Shew that the spheres will part company when
cos 0=,/3—1.
2. Two equal smooth spheres rest in contact on a
smooth horizontal plane and another sphere is placed between
them, so that motion ensues. Find the pressure between
them at any time in terms of the inclination to the horizon
of the lines joining their centres.
EXAMPLES, 287
3. If two weights be suspended by a weightless string,
which passes over a rough circular cylinder of given mass,
the space described by either in any time is independent of
the radius of the cylinder.
4, Two equal smooth spheres are placed one upon the
other and both in contact with a smooth vertical wall.
If the lower one just leave the wall, prove that they will
separate when the line joining their centres is inclined to the
horizon at an angle cos’ (2), the motion being supposed to
take place in a vertical plane.
5. Four equal rods are jointed together so as to form a
square ABCD, and the system is suspended from the point
A, the square form being maintained by a string connecting
A and C. Find the tension of the string.
‘If the string be cut, prove that during the subsequent
motion,
aG (1 + 8sin’ 6) = 3g (cos g- =) ;
2a being the length of each rod, and @ the inclination to the
vertical.
6. Three equal smooth balls are kept in contact with
each other on a smooth horizontal plane by a string passing
round them, and a fourth equal ball rests upon the three; if
the string be cut, what is the initial change of pressure
between the upper ball and each of the lower ones?
7. Four equal smooth inelastic circular discs, of radius
a, are placed in one plane with their centres at the four
corners of a square of which each side is 2a. They attract
one another with a force varying as the distance. 2a. If the
rod be slightly displaced from its position of stable equi-
librium, prove that the time of a small oscillation is
9 Qac B
™ 139 (¢—2a)) *
44, Four equal uniform rods are jointed together so as
to form a square ABCD, and the system is suspended from
the joint A, the square form being maintained by an elastic
string joining A and C.
Find the tension of the string, and, the modulus of
elasticity being twice the weight of one of the rods, prove
that, if C be slightly depressed, the length of the simple
isochronous pendulum will be 540/12. If, when there is
equilibrium, the string be cut, prove that the initial pressure
at C is equal to one-tenth of the weight of one of the rods,
and that the initial acceleration of C is equal to 69/5.
45. A cylindrical mass of snow rolls down an inclined
plane covered with snow of uniform depth e; gathering up
all the snow it rolls over, and always remaining circular.
Prove that it will move with uniform acceleration g sin a/5 if
initially when its radius is a it be started with velocity
a2: sin a/5¢, where a is the inclination of the plane to the
horizon.
296 EXAMPLES.
46. Three particles A,B, C are connected by two strings
AB, AC and placed in a line on a smooth table. The
extreme particles B and C are then projected at right angles
to the strings with velocities u, v. Prove that the initial
curvatures of the paths of the extreme particles are respec-
tively
v v wu
uw
(q+ m) — +O 5 a (p +m) 5 +P
(p+q+m) wu (p+q+m)v
m, p, ¢ being the masses of the particles, and a, b the lengths
of the strings.
>
47. Two particles of masses m,, m, are tied to the
extremities of a string that passes through a bead of mass VM,
the whole is placed on a smooth table with m,, m, at the
acute angles and M at the right angle of a right-angled
triangle, if the particles at the ends be projected with
velocities w,, w,, perpendicular to the respective strings, then
shew that the initial radii of curvature of their paths are p,, p,
2 2
U, U,
2 2 _ Pa
where MU Melly Gy
A fe UD
—+ 7+
m LW,,
and therefore
h, = Xm (y? +24) @, —¥ (may) wo, — 5 (may) 0,
and, if we represent the three moments of inertia by
A, B, C and the three products of inertia by D, #, F
we have
h, = Ao, — Fo, — Eo,,
h,= Bo, — Do, — Fo,,
h,= Co, — Ew, — Do,
If the expressions D, EH’, F all vanish the axes are said to
be principal axes; if two vanish, the corresponding axis is a
principal axis.
302 SPHERE ON PLANE.
In the case of a sphere, or a solid bounded by any
regular polyhedron, when the centre is the origin, D, H, F all
vanish, and A, B, C are all the same, so that the angular
momenta take the forms .
Aw,, Ao,, Ao,
In the case of a solid of revolution, or of a regular
pyramid, the axis of which is one of the axes, D, H, F all
vanish, and the angular momenta.are
Aw,, Aw,, Co,.
In the case of a plane lamina, when one axis is perpen-
dicular to its plane, D and £ vanish, and the angular
momenta are
Ao, —Fw,, Bo,— Fw,, (A + B) a,.
234. If the axis of z be fixed in space, the time-
fluxes of angular momenta about the instantaneous positions
of the axes are I . é
h,—h,O,, h, +h,O,, hg
It may be instructive to obtain these expressions directly.
Thus, at the time ¢ + 6, the angular momenta about Oz’, Oy’,
the consecutive positions of Om, Oy, being h,+ dh,, h, + 8h,,
it follows that the angular momenta about Ox and Oy are
respectively
(h, + 8h,) cos 0,5¢ — (h, + 8h,) sin 6,8¢,
(h, + 5h,) cos ,6t + (h, + 6h,) sin 6,64,
and, subtracting h, and h, and dividing by 6, we obtain, in
the limit, the expressions given above.
The general expressions of Art, 230 may be obtained in a
similar manner.
235. We are now in a position to solve some problems,
and we commence with the motion of a sphere on a rough
plane, under the action of forces the resultant of which passes
through the centre of the sphere.
Referring to fixed axes the linear momenta are ma, my,
and the time-fluxes of the angular momenta are
Aw, Aw, Aw, where A = 2me’/5.
FIXED AXIS. 303
Assuming X, Yas the forces, and taking moments about
the lines in the plane through the point of contact parallel to
x and y, we obtain
—mijc+ Ao, =— Ye, miic+ Aa, = Xe.
We have also the geometrical conditions,
é—cw,=0, y+ cw, =0,
and we hence obtain
mi =iX, my =hY.
If the frictional reactions be required, they are given by
the equations
mé&=F+X, my=G+Y,
so that F=—-2X and G=-32Y.
If the plane be made to revolve uniformly, with the
angular velocity Q about the axis of 2, the equations of
motion are the same, but the geometrical conditions are
é—cw, =— Oy, y+cw, = On.
If in this case there be no forces in action, the elimination
of w, and w, leads to the equations
Ti+ 20y=0, 77 —20%=0,
or,if Tnr=20, +n? (e@—a)=0, +n? (y—b) =0,
where a and 6 are constants.
Integrating these equations and eliminating the time, we
shall find that the path of the centre of the sphere is an
ellipse, of which the point (a, 0) is the centre.
236. To illustrate the use of two moving axes, consider
the motion of a rigid body about a fixed axis.
Taking, as in Art. 211, the line OG as the axis of w and
the fixed axis as the axis of z,
w=— Yo, v= 20, w=),
and therefore,
h,=— Eo, h,=—- Dw, h,=Co.
30+ ROTATING DISC.
Hence h, —h,0,= — Eo + Do’,
h,+h,0, =—Do— Eo’,
and equating these expressions to the moments of the
acting forces, we obtain, as in Art. 211, the stresses on
the axis.
237. A circular disc, the plane of which is vertical, and
centre fixed, is rotating about a horizontal amis through its
centre perpendicular to its plane, which axis is itself rotating
Jreely in the horizontal plane through the centre, and an
insect crawls in a given manner on the disc.
Taking the figure of Art. (247), let ZC be the plane of
disc, OC being a given radius of the disc.
The equations of motion are obtained by observing that
the angular momentum about Oz is constant, and that the
time-flux of the angular momentum about OF’ is equal to the
moment about OF of the weight of the insect.
Let p be the distance of the insect from O, and ¢ the
angular distance of p from OC measured in the direction CZ,
so that p and ¢ are known functions of the time.
Putting ZC = 6, and XZC'= wy, we obtain
Mk'yp + mp’ sin’ (0+ $) p=C.
» 2, be the angular momenta about OK and OF,
h, = mp" sin (0+) cos (8 + $),
h, = 2Mk’O + mp’ (6 + ).
Hence we obtain, since h,+h, is the time-flux of the
angular momentum about OF,
2MKO + mp? (6+46)-+ 2mpp (0+46)-+mpp? sin (4+ ) cos (0+¢)
= mgp sin (0 + $),
and 6 and are determined by these equations.
If h
238. Motion of a heavy sphere on the interior rough
surface of a vertical cylinder.
The figure being a section by the horizontal plane through
the centre of the sphere, take the axis (3) through C vertically
upwards and measure z upwards.
SPHERE ON CYLINDER, 305
The accelerations of C in the directions (1) (2) and (8) are
—(a—c) $*, (a—c) , 2.
In this case, since h, = Aa,,h, = Aw, and 0,= 4, the time-
fluxes of the angular momenta about the instantaneous
positions of the lines (1), (2), and (3) are
Ao, — Aa, , Aw, + Ao, d, Ao,
Tv
_ Taking moments about CP, PT, and the vertical through
P, we obtain
0, —o,6 = 0, Aw, + Aw,d + mez=—mge, Aw,—m (a—c) ch=0.
Expressing the fact that the point P of the sphere has
no velocity, the geometrical conditions are
(a—c)p + cw, = 0, z—cw, =0,
we at once see that ¢ and a, are constant, that co, = dz, and
therefore that 47+ Ad¢’z+mc’z is constant, or that if 2¢7=7n’,
Z+nv7z=C,
shewing that the ball rolls up and down, between two fixed
levels, in the time 7/n.
If the cylinder, instead of being fixed, be made to revolve
with a constant angular velocity about a vertical generating
line through the point O in the figure, the angular velocity
of the line CH is +; and the accelerations of C in the
directions (1), (2) and (3) are, putting b for a—c,
aw® cos d —b (w +b)’, bf — aw’ sin ¢, 2.
B. D. 20
306 SPHERE ON CONE.
Hence, taking moments about the same axes as before,
we obtain,
@,— @, (o +) =0, $ cw, + 3CO, (o+ d) +Z=- 9,
2 cw, —b G+ aw’ sin = 0.
The geometrical conditions are that the velocities of the
point P of the sphere and of the point P of the cylinder are
the same,
cw, +b (w +) — aw cos 6 = aw—awcos d
or co, +b (w+¢) = aa,
and %—cw, = 0.
Eliminating , we find that
7b = 5aw* sin ¢,
an equation which determines the angular motion of the
centre of the sphere relative to the cylinder. —
239. Motion of a heavy sphere on the interior rough
surface of a cone having tts axis vertical and vertex
downwards..
The figure being a section of the system by the vertical
plane through the axis of the cone and the centre of the
sphere, the accelerations of C are
F—r¢’, rot 2rd, 2,
and the time-fluxes of angular momenta are the same as in
the preceding case.
The geometrical conditions are
TF — CW, SIN A= Oe eeeeeee eens (1)
rh + cw, Sin a+ Co, COS4=O.eeeeseeeeee (2)
B= Oil, COR = Oo. sa sidaaisac'vonain re (3).
Taking moments about PH, PC, and the line through P
perpendicular to the plane of the figure we obtain
(Ao, — Aw,¢) sin a+ Ad, cos a—m (rb + 27) o= 0...(4)
(Ao, — Aw, d) cos a— Ad, SNA =Ovieeceeserrereeees (5)
Ao, + Aw, p+ m (i — 7g") csina + mic cosa =— mge cosa...(6).
SURFACE OF REVOLUTION. 307
From (4) and (2) we find that rd + 27'6=0, or that r°d=h,
From (4) and (5) it follows that #,=0, or that a, =n.
(3)
H
N (1)
0
Lastly from (6), with the aid of (1), (2), (3), and the
preceding results, we find, if we write w for 1/r, the equation,
du 2+5sin"a ,gsinacosa ,cncosa
dd? eee
240. The general problem of the motion of a sphere on
any surface of revolution may be treated in the same manner,
or we may employ three moving axes.
Taking the axes as in the figure, and taking wu, v, w as the
velocities of C in the directions (1), (2), and (8), the geo-
metrical conditions are
u—co,=0, v+co,=0, w=0.
Since 0,=¢ cos 6, 6,=6, 0,=¢sin 8,
&— v0, + wO,= cw, + co, sin 0,
d—w0, + uO, = — ca, + ca, sin 8,
w — uO, + v0,= — cw,0 — cw, p cos 9,
which are the accelerations of C.
308 SURFACES OF REVOLUTION.
Hence, if L, M@, N be the moments of the acting forces
about PT, about the line through P perpendicular to the
plane AGP, and about PO, the equations of motion are
A (o, — @,g sind + w,6) — me (— cw, + cw, sin 0) = L,...,
A (&, — ag cos 0 +, sin 8) + me (cm, + 00h sind) = M,...ii,
A (@, — 0,6 +, cos 0) = N.. iii.
It will be seen that C moves on a parallel surface of which
A is the vertex, and if AN=z and CN =r, the relation
between r and z is known, so that z=/(r).
Hence if s be the are AC
co, =u=s=— pb,
if p be the radius of curvature of AC at C.
We also have cw, =—v=— rd.
If for example the surface be a sphere, and gravity the
only force in action,
L=0, N=0, and M=— mge cos 0.
Also, in this case,
cw, = — a6, cw, = — acos 64,
and therefore, from equation iii,
®,=0, or o, =n.
SPHERE ON DISC. 309
These values of w,, w,, o, being substituted in equation
1, we obtain
a cos Op — 2a sin 6 6b = 3 end, °
and therefore
cos"0g = C +2 = sin 0.
Substituting in equation ii and integrating we obtain a
differential equation of the first order for 0.
This last however is more easily obtained from the
equation of energy which is
a6” + a? cos* 04 + 20 (w,? +o," + ,°) = D + 2ga.cos 6,
‘9 con. ,\* 10g
or 0 + s00%9 (C+? sind) =H+ >~ cos 6,
a 7a
C and £ being constants determined by initial conditions.
241. Motion of a rough sphere on the surface of a flat
disc, which is moveable on a smooth horizontal plane, the
upper surface of the disc being perfectly rough.
wt
7 NV ax
FO i.
(2)
We shall suppose that the centre of gravity of the system
has no motion; this will be the case if the disc be initially at
310 SPHERE ON DISC.
rest, and if the sphere, in a state of rotation about a diameter,
be placed gently upon the disc.
In the figure O is the projection on a horizontal plane of
the centre of gravity of the system, Z of the centre of gravity
of the disc, and C of the centre of the sphere; Ox, Oy are
fixed directions.
Taking £, 7, and a, y, as the co-ordinates of H and 0,
measured in opposite directions, and Q as the angular velocity
of the disc, the geometrical conditions are
& — c0,= — E—O (yt), veceeceeeeseennees (1)
YtCo, =—AEA(GHE). creccrcceccseceees (2).
Taking moments for the motion of the sphere, about the
horizontal tangent lines parallel to the axes,
mic+mk'o,=0, mijc—mk*o, =0,
and therefore #+2cw,=A, y—2cw,=B....... (3), (4).
The angular momentum of the system about any
assigned vertical line is constant, and if the sphere have
initially no rotation about the vertical diameter this constant
is zero.
Taking moments about the vertical line, fixed in space,
through which JF is passing,
MK*O,= ma (y +) — my (@+ &),
or MRP =m (+ M) (bY — Yb) ciececcceceves (5).
We have besides ma = ME, and my = My, and we thus
have seven equations to determine the seven unknown
quantities.
If the original axis of rotation of the sphere be above the
line Ox and parallel to it, so that initially
o,=n, and wo, =0,
we obtain &+2co,=0, y—2co, = B.
The elimination of w, and », leads to
24 (M+ m) + 5Mé = — 2yO, (iM +m),
2y (M +m) + 5My — 5MB= 220 (M+ m),
ROTATING ROD. 311
and, substituting for Q its value from (5), these equations
take the forms
(a+ by’) & =bay y, (a+ ba’) y = bay é+e,
where a, 6 and c are constants.
The integration of the first of these equations gives
a+ by’ = Cx’,
shewing that the path in space of the centre of the sphere is
a hyperbola, (a result given in the Tripos Examination,
Jan. 1882).
It should be mentioned that nm is the initial angular
velocity of the sphere just after having been placed in contact
with the disc.
‘If w be the angular velocity of the sphere about the
diameter parallel to the axis of # before the contact, and if X
be the angular velocity of the disc immediately after the
impact, m and A are determined by the equation
mk'n — myc = mk*w,
combined with the preceding equations (1), (2), and (5) in
their initial forms.
242. Motion of a heavy rod AB, the ends of which shide
on a fixed vertical rod OB, and a horizontal rod OA, which 1s
made to revolve uniformly.
If r be the distance from G, in the direction GA, of a
point P of the rod, the accelerations f, f’ of the point in the
2 2
directions LP and MNP, are - PL—o'PL, and ae PN,
where PL, PN are the perpendiculars upon OB and OA, so
that PL =(a+r)cos 0, and PN= (a—1) sin @.
Taking moments about the line through £ perpendicular
to the plane OAB, we obtain
: mo {(a+r) fsin 0—(a—7r) f’ cos 6} = mga cos 0.
—a
312 ROTATING ROD.
Substituting for f and /’ their values, and integrating,
this reduces to
oe ie 3g
2 a I
0+’ sin 8 cos 6 = he 08
We have solved this question by an appeal to first princi-
ples, but it may be instructive to indicate the method of
dealing with it by the aid of the expressions for angular
momenta,
()
B B
¢ F,
y : P $
wv 4
Taking for axes the line GA, and the lines through G
perpendicular to and in the plane OAB,
6,=—asin6, 6,=6, 0,=acos8,
and h,=0, h,=mk’o,, h, = mk’o,.
The acceleration of G in the plane OAB, perpendicular
to OG =a +asin@cos@.0%. Art. 15,
and the rate of change of the angular momentum about the
second axis =mk’o, + mk’w, w sin 6.
Hence the equation of moments about the line through Z
perpendicular to the plane is
2
a? a ‘
3 tm ww sin @=— mga cos 6;
and, observing that , = 6 and that w, = cos 0, this reduces
to the equation previously obtained.
ma? (6 + sin 6 cos Ow") +m
SOLID OF REVOLUTION. 313
If the system instead of being made to revolve uniformly
be set in motion and left to itself, we shall have, taking ¢ for
the azimuthal motion, and neglecting the inertia of the rods
OA, OB,
6+ gtsin 0 cos 6 = — 22 cos 6,
with the additional equation, derived from the fact that the
angular momentum about OB is constant,
c mo (a+r) cos’ 0.46 = C.
—a
243, Steady motion of a heavy body in the form of a solid
of revolution, rotating uniformly about its axis, one point O of
which is fixed while the amis has a constant inclination to the
vertical (a), and a constant azimuthal motion (Q).
(3)
®
Taking moving axes as in the figure, the second axis
being perpendicular to the plane of the paper,
6,=—QOsina, 0,=0, 0,= 0 cosa,
314 SOLID OF REVOLUTION.
also o,=0 and o,=—Q sina, and, taking moments about
the axes, we obtain
Ao, =0, Co, Asina+ Ao, XO cosa=mgasina, Co, =0.
Putting n for w, this gives
COn — AQ? cos a = mga,
as the condition for steady motion.
Ifa=— , COn = mga, so that if the angular velocity n be
imparted to the body about OC, when OC is _ horizontal,
and OC be then started with the angular velocity mga/Cn
about Oz, the axis OC will continue to revolve in a horizontal
plane.
_ In the general case, when the motion is not steady, take
ap as the azimuthal motion, so that
6,=—wsin 0, 0,=6, 6,= cos 8,
and therefore
Ad, — Aap cos 6+ Cw,6 = 0,
Aw, + Co, sin 6+ Aw, cos 6 = mgasin 6,
Ca, — Aw,6 — Ao, sin 0 = 0.
Now o,=—sin 0, and w,=6, and we find that , is a
constant (n) and that
— Ap sin 6 — 2AW4 cos 0 + Cnb =0,
AG + Cn sin 6 — Ary’ sin 6 cos 6 = mgasin 6,
two equations which completely determine the motion.
If the motion be very nearly steady, the small oscillations
are determined by putting
6=a+¢, and p=N+4+y,
and neglecting the squares and products of the small quanti-
ties @ and x.
These results are roughly illustrated by observing the
SOLID OF REVOLUTION. 315
motion of an ordinary spinning top on a rough horizontal
plane.
The most complete illustration is obtained by means of a
Gyroscope.
K
A heavy brass solid ring is moveable about the diameter
OC of a circular brass framework, and, holding this frame-
work, a rapid rotation can be imparted to the ring. This
can be effected by looping a string to a peg at H, winding up
the string and pulling it out sharply.
This being done, the point O may be held by a string,
and OC placed at any inclination to the vertical.
Or, if a small peg be fixed at O underneath the rim of
OC, this may be placed on the cup K of a fixed vertical _
stand KZ, and then the axis OC may be seen to revolve |
horizontally.
244, Steady motion, about a fixed point O, of a rigid
body so constituted that two of the principal moments of inertia
at the point O are equal.
In this case, of which the preceding is a particular case,
the constraining couple is equal to
(COn — AQ? cos a) sin a.
If Cn = AQ cos a, this expression vanishes, and the steady
motion continues without the action of any extraneous force.
316 CASE OF TWO EQUAL MOMENTS.
245. Motion of a rigid body about a fixed point O under
the action of no extraneous forces, the body being so constituted
that A and B are equal at the point O.
The body is supposed to be set in motion in a given
manner, or by means of given impulses.
The moments about the principal axes of the given
impulses are the initial values of the angular momenta
Aa,, Aw,, Ca,
There being no forces in action the angular momenta
about any fixed lines through the point O remain unchanged
and therefore the resultant angular momentum is a constant
quantity, H, and the axis of resultant angular momentum is
a fixed line.
This line, which is called the invariable line, we shall take
for Oz.
Take OC as the axis of (3), and, for axes of (1) and (2)
the line in the plane zOC perpendicular to OC, and the line
perpendicular to the plane 200.
Then if y be the inclination of the plane 200 to a fixed
plane through Oz,
6,=—ysin 6, 6,=6, 0,= cos 8,
and the equations of motion are
A@, — Ao,rp cos 6 + 00,0 = 0, cescceccsseeeesees (i)
Ao, + Cor sin 0+ Aw, cos 0 = 0, oe (ii)
Co, — Aw,6 — Aor sin 0=0. veces (iii).
We have also o,=— sin 9, and o, = 6, and therefore,
from (iii), it follows that @, is constant.
Now, Hcos 6=Cw,, and therefore. it follows that @ is
constant,
From equation (i), we find that w, is constant and there-
fore that vf is constant.
Further since — Hsin 0 = Aw,, we obtain Ay = H.
CASE OF TWO EQUAL MOMENTS. 317
_ The condition, Cw, sin 8+ Aa, cos 0 = 0, derived from (ii),
simply expresses the known fact that the angular momentum
- about the line in the plane zOC which is perpendicular to Oz
is zero,
The conclusion is that the angular velocity about OC is
constant, and that the plane zOC revolves with uniform
angular velocity H/A about the axis of resultant angular
momentum Oz.
246. What has been proved of motion about a fixed
point is equally true of the motion of a rigid body relative
to its centre of gravity.
This can be easily illustrated by tossing into the air a
solid body of any symmetrical shape, such as a piece of wood
in the form of a circular cylinder, or in the form of a cir-
cular cone, or any regular prism or regular pyramid, taking
care to give the body rather a rapid rotation about its axis.
In all such cases, in whatever manner the body may be
thrown up, its axis will be seen to describe uniformly a right
circular cone about a line through the centre of gravity the
direction of which remains unchanged.
This line is the axis of the resultant angular momentum
originally imparted to the body.
If the Gyroscope described in Art. (243) be mounted in
a fixed framework so as to give the diameter OC free motion
about the fixed point G, we obtain an apparatus for directly
demonstrating the fact that the earth has a motion of
rotation independently of its motion of translation.
The ring being set rotating with great rapidity, so as to
continue rotating for some hours, it will be seen that its
position relative to the room in which the machine is
situated gradually changes; and, as we know that the
direction of the axis of rotation of the ring does not change,
it follows that the earth itself is in a state of rotation.
247. Euler's Equations. In the case of the motion of a
single rigid body about a fixed point or about its centre of
318 EULER'S EQUATIONS.
gravity, if we take for our moving axes three straight lines
which are always coincident with three given lines in the
body,
0,=0,, 0,=0,, 0,=o%
If further we take these three lines to be principal axes,
h,=Aa,, h,=Bo,, h,=Ca,,
and the equations of motion take the forms
Ao, —(B- C) 0,0, = L,
Bo,—(C— A) o,0,=M,
Co,—(A—B) oo, =N,
which are Euler’s Equations.
Geometrical equations connecting the angular motions about
three moving axes with the motion of the body referred to lines
Jixed in space.
If OA, OB, OC be three lines fixed in the body, and OX,
OY, OZ three lines fixed in space, and if these lines end on
the surface of a sphere, the position of the body will be
completely determined by the quantities , 0, ¢, if
v= CZK, 0=Z0, =ACE.
Zz
Z
Moreover the motion is completely determined by the
rotation @ about OF, the rotation y about OZ and by the
°
IMPULSES. 319
rate of separation d of the plane OCA in the body from the
moving plane ZCE.
This system must be equivalent to the system of angular
rotations w,, ,, and w, about OA, OB and OC.
Expressing this equivalence we obtain,
o, =6cos FA +> cos ZA = 6sin d — sin 0 cos ¢,
w,=6 cos FB+ cos ZB=6cos$+sin O sin d,
w, = cos 0+ d.
These equations may be employed in the discussion of
the general problem of the motion of a rigid body about a
fixed point, :
For this however we refer the student to Poinsot’s
Nouvelle Théorie de ta Rotation des corps solides, to Dr
Routh’s Rigid Dynamics, and other treatises.
248. Impulses. We have given in Arts. (200) and (201),
the principles which determine the effects of impulses, and
the equations for the calculation of those effects.
If smooth inelastic bodies impinge on each other, it must
be carefully borne in mind, that the velocities, immediately
after impact, of the points of the bodies in contact with each
other, are the same in the direction of the common normal
to their surfaces. y
If however two perfectly rough inelastic bodies impinge
‘on each other, the geometrical condition is that the velocities
of the points of contact are the same in any direction.
If when a system is in motion, a straight line in the
system is suddenly fixed, the impulses called into action
have no moment about the line, and consequently the
angular momentum about it remains unchanged.
If a point of the system be suddenly fixed, the change
of motion is determined by the fact that the angular
momentum round any straight line whatever, through the
point, remains unchanged.
320 ILLUSTRATIONS OF WORK.
In the case of a single rigid body, if u, v, w be the
velocities of the centre of gravity, and @,, @,, @, the angular
velocities about principal axes through the centre of gravity,
the changes of these quantities due to impulses whose com-
ponents are P, @, R, and moments, about axes through the
centre of gravity, G, H, K are given by the equations
M(u'—u) =P, M (v1) =Q, Mw'—w) =,
A (w,’—0,)=G, B(w,'—o,) = H, C (a, —@,) = K.
The solution of problems involving impulses may some-
times be facilitated by the use of the principle of virtual
velocities.
For any imagined geometrical displacement the virtual
moment of the changes of linear and angular momenta is
equal to the virtual moment of the applied impulses.
It may be well to notice that if a couple be displaced
about a line parallel to its plane the virtual work is zero, so
that if a couple is displaced about an axis not perpendicular
to its plane, all that is necessary is to find the component of
the couple about the axis of displacement.
The solutions of the two following problems will serve as
further illustrations of the application of the principles of
momentum and energy.
249. A system, consisting of four equal rods forming a
square ABCD, having universal joints at A, B, C and D, is
rotating freely with an angular velocity n about the line EF
joining the middle points of BC' and DA; it is required to
determine the changes of motion produced ‘when the point A
ais suddenly fixed.
In order to mark directions take the axis of z per-
pendicular to the plane of the square, and let @,, @,, @,, @, be
the angular velocities of AB, BC, CD, DA immediately after
A is fixed.
Expressing the fact that the angular momentum of the
ILLUSTRATIONS OF WORK. 321
rods AB, BC about the straight line AC is unchanged, we
obtain
an an
Prag 2 geen
< at % at 2m) rc 53 v2 3y2?
or 5@, +@, = —2n.
D BR a
Me ! Pd
igs ie
‘ i x
MK \ ra
Faas pee eae I a
oe "ee
co ' ah
Bg i “sy
c Ei B
y
Further the angular momenta of ADC about AC, and
of BCD about BD are unchanged, and therefore
264 a(o,+20,) ao, _ an, an
+R 2 ~ 3/2 So fe”
a 4 H% an an
@ (0, + 20,) 5 + 5s ta (0, + 20,) vat 3/2 = 3/72 +»
or 5o,+ 0, = 2n,
3, + 20, + 20, + 30, = 2n.
Further we have the geometrical condition obtained by
equating the two expressions for the velocity of C which is
2aw, + 2aw, = 2aw, + 2aw,
or @, +0, =O, +0,
322 ILLUSTRATIONS OF WORK.
From these equations we find that
Ee ey
If P, Q, R be the impulses at B, C, D, we obtain, by
taking moments about A, B, C, for the rods AB, BC, CD,
Po, + ao, + a’n = 2aP,
a’ (w, + 20,) +k* (w, — n) = 2aQ,.
a? (w, + 20,) —a’n — kw, = 2ak,
and therefore Q = 0, 14P = na, 14R = — na.
Finally the impulse at A which is the change of linear
momentum of the system
= a0, + (ao, + 2aw,) + (aw, + 2aw,) + aw, = $ na.
250. A cube, the edges of which are twelve equal uniform
rods hinged together, is hung up by one corner, the cube form
being maintained by a string joining this corner with the
lowest corner. Itis required to find the initial change of stress
at the point of support when the string is cut.
é. EE
B
The corner O being the point of support and the diagonal
ILLUSTRATIONS OF WORK. 323
OD vertical, it is clear that the initial angular accelerations
of OA, OB, OC will be respectively in the planes AOD,
BOD, COD and will be equal to each other; and further
that the angular accelerations of all the other rods will
be the same and will be, respectively, in parallel planes,
If w represent this initial angular acceleration, 2a, which
we shall call 2f will be the linear acceleration of A in the
direction AD, of B in direction BD, and of C in direction CD.
Taking accelerations parallel to OA, OB, and OC, we
obtain the following forms, where K and JL are the centres of
the rods CE, ED.
The accelerations of Cc are
IV 2, fr/2, 9,
the accelerations of K relative to C are
. 0, v2, f/./2,
of E relative to C,
0, f2, f./2,
and of Z relative to E,
S/V2, 0, f//2.
Therefore the actual accelerations of K are
Iv/2, 3/2, fl’ 2,
8f)/2, 2fr/2, 8f]r/2.
Now suppose a displacement made by slightly increasing
the length of OD, so as to turn every rod through a small
angle 0.
The displacements of the various points follow the law of
the accelerations and are of the same forms, replacing o
by @.
Observing that there are six rods under the same condi-
tions as CEH, three under the same conditions as FD, and
three other rods OA, OB, OC, the equation of virtual
work is
6mfab (2 + $+ 4) + 3mfad (3 +8 + ¥)
2 2
+3m a. wf + 9m i w8 = 12mgabn/6,
21—2
and of Z
324 ILLUSTRATIONS OF WORK.
for the displacement of D is the resultant of the displace-
ments of A, B, and C.
From this equation we obtain
25aw = 3g 1/6,
and since the acceleration of D is 2aw /6, it follows that the
acceleration of G is aw 1/6 and is therefore 189/25.
Hence it follows that the diminution of stress at O is
18/25 of the total weight of the system.
The initial stresses at the several joints can be obtained
by giving independent displacements to the.several rods,
breaking the connections at the different joints.
251. The endeavour of this chapter has been to explain
the use of moving axes, and to illustrate the solution of
problems in three dimensions by the direct application of
fundamental conceptions and of equations derived imme-
diately from these conceptions.
It is hoped that these illustrations will serve as an
introduction to a very extensive field of thought, a field
which has been worked extensively by many mathematicians
with great power and success.
For the more general problems of the motions of solid
bodies on surfaces, for the great problems of Precession and
Nutation, and for the utilization and application of systems
of generalized coordinates, the student will consult such
English works as the Natural Philosophy of Sir William
Thomson and Professor Tait, Dr Routh’s Rigid Dynamics,
and the Treatise on Generalised Coordinates by Dr H. W.
Watson and Mr S. H. Burbury.
The student who has time at his disposal will study the
great works of Laplace and Lagrange, and those works, with
the English Treatises to which we have referred, and the
treatises and papers of Jacobi, Laurent, Bertrand, Resal,
Mathieu and numerous others, offer a vast area for considera-
tion, and suggest unlimited fields of research.
EXAMPLES. 825
EXAMPLES.
1. Two equal smooth circles are fixed so as to touch the
same horizontal plane, their planes being at different inclina-
tions; two small heavy beads are projected at the same
instant along these circles from their lowest points, the
velocity of each bead being that due to the height of the
highest point of the other circle above the horizontal plane,
shew that during the motion the two beads will always be at
equal heights above the horizontal plane.
2. A sphere is projected horizontally on an inclined
plane, the surface of which is perfectly rough; shew that its
centre will describe a parabola.
3. An imperfectly elastic rough sphere is projected
obliquely without rotation against a fixed plane; if 1,7’, be
the angles of incidence and reflection, A the coefficient of
elasticity for direct impact, and p the ratio of the tangential
forces of restitution and compression, prove that
29=5—T7rtanv coti.
4. Two particles of masses m, 2m are fixed to the ends
of a weightless rod of length 2a which is freely moveable
about its middle point. Prove that if @ be the inclination of
the rod to the vertical when the particles are moving with
uniform angular velocity o,
30a cos 0 = g.
5. A solid rectangular parallelepiped with edges of
length a, b, c, is acted on by instantaneous couples with axes
parallel to these edges and of moments proportional to
p:q:7; shew that the direction cosines of the instantaneous
axis of rotation are in the ratio
Oe a
P+ C+a° a+b
326 EXAMPLES.
6. If an octant of an ellipsoid bounded by three principal
planes be rotating about the axis a with angular velocity ,
and if this axis suddenly become free, and the axis 0 fixed,
hew that th lar velocity is "2
shew that the new angular velocity is Fee
7.