CHAPTER III.

WHAT BINDS THE FAMILY TOGETHER?

What is it which binds together all the members of the Solar System?

Ah, what? Why should not the sun at any moment rush away in one

direction, the earth in a second, the planets in half a dozen others?

What is there to hinder such a catastrophe? Nothing--except that

they are all held together by a certain close family tie; or, more

correctly, by the powerful influence of the head of the family.

This mysterious power which the sun has, and which all the planets

have also in their smaller degrees, is called Attraction. Sometimes

it is named Gravitation or Gravity. When we speak, as we often do,

of the _law_ of attraction or gravitation, we mean simply this--that

throughout the universe, in things little and great, is found a certain

wonderful _something_, in constant action, which we call a “law.” What

the “something” may be, man can not tell; for he knows it only by its

effects. But these effects are seen everywhere, on all sides, in the

earth and in the universe. It is well named in being called a “law;”

for we are compelled to obey it. None but the Divine Lawgiver who made

this law can for a single moment suspend its working.

What causes an apple to fall to the ground when it drops from the

branch? Why should it not, instead, rise upwards? Because, of course,

it is heavy, or has weight. But what _is_ weight? Simply this--that

the earth draws or drags everything downwards towards herself by the

power of attraction. Every substance, great or small, light or heavy,

is made up of tiny atoms. Each one of these atoms attracts or draws all

the other atoms towards itself; and the closer they are together, the

more strongly they pull one another.

The atoms in a piece of iron are much closer than the atoms in a piece

of wood; therefore the iron is called the “more _dense_” of the two,

and its weight or “mass” is greater. The more closely the atoms are

pressed together, the greater the number of them in a small space, and

the more strong the drawing towards the earth; for the earth draws each

one of these atoms equally. That is only another way of saying that

a thing is “heavier.” If you drop a stone from the top of a cliff,

will it rise upwards or float in the air? No, indeed. The pull of the

earth’s attraction, dragging and still dragging downward, makes it rush

through the air, with speed quickening each instant, till it strikes

the ground. Every single atom in every single body _pulls_ every other

atom, whether far or near. The nearer it is, the stronger always the

pulling.

We do not always feel this, because the very much greater attraction of

the earth hides--or smothers, as we may say--the lesser attraction of

each small thing for another. But though you and I might stand side by

side upon earth, and feel no mutual attraction, yet if we could mount

up a few thousands of miles, far away from earth, and float in distant

space, there we should find ourselves drawn together, and unable to

remain apart.

Now precisely as an apple falling from a tree and a stone dropping

from a cliff are dragged downward to the earth, just so our earth and

all the planets are dragged downwards towards the sun and towards each

other. The law of the earth’s attraction of all objects on its surface

to itself was indistinctly suspected a very long time ago; but it was

the great Newton who first discovered that this same law was to be

found working among the members of the whole Solar System. The sun

attracts the earth, and the earth attracts the sun. But the enormous

size of the sun compared with our earth--like a great nine-foot globe

beside a tiny one-inch ball--makes our power of attraction to be quite

lost sight of in his, which is so much greater.

The principle of gravitation is of far wider scope than we have yet

indicated. We have spoken merely of the attraction of the earth, and

we have stated that its attraction extends throughout space. But the

law of gravitation is not so limited. Not only does the earth attract

every other body, and every other body attract the earth, but each of

these bodies attracts each other; so that, in its more complete shape,

the law of gravitation announces that “every body in the universe

attracts every other body with a force which varies inversely as the

square of the distance.” It is impossible for us to overestimate the

importance of this law. It supplies the clue by which we can unravel

the complicated movements of the planets. It has led to marvelous

discoveries, in which the law of gravitation has enabled us to

anticipate the telescope, and, indeed, actually to feel the existence

of bodies before those bodies have even been seen.

We come now to another question. If the sun is pulling with such power

at the earth and all her sister planets, why do they not fall down upon

him? What is to prevent their rolling some day into one of those deep

rents in his fiery envelope? Did you ever tie a ball to a string, and

swing it rapidly round and round your head? If you did, you must have

noticed the steady outward pull of the ball. The heavier the ball, and

the more rapid its whirl, the stronger the pull will be. Let the string

slip, and the rush of the ball through the air to the side of the room

will make this yet more plain. Did you ever carry a glass of water

quickly along, and then, on suddenly turning a corner, find that the

water has not turned with you? It has gone on in its former direction,

leaving the glass, and spilling itself on the floor.

The cause in both cases is the same. Here is another “law of nature,”

so-called. Though we can neither explain nor understand why and how

it is so, we see it to be one of the fixed rules of God’s working in

every-day life throughout his universe. The law, as we see it, seems

to be this: Everything which is at rest must remain at rest, until

set moving by some cause outside of, or independent of itself; and

everything which is once set moving, must continue moving in a straight

line until checked.

According to this a cannon-ball lying on the ground ought to remain

there until it is set in motion; and, once set in motion by being fired

from a cannon, it ought to go on forever. Exactly so--if nothing

stops it. But the earth’s attraction draws the cannon-ball downward,

and every time it strikes the ground it is partly checked. Also each

particle of air that touches it helps to bring it to rest. If there

were no earth and no air in the question, the cannon-ball might rush on

in space for thousands of years.

Why did the water get spilled? Because it necessarily continued moving

in a straight line. Your sudden change of direction compelled the solid

glass to make the same change, but the liquid water was free to go

straight on in its former course; so it obeyed this law, and _did_ go

on. Why did the ball pull hard at the string as you swung it round?

Because at each instant it was striving to obey this same law, and to

rush onward in a straight line. The pull of the string was every moment

fighting against that inclination, and forcing the ball to move in a

circle.

Just such is the earth’s movement in her yearly journey round the sun.

The string holding in the ball pictures the sun’s attraction holding

in the earth. The pulling of the ball outward in order to continue

its course in a straight line, pictures the pulling of our earth each

moment to break loose from the sun’s attraction and to flee away into

distant space.

For the earth is not at rest. Each tick of the clock she has sped

onward over more than eighteen miles of her pathway through the sky.

Every instant the sun is dragging, with the tremendous force of his

attraction, to make her fall nearer to him. Every instant the earth is

dragging with the tremendous force of her rapid rush, to get away from

him. These two pullings so far balance each other, or, more strictly,

so far combine together, that between the two she journeys steadily

round and round in her nearly circular orbit.

If the sun pulled a little harder she would need to travel a little

faster, or she would gradually go nearer to him. If the earth went

faster, and the sun’s attraction remained the same as it is now, she

would gradually widen her distance. Indeed, it would only be needful

for the earth to quicken her pace to about five-and-twenty miles a

second, the sun’s power to draw her being unchanged, and she would then

wander away from him for ever. Day by day we on our earth should travel

farther and farther away, leaving behind us all light, all heat, all

life, and finding ourselves slowly lost in darkness, cold, and death.

For what should we do without the sun? All our light, all our warmth,

come from him. Without the sun, life could not exist on the earth.

Plants, herbage, trees, would wither; the waters of rivers, lakes,

oceans, would turn to masses of ice; animals and men would die. Our

earth would soon be one vast, cold, forsaken tomb of darkness and

desolation.

We may not think so, but everything which moves, circulates, and lives

on our planet is the child of the sun. The most nutritious foods come

from the sun. The wood which warms us in winter is, again, the sun in

fragments. Every cubic inch, every pound of wood, is formed by the

power of the sun. The mill which turns under the impulse of wind or

water, revolves only by the sun. And in the black night, under the rain

or snow, the blind and noisy train, which darts like a flying serpent

through the fields, rushes along above the valleys, is swallowed up

under the mountains, goes hissing past the stations, of which the pale

eyes strike silently through the mist,--in the midst of night and cold,

this modern animal, produced by human industry, is still a child of the

sun. The coal from the earth which feeds its stomach is solar work,

stored up during millions of years in the geological strata of the

globe.

As it is certain that the force which sets the watch in motion is

derived from the hand which has wound it, so it is certain that all

terrestrial power proceeds from the sun. It is its heat which maintains

the three states of bodies--solid, liquid, and gaseous. The last

two would vanish, there would be nothing but solids; water and air

itself would be in massive blocks,--if the solar heat did not maintain

them in the fluid state. It is the sun which blows in the air, which

flows in the water, which moans in the tempest, which sings in the

unwearied throat of the nightingale. It attaches to the sides of the

mountains the sources of the rivers and glaciers, and consequently the

cataracts and the avalanches are precipitated with an energy which

they draw directly from him. Thunder and lightning are in their turn

a manifestation of his power. Every fire which burns and every flame

which shines has received its life from the sun. And when two armies

are hurled together with a crash, each charge of cavalry, each shock

between two army corps, is nothing else but the misuse of mechanical

force from the same star. The sun comes to us in the form of heat,

he leaves us in the form of heat; but between his arrival and his

departure, he has given birth to the varied powers of our globe.

I have spoken before about the old-world notion that our earth was a

fixed plain, with the sun circling round her. When the truth dawned

slowly upon some great minds, anxious only to know what really was the

truth, others made a hard struggle for the older and pleasanter mode

of thinking. It went with many sorely against the grain to give up all

idea of the earth being the chief place in the universe. Also there was

something bewildering and dizzying in the notion that our solid world

is never for one moment still. But truth won the victory at last. Men

consented slowly to give up the past dream, and to learn the new lesson

put before them.

We still talk of the sun rising and setting, and of the stars doing the

same. This is, however, merely a common form of speech, which means

just the opposite. For instead of the sun and stars moving, it is the

earth which moves.

The earth has two distinct movements. Indeed, I ought to say that she

has three; but we will leave all thought of the third for the present.

First, she turns round upon her axis once in every twenty-four hours.

Secondly, she travels round the sun once in about every three hundred

and sixty-five days and a quarter. No wonder our ancestors were

startled to learn that the world, which they had counted so immovable,

was perpetually spinning like a humming-top, and rushing through space

like an arrow.

You may gain some clear notions as to the daily rising and setting of

our sun, with the help of an orange. Pass a slender knitting-needle

through the orange, from end to end, and hold it about a yard distant

from a single candle in a room otherwise darkened. Let the needle or

axis slant somewhat, and turn the orange slowly upon it.

The candle does not move; but as the orange turns, the candle-light

falls in succession upon each portion of the yellow rind. Half of the

orange is always in shade, and half is always in light; while at either

side, if a small fly were standing there, he would be passing round out

of shade into candle-light, or out of candle-light into shade.

Each spot on our earth moves round in turn into half-light, full-light,

half-light, and darkness; or, in other words, has morning-dawn,

midday-light, evening twilight, and night. Each spot on our earth would

undergo regularly these changes every twenty-four hours throughout the

year, were it not for another arrangement which so far affects this

that the North and South Poles are, by turns, cut off from the light

during many months together.

Thus the sun is in the center of the Solar System, turning slowly on

his axis; and the earth and the planets travel round him, each spinning

like a teetotum, so as to make the most of his bright warm rays. But

for this spinning movement of the earth, our day and night, instead of

being each a few hours long, would each last six months.

You may notice that, as you turn the orange steadily round, the outside

surface of the skin has to move much more slowly in those parts close

to the knitting-needle, than in those parts which bulge out farthest

from it. Near the North and South Poles the surface of our earth

travels slowly round a very small circle in the course of twenty-four

hours. But at the equator every piece of ground has to travel about

twenty-five thousand miles in the same time; so that it rushes along at

the rate of more than one thousand miles an hour. A man standing on the

earth at the equator is being carried along at this great speed, not

_through_ the air, for the whole atmosphere partakes of the same rapid

motion, but _with_ the air, round and round the earth’s axis.

Now about the other movement of the earth--her yearly journey round the

sun. While she moves, the sun, as seen from the earth, seems to change

his place. First he is observed against a background of one group of

stars, then against a second, then against a third. Not that the stars

are visible in the daytime when the sun is shining, but their places

are well known in the heavens; and also they can be noted very soon

after he sets, or before he rises, so that the constellations nearest

to him may each day be easily found out.

Of course, in old times the sun was thought to be really taking this

journey among the stars, and men talked of “the sun’s path” in the

heavens. This path was named “the Ecliptic,” and we use the word still,

though we know well that the movements are not really his, but ours.

As the earth’s daily movement causes day and night, so the earth’s

yearly movement causes spring, summer, autumn, and winter. A few pages

back I mentioned, in passing, one slight yet important fact which lies

at the root of this matter about the seasons. The earth, journeying

round the sun, travels with her axis _slanting_. Put your candle in the

middle of the table, and stand at one end, holding your orange. Now let

the knitting-needle, with the orange upon it, so slant that one end

shall point straight over the candle, towards the upper part of the

wall at the farther end of the room. Call the upper end so pointing the

North Pole of your orange. You will see that the candle-light falls

chiefly upon the upper half of the orange; and as you turn it slowly,

to picture day and night, you will find that the North Pole has no

night, and the South Pole has no day. That is summer in the northern

hemisphere, and winter in the southern.

Walk round next to one side of the table, towards the right hand,

taking care to let the knitting-needle point steadily still in exactly

the same direction, not towards the same _spot_, for that would alter

its direction as you move, but towards the same _wall_. Stop, and you

will find the candle lighting up one-half of your orange, from the

North to the South Poles. Turn it slowly, never altering the slope of

the axis, and you will see that every part of the orange comes by turns

under the light. This is the Autumnal Equinox, when days and nights all

over the world are equal in length.

Walk on to the other end of the table, still letting the needle slope

and point steadily as before. Now the candle-light will shine upon the

lower or South Pole, and the North Pole will be entirely in the shade.

This is summer in the southern hemisphere, and winter in the northern.

Pass on to the fourth side of the table, and once more you will find

it, as at the second side, equal light from North Pole to South Pole.

This will be the Spring Equinox.

It is an illustration that may be easily practiced. But everything

depends upon keeping the slant of the needle or axis unchanged

throughout. If it be allowed to point first to right, and then to left,

first towards the ceiling, and then towards the wall, the attempt will

prove a failure.

The story of the sun, moon, and stars · 第 3 / 33 章