CHAPTER XXIX.

A WHIRLING UNIVERSE.

No rest, no quiet, no repose, in that great universe, which to our dim

eyesight looks so fixed and still, but one perpetual rush of moving

suns and worlds. For every star has its own particular motion, every

sun is pressing forward in its own appointed path. And among the

myriads of stars--bright, blazing furnaces of white or golden, red,

blue, or green flame--sweeping with steady rush through space, our sun

also hastens onwards.

The rate of his speed is not very certain, but it is generally believed

to be about one hundred and fifty million miles each year. Possibly he

moves in reality much faster.

When I speak of the sun’s movement, it must of course be understood

that the earth and planets all travel with him, much as a great steamer

on the sea might drag in his wake a number of little boats. From one

of the little boats you could judge of the steamer’s motion quite as

well as if you were on the steamer itself. Astronomers can only judge

of the sun’s motion by watching the seeming backward drift of stars to

the right and left of him; and the watching can be as well accomplished

from earth as from the sun himself.

After all, this mode of judging is, and must be, very uncertain. Among

the millions of stars visible, we only know the real distances of

about twenty-five; and every star has its own real motion, which has to

be separated from the apparent change of position caused by the sun’s

advance.

It seems now pretty clear that the sun’s course is directed towards a

certain point in the constellation Hercules. If the sun’s path were

straight, he might be expected by and by, after long ages, to enter

that constellation. But if orbits of suns, like orbits of planets, are

ellipses, he will curve away sideways long before he reaches Hercules.

[Illustration: HERCULES]

One German astronomer thought he had found the center of the sun’s

orbit. He believed the sun and the stars of the Milky Way to be

traveling round the chief star in the Pleiades, Alcyone. This is

not impossible; but it is now felt that much stronger proof will be

required before the idea can be accepted.

In the last chapter mention was made of star-streams as a late

discovery. Though a discovery still in its infancy, it is one of no

small importance. Briefly stated, the old theory as to the plan of

the Milky Way was as follows: Our sun was a single star among millions

of stars forming the galaxy, some comparatively near, some lying at

distances past human powers of calculation, and all formed upon much

the same model as to size and brightness. Where the band of milky

light showed, stars were believed to extend in countless thousands to

measureless distances. Where dark spaces showed, it was believed that

we looked beyond the limits of our universe into black space. Stars

scattered in other parts of the sky were supposed generally to be

outlying members of the same great Milky Way. Many of the nebulæ and

star-clusters were believed to be vast and distant gatherings of stars,

like the Milky Way itself, but separated by unutterably wide reaches of

space. Some of these views may yet be found to contain truth, though at

the present moment a different theory is afloat.

It is still thought probable that our sun is one among many millions

of suns, forming a vast system or collection of stars, called by

some a universe. It is also thought possible that other such mighty

collections of stars may exist outside and separate from our own at

immense distances. It is thought not impossible or improbable that some

among the nebulæ may be such far-off galaxies of stars; though, on the

other hand, it is felt that every star-cluster and nebula within reach

of man’s sight may form a part of our own “universe.”

According to this view of the question, the Milky Way, instead of

being an enormous universe of countless suns reaching to incalculable

distances, may rather be a vast and mighty star-stream, consisting

of hundreds of brilliant leading suns, intermixed with thousands or

even millions of lesser shining orbs. If this be the true view, the

lesser suns would often be nearer than the greater suns, although more

dim; and the Milky Way would not be itself a universe, though a very

wonderful and beautiful portion of our universe.

Which of these two different theories or opinions contains the most

truth remains to be found out. But respecting the arrangement of

stars into streams, interesting facts have lately been discovered. We

certainly see in the Solar System a tendency of heavenly bodies to

travel in the same lines and in companies. Not to speak of Jupiter and

his moons, or Saturn and his moons, we see it more remarkably in the

hundreds of asteroids pursuing one path, the millions of meteorites

whirling in herds. Would there be anything startling in the same

tendency appearing on a mightier scale? Should we be greatly astonished

to find streams of stars, as well as streams of planets?

For such, indeed, appears to be the case. Separated by abysses of

space, brother suns are plainly to be seen journeying side by side

through the heavens, towards the same goal.

The question of star-drift is too complex and difficult to be gone

into closely in a book of this kind. One example, however, may be

given. Almost everybody knows by sight the constellation of the Great

Bear--the seven principal stars of which are called also Charles’s

Wain, a corruption of the old Gothic _Karl Wagen_, the churl’s or

peasant’s wagon. It is also called the Great Dipper. Four bright stars

form a rough sort of oblong, and from one of the corners three more

bright stars stretch away in a curve, representing the Bear’s tail.

Many smaller stars are intermixed.

[Illustration: THE GREAT BEAR.]

These seven bright stars have always been bound together in men’s

minds, as if they belonged to one another. But who, through the

centuries past, since aught was known of the real distances of the

stars from ourselves and from one another, ever supposed that any among

the seven were _really_ connected together?

One of these seven stars, the middle one in the tail, has a tiny

companion-star, close to it, visible to the naked eye. For a good

while it was uncertain whether the two were a “real double,” or only

a seeming double. In time it became clear that the two did actually

belong to one another.

Mizar is the name of the chief star, and Alcor of the companion. Alcor

is believed to be about three thousand times as far away from Mizar,

as our earth from the sun. Now, if this be the width of space between

those two bright points, lying seemingly so close together as almost to

look to the naked eye like one, what must be the distance between the

seven leading stars of the Great Bear, separated by broad sky-spaces?

Who could imagine that one of these suns had aught to do with the rest?

Yet among other amazing discoveries of late years it has been found by

means of the new instrument, the spectroscope, that _five_ out of these

seven suns are traveling the same journey, with the same speed. Two of

the seven appear to be moving in another direction, but three of the

body-stars and two of the tail-stars are hastening in the direction

away from us, all in the same line of march, all rushing through space

at the rate of twenty miles each second. Some smaller stars close to

them are also moving in the same path. Is not this wonderful? We see

here a vast system of suns, all moving towards one goal, and each

probably bearing with him his own family of worlds.

Many such streams have been noticed, and many more will doubtless be

found. For aught we know, our own sun may be one among such a company

of brother-suns, traveling in company.

It is difficult to give any clear idea of the immensity of the

universe--even of that portion of the universe which lies within reach

of our most powerful telescopes. How far beyond such limits it may

reach, we lose ourselves in imagining.

Earlier in the book we have supposed possible models of the Solar

System, bringing down the sun and worlds to a small size, yet keeping

due proportions. What if we were to attempt to make a reduced model of

the universe; that is of just so much of it as comes within our ken?

Suppose a man were to set himself to form such a model, including

every star which has ever been seen. Let him have one tiny ball for

the sun, and another tiny ball for Alpha Centauri; and let him, as a

beginning, set the two _one yard apart_. That single yard represents

ninety-three millions of miles, two hundred and seventy-five thousand

times repeated. Then let him arrange countless multitudes of other tiny

balls, at due distances--some five times, ten times, twenty times,

fifty times, as far away from the sun as Alpha Centauri.

It is said that the known universe, made upon a model of these

proportions, would be many miles in length and breadth. But the model

would appear fixed as marble. The sizes and distances of the stars

being so enormously reduced, their rates of motion would be lessened

in proportion. Long intervals of time would need to pass before the

faintest motion in one of the millions of tiny balls could become

visible to a human eye.

The story of the sun, moon, and stars · 第 29 / 33 章