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^^ 



il GENERAL FOREWORD 

is not necessarily dull or fenced off by a barrier of 
technical jargon. Of course, specialisation in this as in 
other subjects is not for everyone, but the publication of 
this series of books enables any man or woman to learn, 
any child to be taught, to pass with imderstanding and 
safety the *^ Thresholds of Science." 



THSB8E0LD8 OF SCIENCE 



MECHANICS 



THRESHOLDS OF SCIENCE 

Otber Volttinci In Preparation i 
MATHEMATICS hj C A. Laiuuit 
ZOOLOGY by E* Basdket. 

BOTANY by E. Bcocker. 

CHEMISTRY by Geofgei Dar^cna. 



THRESHOLDS OF SCIENCE ' ' " 

^7 

MECHANICS 

BY 

C. E. GUILLAUME 
I 

ILLUSTRATED 

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Garden City New York 

J)OUBLEDAY, PAGE & COMP^Ny 



1915 

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METEIC MEASUEES 



1000 metres 

100 m. 

10 m. 

1 metre 

•1 m. 

•01 m. 

•001 m. 



I 



1000 grammes 
100 g. 
10 g. 



1 gramme 



I 



•Ig. 
•01 g. 

•001 g. 



LENGTH 

1 kilometre = 1093*6 yards 

= about g mile. 
1 hectometre. 
1 decametre. 
39-37 ins. = 109 yard. 
1 decimetre. 
1 centimetre. 
1 millimetre = abont ^ in. 

MASS 

1 kilogramme = about 2 J lbs. 

1 hectogramme. 

1 decagramme. 

weight of 1 c.c! of wat^r at 

4? C. = 16'43 grains = 

•036 oz. 
1 decigramme. 
1 centigramme. 
1 milligramme. 



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£ /&. 



CONTENTS 



PAGB 

General Forewobd to the Sebies • • • i 
Metbic Measures v 



FIRST PART. 

PEEPARATION FOR THE STUDY OP MECHANICS. 

Chapter I. 

HOW TO study nature. 



1. Observation and Experiment 

2. Approximation and Simplification 

3. The Need for Simplification . 

4. Limits of Experiment . 

5. Illusion ..... 

6. Education of the Senses : Measurement 

7. Induction and Deduction • • 



Chapter II. 

MOTION. 



1 
2 

4 
5 
7 
9 
14 



8. How Velocity is Defined 20 

9. Relative and Absolute Velocity . • • • 22 

10. lUusion in the Observation of Motion • • • 25 

11. Distance, Time, Velocity, and Acceleration • • 29 

12. Direction of Velocity. Composition and Resolution 

of Motions ,«.,,,. 34 



VIII 



CONTENTS 



SECOND PART. 



EXPOSITION OF PRINCIPLES. 



CnAPTER III. 

FORCE, THE CAUSE OP ACCELERATION. 

PAGE 

13. Velocity, Accoloration, Force, and Inertia . . 38 

14. Laws of Falling Bodies 42 

16. Doiliiotion from the Laws of Falling. Symbols . 45 

16. Exaggeration of the Disturbing Causes ; their Study 

and Elimination 47 

17. Gonoralisatiou of the Laws of Falling • . .51 



Chapter IV. 



THE WORK OF FORCES. 



18. The Meaning of Work . 

19. Storage and Restitution of Work 
Mass ..... 



20 

21. Kinetic Energy . 

22. Power 

23. Conservation of Work . 

24. Action and Reaction. Momentum 



53 
54 
57 
62 
65 
67 
70 



Chapter V. 



FORCES without MOTION. 

26. Reactions of Matter ; Elasticity and Friction . 74 

26. Forces in Equilibrium ; Composition and Resolution 

of Forces :...... 78 

27. The Law of Attraction ; Weight and Mass . . 85 

28. Couples 92 

29. The Lever 95 

30. Centre of Gravity 98 

31. Pressure •..»•••• 102 



CONTENTS 



ix 



Chaptbb VI. 

REST AND MOTIOK DUB TO FOftCES. 

PAGE 

32. Virtual and Beal Acceleration • • • • 108 

33. The Price of Acceleration . . . • .110 

34. Centripetal Acceleration and Centrifugal Force . 113 

35. Central or Eccentric Percussion ; Reciprocal Centres 120 

36. Moment of Inertia 122 



Chapter VII. 



OSOILLATORT MOTION. 

37. Periodic Forces and Oscillations . 

38. Representation of Oscillatory Motion 

39. Laws of Oscillatory Motion . 

40. The Pendulum and Weight • 

41. Resonance . • • • • 



125 
126 
127 
133 
136 



THIRD PART. 

DEVELOPMENT AND APPLICATION. 



Chapter VIII. 



CALCULATIONS IN MECHANICS. 

42. Qualitative and Quantitative Relations • 

43. Units in Mechanics • • • • 



140 
143 



Chapteb IX. 



impact. 



44. Definition of Impact . 

45. Representation of Elastic Impact 

46. Real Impact 

47. Inelastic Impact . 

48. Forms of Energy. . • 



147 
148 
151 
154 

156 



X CONTENTS 

Chaptxb X. 

RESISTANCE OF MATEBIALS. 

PAGE 

40. Different Properties of Matter . . . .159 
60. Elastic Limit, Breaking Strain, and Modnlna of 

Elasticity 160 

51. The Bending of Bars 162 

62. Fragility, Plasticity, and Hardness . . . 166 

53. Gradual Rupture and Sudden Rupture . . .168 

64. Conservation of Momentum, and Deadening of Shock 171 

65. Speed of Transmission in Sudden Rupture • . 174 



Chapter XI. 

ARTILLERY. 

56. (reneral Conditions in the Firing of a Projectile . 176 

67. Actual Firing 177 

68. Around the Projectile ...... 181 

69. Within the Projectile 184 

60. The Journey from the Earth to the Moon . • .186 

Conclusion 189 

Notes and Problems 191 

Index 196 



xii LIST OF ILLUSTRATIONS 

FTO. PAGE 

23. A shot sent with sufficient speed would travel round 

the earth 88 

24. A ton weighs five kilogrammes more at the pole 

than at the equator 90 

25. A carriage wheel turns because it is under the action 

of a couple 92 

26. The equilibrium of the bar can be brought about in 

many ways ; but always when equal couples are 
opposed at the point of suspension ... 94 

27. In order to balance a couple, a couple of the same 

moment is required . . . . . .96 

28. The lever allows movements to be amplified . . 98 

29. A body supported at its centre of gravity has no 

tendency to rotate 99 

30. The centre of gravity can often be determined geo- 

metrically 100 

31 AND 32. The position of the centre of gravity is some- 
times surprising 101 

33. The pressure on the horizontal bottom of a vessel 

is independent of the shape of the vessel . .104 

34. How centrifugal force is produced . . . .114 

35. Equilibrium of a ball on the surface of a paraboloid 

turning at a suitable speed 117 

36. The projection of rotation gives, the motion of 

oscillation 126 

37. A mass under the action of a force restoring it to its 

position describes an oscillation . • . .128 

38. The most complicated oscillations can be repre- 

sented by the motion of a tooth of a gear- 
wheel . .132 

39. The force that brings the pendulum to its position 

of equilibrium increases more slowly than the 

distance moved 133 

40 AND 41. A spring forces apart two cars running 
towards each other. The diagram of the forces 
acting explains the variations of velocity . .148 

42. In an inelastic impact, the forces during separation 

are less than during the approach . . .154 

43. The shaded areas represent the proportion of work 

recovered in an inelastic impact . • • .155 



LIST OF ILLUSTRATIONS xiii 

PIG. PAGE 

44. A stax made of bread rebounds without being 

deformed . • 159 

45. The mechanical properties of metals can be studied 

by measuring the elongation undergone by A wire 
loaded with a weight 160 

46. Extension and compression 163 

47. In rupture by a falling weight, the wire first absorbs 

the kinetic energy of the fall . . .169 

48. A slow pull breaks the upper wire, a jerk the lower. 

In the first case, the ball acts by its weight ; in 

the second, by its mass 173 

49. The throwing effect and shattering effect depend 

on the development of the pressure in a gun . 179 

50. At the start of a shell the fuse is primed, and on its 

arrival the striker fires the charge . . . 185 



2 MECHANICS 

different routes, because each one is acted upon by forces 
peculiar to itself. 

If we were gifted with a penetration a hundred times 
keener than that of Sherlock Holmes, we might, by dint 
of perseverance, determine the complex forces that each 
stone obeys. But we are naturally dull and slow of 
apprehension ; we must therefore simpUfy our task by 
persuading nature to disclose its secrets. 

For this purpose we must arrange a place where these 
actions can happen in an unusually simple manner. We 
must replace direct observation by a kindred process — 
eayperiment. 

An experiment is a question addressed to nature, which 
is always prepared to answer correctly, if the question is 
correctly put. There will be no false evidence to mislead 
us, no lawyers seeking to prejudice the inquiry. Nature 
discloses itself in all its sincerity, and our art will consist 
merely in asking it a simple question to which it can 
return only a simple answer. 

Replace the mountain-side by a smooth plank, the 
stone by a ball made by a skilful turner, and let the ball 
run down the incUned plank. After our experiment, we 
shall be able to describe very closely not only the path 
that all balls will follow on planks having the same 
incUnation, but other details of their descent ; if our 
observation has been complete, we shall even know the 
moment at which the ball will pass any point on the 
plank, as well as the time occupied in travelling the whole 
length. 

II.— Apppoximation and Simplification. 

Can we describe accurately every feature of the descent 
of the ball ? No ; because the plank is not perfectly 
straight nor the ball perfectly round ; in any other 
experiment both ball and plank would have been different 
in these respects. Yet the plank is much straighter than 



4 MECHANICS 

What we have done is what all men of science do; 
they work as accurately as they can, and interpret the 
result by eUminating the minor interferences that attend it. 

A well-conducted experiment will not then attempt 
an impossible perfection ; it will approach as closely as 
possible ; it will render a single action dominant in such 
a way that the others almost disappear, and subsequent 
reasoning will reject them entirely. 

The details rejected in a first experiment can often be 
examined separately ; thus, in the descent of the ball, 
the undulations are of great interest, for they reveal the 
vibration of the house shaken by movements from the 
street. If these movements of the ground have not, as 
is the case in towns, an artificial origin, they are called 
seismic, and are of extreme importance ; but that is 
another problem, to be approached by other methods. 

It has always been thus. The early naturalists de- 
scribed great animals in their general forms, then others 
examined their anatomy ; next came histologists, who 
examined. their tissues under the microscope ; last of all, 
the study of microbes, of which they are the hosts, has 
concentrated upon the infinitely small the largest amount 
of interest. These are separate problems whose import- 
ance appears successively. The subject is first approached 
by simpHfying, and retaining only the main facts ; then 
little by Uttle, the neglected detail is taken into account. 

III.— The Need for Simplification. 

Whether it is from natural indolence or* from need of 
clearness, the mind prefers what is understood without 
much difficulty and, accordingly, it constantly resorts to 
simplification. When, we say the number of inhabitants of 
France is 39 millions, we knowingly make a mis-statement. 
The truth is that we have not remembered the number of 
inhabitants. By saying 38,893,654 we should perhaps be 
nearer the truth, but that is not certain ; and, given two 



6 MECHANICS 

of otir senses ; they vary with the means adopted fof 
examination. 

An echo is an image of sound as a reflection in a mirror 
is the echo of a face. If the reflection is good it must be 
formed on a surface from which every trace of unevenness 
or irregularity has been removed. An echo, on the 
contrary, is returned by a stretched sheet, by a wall, and 
by a screen of trees — not very distinctly in the case of 
the last, but very clearly in the case of the house, which 
is therefore a very suitable mirror for sound, as it returns 
the image without appreciable distortion. 

Why this difference ? The structure of light is much 
finer than that of sound ; the latter, like the labourer 
with the plank, declares the wall perfectly smooth, while 
the light penetrates and discloses all its irregularities, as 
the laccmaker separates and classifies threads. 

This difference in the nature of hght and sound is 
discernible in all their manifestations ; it enables us to 
hear the words of a person through a wall, while, in order 
to see him, we must be able to look directly at him. 

In studying nature, we must be perfectly aware of the 
degree of dehcacy of our process. Sometimes it has to be 
exact, sometimes it is preferred less exact. Look at a 
good engraving through a lens ; it is easy to distinguish, 
lighter and darker, and separated \>y more or less black, 
all the separate points that constitute the picture ; but 
the picture, though now not so pleasant to look at, will 
not have completely disappeared. Let us now examine 
it under the microscope ; only the points remain, and we 
cannot unite them. Just as trees prevent us from seeing 
the forest, so the points prevent us from seeing the picture. 
Too close an examination exaggerates the detail and leaves 
the whole indistinct. 

The roughness of a process of examination brings about 
that simplification which otherwise our minds would be 
forced to effect. At first glance, the line on the plank 
appeared straight, but close examination proved it not so ; 



\ 



8 MECHANICS 

The inyentor of this inusion desired to deceive our 
sight, and he has completely succeeded ; our eyes in 
turn deceive us, without intending to do so. 

Illusions are found everywhere. ^Vhen, in the six- 
teenth century, the thermometer enabled temperature to 
be determined otherwise than by touching a bodj- with the 
hand, men were astonished to discover that springs are 
colder in winter than in summer, since the evidence of the 
senses had always taught the contrary. The cause of this 
illusion we shall recognise if we plunge the right hand 
into cold water, the left into warm water, and then both 
into tepid water. The water will appear cold to the left 
and warm to the right. 

Bodies of equal weight seem heavier to us in inverse 
proportion to their size. Tlie following experiment is 
always successful. Put upon the hands of a friend a 
cardboard box and a lead ball of equal weight. Ask him 
the question, " How much heavier is the ball than the 
box?*' The reply is generally, "Three or four times." 
We never trust, then, the evidence of our hands if we 
have to buy anything by weight. 

Occupation enables us to forget the passing of time ; 
but when a day has been very full of events, although it 
may have appeared short at the time, the morning seems 
very far off when evening comes. On a journey we often 
confuse yesterday with the day before. 

Waiting makes time seem endless ; the popular expres- 
sion *' I have waited an age for you," is a significant proof. 

The loss of illusions is a cause for regret, and in ordinary 
life we arc happier if we retain some of them. Painters, 
engravers, and all those who present images for our 
enjoyment appeal to our capacity for illusion ; and the 
better they succeed, the more grateful we are. 

When, instead of believing, we wish to know, we must 
rid ourselves of illusions, and try to see things as they 
really are, within the range of power and penetration of 
Qur senses, 



HOW TO STUDY NATURE 19 

By using in turn each method of investigation, we are 
going to form an idea of the laws of Mechanics. The 
experiments we shall make, and the reasoning to which 
we shall submit the causes, would strictly lead to the 
discovery of the facts of the science, if they were not. 
already known. Our sole advantage in working together 
will be like that of a party of tourists, exploring, by the 
aid of a map, a country covered with good roads and with 
a sign-post at every crossing. Having explored this, to 
us, new country, we shall feel a great admiration for the 
pioneers who opened it up and for the engineers who 
mapped it and made the roads. If, further, we succeed 
in knowing it well, we shall have gained, in addition to 
the enjo5'Tnent of the scenery, a facility in finding our 
way in future exploration in a wilder country, where 
the paths are aimless and the heights hidden in mist. 



c^ 



28 MECHANICS 

propagation of sound from A to B. We should therefore 
hear the projectile at D before hearing it at A. It is also 
obvious that the sound from C would reach us after that 
from D. There is accordingly a certain point in the 
trajectory in respect of which sound is first heard ; sounds 
proceeding from any other points of the flight are heard 
subsequent to this. In other words, the projectile seems 
to start its flight from a certain point and to be imme- 
diately divided into two projectiles, which niove, one 
towards the gun, the other towards the target.* 

This example is an indication of the caution ^vith which 
the subject of motion must be approached. We certainly 
shall not err in trusting the evidence of our eyes so lon<][ 
as we are dealing with terrestrial objects, but a like 
affirmation cannot be ventured with regard to celestial 
objects. We believe that we see a star at a definite 
point in the sky ; yet the light from some stars reaches 
us only after many years — hundreds or thousands of 
years. While the light has been travelUng, the earth 
has rotated thousands of times and has travelled thousands 
of millions of miles. The star is then far from the point 
where we judged it to be. 

In addition, a star sometimes appears, shines for 
some time, and then disappears. Thus, on the 21st of 
February, 1901, a splendid and hitherto unknown star 
was observed in the constellation Perseus. It rapidly 
increased in brilliance, then darkened and disappeared. 
The examination that could be made of it during the 
short time it existed was sufficient to allow its distance 
from the earth to be calculated and the time its light 
had required to reach us to be determined It was 
consequently found that, at an immense distance, a fearful 
conflagration had taken place in the middle of the 
sixteenth century. 

* M. Durand-Greville has observed that the explosion 
frequently attributed to aerolites is simply due to an aualogoas 
illusion. 



86 MECHANICS 

Suppose the balloon, instead of moving in a straight line, 
had described a curve. Each part of this line could be 
replaced by its two components, or by its two projections, 
as they are called ; and the motion of the balloon would 
be known by describing the motion of two points simul- 
taneously displaced along the straight lines A'C and 
A'B , so that by drawing from these points the perpen- 
diculars to the two axes the position of the balloon would 
be at their intersection. 

It is somewhat after this manner that the position of a 
warship forcing an entrance into a channel is determined, 
when a mine is to be fired beneath it. Two observers 
on the shore follow the course of the vessel with telescopes ; 
each ascertains one of the projections of its movement, 
and, by prearranged signals, they communicate their 
observations. One of them, in charge of the mines, which 
are exactly marked on a map, traces on the map the course 
of the ship, and when it passes near a mine he causes an 
explosion by means of an electric current. 

Let us watch, from a distance, a wheel turning in the 
horizontal plane and carrying a light. We can see only 
a motion from right to left, and from left to right, rapid in 
the middle of its course, but much slower at the ends; 
that is all our observation reveals, and we are reduced to 
conjecturing the real motion of the light. If another 
observer follows the motion from a point in the plane of 
the wheel, but at right angles to our Une of sight, he will 
see exactly the same movement, except that, when the 
light is at the end of its course for us, it is at the middle 
for him. He will be as incapable of defining its motion 
as we are, for he will have observed only one of its elements. 
Yet, if wc know his observation at every instant, or if he 
knows ours, the position of the luminous point can be 
determined, and hence the circumference that it is 
describing can be constructed. 

We can also measure the distance travelled by the 
luminous point and calculate iU vdooity or acceleri^tiont 



MOTION 87 

In addition, we may consider the motion of the straight 
line joining it to the centre of the circle and describing 
angles. This motion will be known if we can indicate the 
angular velocity, expressed in revolutions per second, or, 
generally, by the quotient of any unit angle divided by 
any unit of time. 

One peculiarity of the observation is noteworthy ; 
while the light moves in a circle with a constant velocity, 
it appears to come and go, to stop and start. For each 
observer the apparent motion is subject to an acceleration, 
sometimes positive, sometimes negative. The uniform 
motion, of which the projection possesses variable velocity, 
is affected by an acceleration of direction, as it is called. 
The importance of this will soon be understood. 

The analogy between an oscillation and a circular motion 
is not as distant as it appears ; it is very close, and we shall 
see later (§ XXXVIII.) that the consideration of oscillation 
as the projection of a uniform circular motion is full of 
consequences. 



SECOND PART 

Exposition of Principles 

CHAPTER III 

FORCE, THE CAUSE OF ACCELERATION 

XIIL— Velocity, Acceleration, Force, and Inertia. 

Experts in the interesting game of bowls always 
choose with the very greatest care the piece of ground on 
which they are to play. They unhesitatingly reject 
ploughed land, and have no liking for gravel. They look 
for a place with- a flat, smooth surface — either sand or 
rolled turf. Ice likewise would not suit them, for, if they 
disregarded the danger of slipping and falling, they would 
experience little pleasure in chasing bowls which a slight 
effort would send rolling undesirabl j distance j over the 
smooth surface. 

Let us follow the movements of the bowl from the 
moment it is taken in hand until it comes to a dead stop at 
the end of its course. The player takes hold of it, throws 
it forward with a swing of his arm, thereby imparting to 
it a certain velocity, and releases it ; it does not fall 
right down at his feet, for it has acquired a new property 
by virtue of which it falls obliquely and then rolls away 
along the surface of the ground. Upon prepared ground 
it rolls a fairly moderate distance ; on ploughed, soft, 
soil, however, it would very quickly come to rest, perhaps 
at its very first contact therewith, or perhaps after re- 
bounding once or twice ; on gravel, the motion would be 



44 



MECHANICS 



The lengths of the successive lines are greater and 
greater, which shows that in equal times the vertical 
distances travelled by the ring in its fall have kept on 
increasing — in other words, its velocity has been increasing. 

If we measure the distances fallen and divide them by 
the distance corresponding to the point 1, we shall find 
that they are represented very nearly by the figures 
4, 9, 16, i.e., the distances fallen are in the ratio of the 
squares of the natural numbers. 

We shall hereafter see that certain causes have con- 
tributed to falsify slightly the result of our experiment. 
Let us disregard them for the moment, and assume that 
the differences between the numbers found and the squares 
of the natural numbers are due to the effect of these 
interfering forces which we have agreed to disregard. 
Let us apply the principle of simpUfication already 
established, and let us accept as a natural law that a body 
falling from rest traverses distances which are as the 
squares of the times the body has been faUing. 

Now set down these numbers. 



Times. 


Heights. 


First differences 
(average velocities.) 


Second differences 
(average accelera- 
tions.) 




1 

2 
3 
4 
5 




1 

4 

9 

16 

25 


1 

3 
6 

7 
9 


2 
2 
2 
2 



The differences between the distances traversed in 
successive equal periods of time are proportional to the 
average velocities during these periods. These velocities 
are represented by the series of odd numbers. 

The differences between these average velocities are aU 
represented by the number 2. Thus we can assert that 
the average acceleration is constant. 



46 MECHANICS 

of each of the velocities and the time during which it 
lasted. In the present instance, it cannot properly be 
said that any single velocity lasts any time, because it is 
continually changing. But the time can be conceived as 
divided infinitesimally, and then the velocities can be 
multiplied by the periods of time. The product will be 

the area of the triangle OCt, which is equal to — , and 
as » = flrf, this area {i.e., the distance traversed) is given 
by -0-. The course of the body can be represented by 

the curve OP, which is that of a parabola. 

In the special case of falling bodies, it has been cus- 
tomary to denote acceleration by the letter g. 

The three laws applicable to freely falling bodies can 
be written do\vn thus : — 

Constant acceleration . . . , . . = g 

Velocity varying as time . . . . v = gt 

Distance traversed var3dng as the ^ 

square of the time . . . . . • ^ = ^ 

In order to discover the laws associated with falling 
bodies, we have had recourse to a series of symbols. We 
have represented time graphically in such a way as to 
convey a meaning to our mind. Such a mode of repre- 
sentation is not unfamiliar. The hand of a clock indicates 
time by the distance it has travelled ; the angle which it 
describes measures the time, the rotation of the earth 
furnishing the unit. 

We can equally well employ a symbol to represent an 
acceleration, a velocity, or a distance. In fact, we find 
that in the third diagram a distance has been represented 
by another distance ; this is quite permissible. We have 
only represented a relatively long line by a short line. 
This is the method adopted in drawing maps. 

We could have given a more striking example of the 
parabola; it is met with continually in innumerable 



52 MECHANICS 

figure, though a very small addition to the weights in the 
pan had visibly stretched the spring. We conclude that, 
within the Umits of our movements and measurements, 
which are at least as exact as those in the experiment 
on the fall of the ring, the force exerted by the weight on 
its support is the same ; the ring therefore possessed the 
same weight throughout the whole extent of its fall, i.e,, 
it exerted upon itself a constant force. We can then give 
our result in the following more general form : — 

A body acted upon by a constant force possesses a constant 
acceleration and a velocity proportional to the duration of 
application of the force ; it describes a distance which, 
calculated from the position of rest, is proportional to the 
square of the time during which the force acts. 

This law must be remembered, for it is fundamental 
and is encountered everywhere. 

It was useful to make by means of the spring a pre- 
liminary survey of the field of force in which we operate. 
If the scale-pan had carried a piece of iron into the neigh- 
bourhood of a powerful magnet, we should have found 
that neither the force nor the acceleration was constant. 
The magnet would have been one of the accidental com- 
plications mentioned in our first experiment, and would 
have had to be eliminated. Fortunately for the discovery 
of mechanical laws, powerful magnets are rare and of 
modern invention ; moreover, all bodies do not possess 
the properties of iron. If magnets had long been of 
common use, and if many substances were magnetic, the 
fundamental laws would perhaps be unknown even now. 



70 MECHANICS 

a person weigh when he jumps ? " " It depends," we 
shall reply. Yes, it depends on many causes. The work 
of his fall must be equalised by work done at the 
moment he touches the ground. If the ground is soft, he 
can alight as he pleases ; the work will be met by the 
force between his feet and the ground ; but, if he lands 
on hard ground, he must use up the work on his muscles 
by relaxing his knees and all other joints. If he 
omits to do so, he is subjected to forces that operate over 
such a very short distance, that they may be great enough 
to break has bones. This explains why a man on skis, 
relying too much on th 3 ela ticity of his fall, may be left 
on the frozen snow with a broken leg. 

Here, again, the skill of the packer is great. Though 
he exerts a great force on the head of a nail, he must, 
on the other hand, protect fragile objects from the effects 
of force while on their journey, no great care being taken, 
at stations and wharves, even if the cases are marked 
" fragile." When a case falls heavily, its Contents acquire 
work and velocity. They lose the latter by giving up 
their work ; to avoid violent forces, the work must 
be done over a sufficiently great distance. Hence the 
need for the elasticity of the shavings, etc., used in 
packing. 

In order to understand thoroughly what happens in 
consequence of a shock, certain properties of matter must 
be known. Before undertaking the study of this subject, 
we have first to work through a wide field. 



XXIV.— Action and Reaction. Momentum. 

Watch a bird fly from the end of a flexible twig ; it 
bends its legs under it, extends them suddenly, and takes 
to the wing. At this instant pay attention to the twig ; 
it will be seen to move quickly backwards, and, after 
some oscillations, to return to its normal position. 

Why does this twig do this ? Obviously because the 



TS MECHANICS 

These equal impnbes can be compaied with another 
product. 

We have seen that the forec/is the prodinrt of mass m 
and acceleration a, Le, — 

/= win. 

Elsewhere, we saw that vdocity rs tiie piodact of 
acceleration and time — 

at = v^ 

Multiplying these two equations^ we have 

ft = mr. 

The product of the mass and velocity of the diot ought 
then to be the same as for the gun, no other force having 
acted. The action of the gases preponderates to such a 
degree, during the very short time ctf the firing of the gun 
(about the one hundredth of a second), that the state- 
ment is very nearly correct for the instant the shot leaves 
the gun. We are not concerned with what happens after 
the projectile begins to travel in the air. 

The velocities are in opposite directions; and, if we 
agree to give a positive sign to one directi<Mi, the other 
is consequently negative, and the algebraic sum of the 
products is zero. 

Now imagine the gun placed in the forward turret of 
an ironclad, which is firing directly forward. To an 
observer in the turret, the conditions are the same as in 
the preceding experiment. But an observer of the 
motions from the shore would have to add the velocity 
of the vessel to each velocity measured by the observer in 
the turret. As the result of calculation, it would be 
found that after, as before firing, the sum of the products 
of the masses and their various velocities would be equal 
to the sum of the masses multiplied by the velocity of 
the vessel. 

Descartes called the product of mass and its velocity 
qtumliiy of motion^ i.e., momentum. Our experiment, as 
well as any other we may do, proves that the momentum of 
a number of masses acting upon each other^ xoithout inter^ 



THE WORK OF FORCES 78 

ference from any external force^ is constant. This is the 
principle of conservation of momentum.* 

Thus a body cannot be displaced by internal force, 
alone. A man seated in a boat or a carriage cannot put 
it in motion without an external point to which to apply 
his force. He can make a light boat move alternately 
backward and forward by moving to and fro. When he 
has a velocity, the boat has ; when he stops, it stops ; 
when he sits down, it resumes its original position. To 
displace it, some external force must act — pressure on the 
water, the pull of a rope, or the action of the wind. The 
same conditions apply to a leap from a boat to the bank. 
If any one' tries it, he will see that the boat is indeed 
driven back, because, having lost its load, it is changed ; 
so is he, for he will have fallen into the water. 

We shall meet applications of the principle just 
explained ; but we must now try to discover how a state 
of rest is brought about, since forces seem always to 
produce motion. 

* " Although motion is only a condition of matter which is 
moved, there is nevertheless a fixed quantity of it that never 
increases or diminishes, even if there is sometimes more and 
sometimes less in certain parts." — ^Descabtes 2 " Principles 
of PhHosophy," 1644. 



CHAPTER V 

FORCES WITHOUT MOTION 

XXV,— Reactions of Matter ; Elasticity and Friction. 

Forces do not always produce motion. Innumerable 
objects around us are under the action of forces and yet 
they do not move. Books on the shelf, an inkstand on 
the table, and the table resting on the floor are all sub- 
jected to a force — their weight ; but at the point where 
each object rests is developed an antagonistic force 
(reaction) which exactly counteracts the action of the 
weight. The principle of equality of action and reaction, 
already recognised in the case of bodies in motion, is true 
for bodies at rest. We should have readily said that the 
principle would be applicable, a fortiori^ if one of them 
could be more true than the other. In reaUty, they are 
equally true, but the reaction of a support on a body at 
rest. is not so apparent as the reaction of an object free 
to move under a force exerted by another object. 

Any one going out on a frosty day and observing the 
difficulty of keeping his feet must have been forcibly 
reminded of that property of the ground whereby he 
is enabled to maintain an upright position without great 
effort. The same idea may have come to him when his 
bicycle has slipped on wet paving or when he has seen a 
cab-horse fall on an asphalt road. He may have seen, 
too, some kind-hearted person throw a shovelful of cinders 
under the animal's feet, with the result that its hoofs 
gripped the ground and it could rise. 

In consequence of these examples, it is easy to realise 
bow much we owe to the beneficent action of friction. 



8g MECHANICS 

in the conditions ; so long as the trajectory was entirely 
within a space in which the verticals could be considered 
parallel, the curve was a parabola. Then its shape changed 
as the lines of action of its weight included greater and 
greater angles ; finally, when the velocity was such that 
the variation in the direction of the trajectory was 
equivalent to the variation in the direction of the weight, 
the trajectory cut at right angles the perpendiculars 
from the places passed, i.e., it was horizontal at every 



point. By an exact adjustment of acceleration and 
tendency to travel away in a straight line, a shot sent 
horizontally could maintain a horizontal trajectory, and 
continue round the earth indefinitely. A speed of a little 
over 5 miles per second would be necessary — seven 
times greater than that of the fastest projectiles— but 
much less than that of certain meteorites that, crossing 
the orbit of the earth, deviate from their way and continue 
their course through space. Those of the meteorites that 
eDt«i the atmosphere lose velocity, become heated, and 



92 MECHANICS 

like its colour ; a definition of mass in terms of weight 
would seem as artificial as that of a crab in an old 
dictionary of the French Academy : — " Small red fish that 
walks backwards." 

The idea that mass is the quotient of weight by accelera- 
tion leads to strange errors. 

Some years ago an engineer, who had remembered 
only the formulae of Mechanics, developed the following 
theory : — A balloon in equilibrium in the air weighs 
nothing ; its weight being nothing, so is its mass ; if it 

has no mass, --— = 0, whatever its speed ; therefore a 

dirigible balloon can have no kinetic energy ; it cannot 
maintain its motion, even for an infinitely short time, 
and, if it is to be kept moving, it must be constantly 
propelled. 

True, it could be given a velocity without any effort 
at all. But the engineer had not drawn this last con- 
clusion ; he had gone no further than to condemn the 
balloon for the former reason. Apparently he did not 
know that, from time to time, a balloon knocks down a 
chimney or breaks a branch off a tree. 

XXVIII.— Couples. 

Have you ever wondered why the wheels of a carriage 
turn round ? The horses draw on the traces (automobiles 

are quite different), and the force 
is transmitted to the axles, which 
draw the wheels forward ; but 
these are on the ground and, as 
we have seen, are kept in place 
by friction. The two forces AB, 
CD (Fig. 25) are not directly 
i<w^ opposite ; one acts on the hub. 
^ . the other on the rim. Whenever 

'^""s recauJ^tf^^der ^^^^^ ^^ ^he case, the object on which 
the action of a couple, the forces act begins to rotate. 




\% 



MVvllVW^i 






^ X \ \\ 



1 



::?n of the 


: : r>? in 


:_■-.: even 


_: ~.}.y be 


_ r ■. .J 






'l' 



r > • I. 



•w - r^- 



104 MECHANICS 

and continued as a thin tube. If the liquid rises to the 
same height as in the cyUndrical vessel, that part of the 
bottom vertically below the tube will support the same 
force as before, for the tube can be supposed produced 
to the bottom so as to isolate a small column of liquid. 
In reality, the surrounding liquid forms the walls of this 
extension of the tube ; and in the neighbourhood of the 
bottom, the hquid is pressed as if at the bottom. If it 
is not to escape, the surrounding Uquid must support it 
with the same force, which is communicated to the sides 
and the whole of the bottom. The vessel might be made 

very flat and surmounted by a very 
high tube. The bottom would then be 
under a great force, produced by a 
small amount of hquid. This invari- 
[^ able condition is so incredible that it 
has been given the name of the 
hydrostatic paradox. 

If the bottom of the vessel supports 

Pjq 33 ^he pres- such a force, ought it not to be very 

sure on the hori- heavy, and would not a balance show 
zontal bottom of a a weight greater than that of the vessel 

denTof \he sTJe ^^^ ^^^^^ together ? The difficulty is 

of the vessel. easily solved ; the Uquid, under pres- 

sure in all directions, is held with equal 
force against the dome of the vessel, and exerts as much 
pressure on it upwards as it exerts on the bottom down- 
wards, the small surface of the tube excepted. If the 
dome is pierced, the water escapes in a strong jet. 

This fact can be expressed by saying that the pressure 
at any point whatever in a hquid depends only on the 
height of the column above it, and not on the section. 

However small the fissures in rock, water succeeds 
in penetrating, and the further it descends the more 
easily it makes a way, for it is under pressure from the 
whole column. This is why the cutting of tunnels such 
as the Simplon is so difficult. When the tunnel is under 




114 



MECHANICS 




acceleraiian^ and will exercise upon the string an outward 

force the stronger as the ball is turned 
^ the more rapidly. This is the force 
called centrifugal force. 

We have seen (§ XXVII.) a similar 
rotation, on a vast scale, in the move- 
ment of stars in a planetary system ; by 
resuming this problem, we shall lean 
how to calculate the value of centri- 
fugal force. 

Consider, for example (Fig. 84), the 
rotation of the moon round the earth. 
E If the moon were free, it would travel 
Pig. 34.— How cen- away in a straight line MA ; but, in 

SSSd ^""^"^ ^ ""^^^^^ '^ trajectory is inclined 

towards B. For a very short time, 
during which the straight lines joining the centre of the 
moon and the earth may be taken as parallel, the laws of 
falling may be applied to the motion of the moon ; if its 
acceleration is a, the distance it will travel towards tie 

earth will be — , after a time t. The mass of the moon 

being m, the force to produce the supposed accderation 
is ma. 

Now, the theorem of Pythagoras enables us to write 



EM2 + Mm2 = Em2 = (EM + nmy^ 
or, substituting r for EM and v for the velocity of the 



moon, 



r2 + (i;^^ = {r +^y. 



Suppressing r\ this reduces to v-i^ = raP + ??r. 

Since t is extremely short, f* is extremely small; B 
can therefore be neglected, giving 



v-v = raP, or v^ = ra. 



2 — 



188 MECHANICS 

to produce real resonance. It is \viser to break up the 
impulses whenever possible ; for this reason the order is 
always given to troops passing over a suspension bridge 
to break step and to walk like a flock of sheep. It is a 
wise precaution, suggested by the catastrophe at Angers. 

The effects of resonance would be disastrous more 
often, if a closely associated action did not always interfere 
and restrict it ; this is the limiting action of friction and 
all the other causes that consume kinetic energy. The 
consumption increases with the amplitude of the motion, 
and finally equals the energy of the impulse ; at this stage 
the oscillation has reached its maximum value. The 
difficulty is to determine whether this value is below that 
of the dangerous amplitude ; if not, the limiting action 
must be increased, or the period of oscillation either of 
the moving body or of the exciting cause must be altered. 
This process is well known to engineers, who frequently 
make use of it. 

The tenor Tamburini used to cause a cut glass vessel 
to break in pieces, by giving loudly the note corresponding 
with its natural vibration. The vibration, stimulated by 
the sound waves, gradually increased and exceeded the 
hmit of deformation that cut glass can bear. It would 
have been enough to touch the rim with a feather to 
prevent the vibration from reaching the dangerous limit, 
and even to restrict it to a very small amplitude. 

Thus, in turn, we utilise or avoid resonance. The 
commonest example of sustained resonance is furnished 
by the regulator of clocks and watches ; the shock induced 
by the oscillating part itself restores to it the energy that 
it has expended in overcoming the resistance of the air 
and in moving the wheels. 



THIRD PART 

Development and Application 

Although, in our rapid survey of the principles of 
Mechanics, we have always had every-day occurrences 
to impress upon us the reaUty of these principles, we have 
regarded them so far in a somewhat limited way, in 
consequence of our having selected for special attention 
only certain aspects of the facts under examination. We 
have now to undertake more complex problems in which 
various principles contribute to produce the effect we are 
studying. Thus we shall grasp more fully their co- 
ordination and relation, and after solving some problems 
we shall be better prepared to apply the knowledge we 
have gained. These problems will no longer be of a 
general kind ; they will have reference to particular cases 
and will give numerical results. We must first, therefore, 
become acquainted with the units in whicli all the 
quantities that come within the domain of Mechanics 
are expressed. 



146 



MECHANICS 



century ago, Laplace proposed to use as the unit of pressure 
the mean pressure of the atmosphere at sea-level ; this 
is called an atmosphere^ and is defined by a column of 
mercury 76 centimetres high. The distribution of 1 
kilogramme-force on 1 square centimetre gives a third 
unit of pressure which is much used in industry. 

The numerical relations of the dynamic units are 
summarised below. 



Force: 
Work: 

Power : 



1 kilogramme-force 
kjlog] 
joule 

1 poncelet 



( 1 kjlogrammetre 

( 1 jor 



^— - [ \ ssr '^"*/^"" 



0*981 megadyne. 
9*81 joules. 

1 megadyne-decimetre. 
100 lalogrammetres per 

second. 
0-981 kilowatt. 
0*981 megabar. 
1*013 megabar. 



150 MECHANICS 

The result, though surprising, is correct ; the velocities 
are exchanged. 

The theory of impact seemed so incredible to those 
who established it, that the celebrated Huyghens, in order 
to realise this exchange of velocities, utilised the very 
elementary experiment that we have just performed. 

We can arrive at this result by considering the work 
done by the spring on the two cars. 

The spring is compressed until the moment when the 
two velocities are equal, i.^., until the cars are at relative 
rest. In accordance with the principle of conservation 
of momentum, the common velocity will be half the 
initial velocity of the left-hand car. The momentum 
before the impact was 

m,2v + m.O = 2mv, 
At the middle of the impact it is 

2m X common velocity = 2nvo. 

Therefore the common velocity is = ». 

The work of the spring having given the right-hand 
car a velocity u, the same amount of work done in the 
opposite direction (areas APP' and BQQ') will destroy 
the velocity of the left car. 

We could have given the two cars any velocity what- 
ever ; the two methods we have used would have led to 
this final result : When two equal mousses meet in an elastic 
impacty they exchange their velocities. 

If the masses are unequal, it is evident that there can 
be no exchange. A shell striking an armour-plate does 
not, fortunately, communicate to it its own velocity. We 
could easily discover formulae suitable for that case ; but 
the time so spent could be more usefully employed ; it 
will be enough to indicate the method. We should first 
say that the momentum of the two masses together 
remains constant ; then we should imagine we were on 
one of the moving bodies against which the other is to 
strike, such as a rubber ball against a wail. The velocity 



170 MECHANICS 

It is interesting to notice that the static rupture of the 
rubber was brought about by one seventy-fifth of the 
weight required for the steel ; but the energy necessary 
for sudden rupture was seven times as much; according to 
our method of estimating the relative merits of steel 
and rubber, we can express them by numbers whose 
ratios will vary from about 1 to 500. This example 
makes it plain that the method of testing materials ought 
to be perfectly definite, if any significance whatever is 
to be attached to the numbers that indicate their qualities. 

We shall understand, too, without its being emphasised, 
that the steel would have resisted the shock much better 
if it had been fastened to its support by a piece of rubber. 
In order to withstand the static weight, this would have 
had to be of large section ; but it would have served to 
nullify the energy of the falUng weight in the second 
experiment, and would have prevented rupture. 

For a static weight, the breaking stress is obviously 
almost independent of the length of the wire. It would 
be absolutely independent if the wire were weightless, and 
if it were quite homogeneous ; the longer it is, the greater 
probability there is of a weak part whose breaking strain is 
a little less than that of the average of the other sections. 
The wire withstands a falling weight all the better if it is 
long, for the quantity of kinetic energy that it can reduce 
to the potential form is proportional to its length. 

Let us now take an extreme case. A very short wire 
ought to be broken by the energy of a very slight shock. 
If we reduce the wire to a length of 1 millimetre, it ought 
to be enough to allow a weight of 100 grammes to fall 
from a height of about '8 milUmetre. But an experiment 
would not confirm this apparently accurate result. The 
reason is that the deformation of the clamps in contact 
with the wire could no longer be neglected ; all these 
deformations transform kinetic energy into potential 
energy, and assist the wire to bear the stress. 

Our young pupils will draw from these remarks all the 



mCEGyHES 

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INDEX 



199 



Time, 29 

of pendulum - swing, 

134, 135 
measurement of, 11, 12 
unit of, 143 

Units, 143 
Upward direction, 86 

Velocity, 29, 38, 45 
absolute, 22 
angular, 37, 124 
average, 21, 29 
definition of, 20 
direction of, 34 
instantaneous, 21^ 

29 
relative, 22 
unit of, 144 



Vertical, illusion of the, 86, 

108, 116 
Vibration, 125, 137 
Virtual acceleration, 108, 112 
von Guericke, Otto, 50 



Wab of Secession, 167, 186 

Watt, 145 

Weight, 51, 111, 133, 135 

and mass, 61, 64, 91, 
173 

Work, 53, 54, 63, 106 

capacity for, 57, 61 
conservation of, 67 
definition of, 54 
restitution of, 54 
storage of, 54 
unit of» 145 



The Country Life Press, Gardkn City. N. Y. 




THB COUNTRY UFE 
GARDEN aTY, N.T. 



•* 

Op^