CHAPTER I.

[Illustration: HIPPARCHUS IN THE OBSERVATORY OF ALEXANDRIA.]

THE STORY

OF THE

SUN, MOON, AND STARS

BY

AGNES GIBERNE

AUTHOR OF “THE STARRY SKIES,” “THE WORLD’S FOUNDATIONS,”

“RADIANT SUNS,” ETC.

[Illustration]

WITH COPIOUS ADDITIONS

Fully Illustrated

CINCINNATI

NATIONAL BOOK COMPANY

COPYRIGHT, 1898,

BY J. T. JONES.

INTRODUCTION.

BY CHARLES PRITCHARD, M. A., F. R. S.,

PROFESSOR OF ASTRONOMY IN THE UNIVERSITY OF OXFORD.

The pages of this volume on a great subject were submitted to my

criticism while passing through the press, with a request from a friend

that I would make any suggestions which might occur to me for its

improvement. Naturally, such a request was entertained, in the first

instance, with hesitation and misgiving. But after a rapid perusal

of the first sheet, I found my interest awakened, and then gradually

secured; for the book seemed to me to possess certain features of

no ordinary character, and, in my judgment, held out the promise of

supplying an undoubted want, thus enabling me to answer a question

which I have been often asked, and which had as often puzzled me,

to the effect, “Can you tell me of any book on astronomy suited to

beginners?” I think just such a book is here presented to the reader;

for the tale of the stellar universe is therein told with great

simplicity, and perhaps with sufficient completeness, in an earnest and

pleasant style, equally free, I think, from inaccuracy or unpardonable

exaggeration. We have here the outlines of elementary astronomy,

not merely detailed without mathematics, but to a very great extent

expressed in untechnical language. Success in such an attempt I regard

as a considerable feat, and one of much practical utility.

For the science of astronomy is essentially a science of great

magnitude and great difficulty. From the time of Hipparchus, some

century and a half before the Christian era, down to the present

day, the cultivation of astronomy has severely taxed the minds of a

succession of men endowed with the rarest genius. The facts and the

truths of the science thus secured have been of very slow accretion;

but like all other truths, when once secured and thoroughly understood,

they are found to admit of very simple verbal expression, and to lie

well within the general comprehension, and, I may safely add, within

the sympathies of all educated men and women.

Thus the great astronomers, the original discoverers of the last

twenty centuries, have labored, each in his separate field of the

vast universe of nature, and other men, endowed with other gifts,

have entered on their labors, and by systematizing, correlating, and

simplifying the expression of their results, have brought the whole

within the grasp of cultivated men engaged in other branches of the

varied pursuits of our complicated life. It is in this sort of order

that the amelioration and civilization of mankind have proceeded, and

at the present moment are, I hope and believe, rapidly proceeding.

It was, I suspect, under this point of view, though half unconsciously

so, that my attention was arrested by the book now presented to the

reader; for we have here many of the chief results of the laborious

researches of such men as Ptolemy, Kepler, Newton, Herschel,

Fraunhofer, Janssen, Lockyer, Schiaparelli, and others--no matter

where accumulated or by whom recorded--filtered through the mind of

a thoughtful and cultured lady, and here presented to other minds in

the very forms wherein they have been assimilated and pictured in her

own. And these forms and pictures are true. It is in this way that the

intellectual “protoplasm” of the human mind is fostered and practically

disseminated.

And, then, there is still another point of view from which this general

dissemination of great truths in a simple style assumes an aspect of

practical importance. I allude to the influences of this process on the

imaginative or poetic side of our complex nature.

Wordsworth, in one of his prefaces, has stated so clearly the truth

on this subject that I can not do better than give his words. “If the

time should ever come,” he says, “when what is now science becomes

familiarized to men, then the remotest discoveries of the chemist, the

botanist, the mineralogist, will be as proper objects of the poet’s

art as any upon which it can be employed. He will be ready to follow

the steps of the man of science; he will be at his side, carrying

sensation into the midst of the objects of science itself. The poet

will lend his divine spirit to aid the transfiguration, and will

welcome the being thus produced as a dear and genuine inmate of the

household of man.”

It is for reasons such as here stated that I heartily commend this

book to the attention of those who take an interest in the advancement

of the intellectual progress and culture of society. The story of the

Kosmos is told by the authoress in her own language and after her own

method. I believe, as I have said, the story is correct.

OXFORD UNIVERSITY.

CONTENTS.

CHAPTER. PAGE.

I. THE EARTH ONE OF A FAMILY, 13

II. THE HEAD OF OUR FAMILY, 24

III. WHAT BINDS THE FAMILY TOGETHER, 34

IV. THE LEADING MEMBERS OF OUR FAMILY.--FIRST

GROUP, 46

V. THE LEADING MEMBERS OF OUR FAMILY.--SECOND

GROUP, 55

VI. THE MOON, 62

VII. VISITORS, 73

VIII. LITTLE SERVANTS, 83

IX. NEIGHBORING FAMILIES, 95

X. OUR NEIGHBORS’ MOVEMENTS, 106

XI. MORE ABOUT THE SOLAR SYSTEM, 122

XII. MORE ABOUT THE SUN, 133

XIII. YET MORE ABOUT THE SUN, 148

XIV. MORE ABOUT THE MOON, 157

XV. YET MORE ABOUT THE MOON, 164

XVI. MERCURY, VENUS, AND MARS, 180

XVII. JUPITER, 199

XVIII. SATURN, 214

XIX. URANUS AND NEPTUNE, 225

XX. COMETS AND METEORITES, 240

XXI. MORE ABOUT COMETS AND METEORITES, 246

XXII. MANY SUNS, 267

XXIII. SOME PARTICULAR SUNS, 278

XXIV. DIFFERENT KINDS OF SUNS, 291

XXV. GROUPS AND CLUSTERS OF SUNS, 304

XXVI. THE PROBLEM OF SUN AND STAR DISTANCES, 310

XXVII. MEASUREMENT OF STAR DISTANCES, 320

XXVIII. THE MILKY WAY, 329

XXIX. A WHIRLING UNIVERSE, 337

XXX. READING THE LIGHT, 344

XXXI. STELLAR PHOTOGRAPHY, 355

XXXII. THE DAWN OF ASTRONOMY, 363

XXXIII. MODERN ASTRONOMY, 375

XXXIV. SIR ISAAC NEWTON, 382

XXXV. LATER ASTRONOMY, 393

LIST OF ILLUSTRATIONS.

PAGE.

Hipparchus in the Observatory at Alexandria _Frontispiece._

The Solar System 15

The Pleiades 19

Sun-spots 29

Phases of Mercury before Inferior Conjunction--Evening Star 50

Appearance of the Full Moon 63

One Form of Lunar Crater 69

The Earth as Seen from the Moon 71

Passage of the Earth and the Moon through the Tail of a Comet 76

Passage of the Comet of 1843 Close to the Sun 79

Meteor Emerging from Behind a Cloud 84

The Great Shower of Shooting-stars, November 27, 1872 90

Constellation of the Great Bear 108

The Great Bear 50,000 Years Ago 109

The Great Bear 50,000 Years Hence 109

Constellation of Orion as it Appears Now 110

Constellation of Orion 50,000 Years Hence 111

Position of Planets Inferior to Jupiter--Showing the Zone of the

Asteroids 123

Comparative Size of the Planetary Worlds 130

A Typical Sun-spot 135

A Solar Eruption 138

Sun-flames, May 3, 1892 143

Solar Corona and Prominence 152

Comparative Size of the Earth and Sun 155

The Moon--an Expired Planet 159

The Lunar Crater Copernicus 170

Lunar Eruption--Brisk Action 172

Lunar Eruption--Feeble Action 173

Nicolaus Copernicus 176

Phases of Venus 186

Mars and the Path of its Satellites 191

General Aspect of Jupiter--Satellite and its Shadow 200

Satellites of Jupiter Compared with the Earth and Moon 206

The System of Jupiter 208

Orbits of Nine Comets Captured by Jupiter 213

Saturn and the Earth--Comparative Size 215

Ideal View of Saturn’s Rings and Satellites from the Planet 222

Great Astronomers of Earlier Times 227

The Great Comet of 1811 247

Donati’s Comet, 1858 249

Great Comet of 1744 254

The First Comet of 1888--June 4 255

Great Comet of 1680 260

Great Comet of 1769 261

Baron Alexander Von Humboldt 264

A Telescopic Field in the Milky Way 270

Cygnus, Constellation of 279

Stars whose Distances are Best Known 281

Lyra, Constellation of 297

Constellations in the Northern Hemisphere 300

A Cluster of Stars in Centaurus 305

The Great Nebula in Andromeda, Compared with Size of the Solar

System 307

A Cluster of Stars in Perseus 332

Hercules, Constellation of 338

The Great Bear, Constellation of 341

The Prism and Spectrum 344

The Spectroscope 345

Spectra, Showing the Dark Lines 347

Great Astronomers of Later Times 377

Sir Isaac Newton 386

Eye-piece of Lick Telescope 407

Lick Observatory 409

Professor E. E. Barnard 410

THE STORY

OF THE

SUN, MOON, AND STARS.

CHAPTER I.

THE EARTH ONE OF A FAMILY.

What is this earth of ours?

Something very great--and yet something very little. Something very

great, compared with the things upon the earth; something very little,

compared with the things outside the earth.

And as our journeyings together are for a while to be away from earth,

we shall find ourselves obliged to count her as something quite small

in the great universe, where so many larger and mightier things are

to be found,--if indeed they are mightier. Not that we have to say

good-bye altogether to our old home. We must linger about her for a

while before starting, and afterwards it will be often needful to come

back, with speed swifter than the flight of light, that we may compare

notes on the sizes and conditions of other places visited by us.

But first of all: what _is_ this earth of ours?

It was rather a pleasant notion which men held in olden days, that

we--that great and important “We” which loves to perch itself upon

a height--stood firm and fixed at the very center of everything. The

earth was supposed to be a vast flat plain, reaching nobody could tell

how far. The sun rose and set for us alone; and the thousands of stars

twinkled in the sky at night for nobody’s good except ours; and the

blue sky overhead was a crystal covering for the men of our earth,

and nothing more. In fact, people seem to have counted themselves not

merely to have had a kind of kingship over the lower animals of our

earth, but to have been kings over the whole universe. Sun, stars, and

sky, as well as earth, were made for man, and for man only.

This was the common belief, though even in those olden days there were

_some_ who knew better. But the world in general knows better now.

Earth the center of the universe! Why, she is not that of even the

particular family in the heavens to which she belongs. For we do not

stand alone. The earth is one of a family of worlds, and that family is

called THE SOLAR SYSTEM. And so far is our earth from being the head of

the family, that she is not even one of the more important members. She

is merely one of the little sisters, as it were.

Men not only believed the earth, in past days, to be at the center

of the universe; but also they believed her to remain there without

change. Sun, moon, stars, planets, sky, might move; but never the

earth. The solid ground beneath their feet, _that_ at least was firm.

Every day the sun rose and set, and every night the stars, in like

manner, rose and set. But this was easily explained. We on our great

earth stood firm and still, while sun, moon, stars, went circling

round us once in every twenty-four hours, just for our sole and

particular convenience. What an important personage man must have felt

himself then in God’s great universe! Once again, we know better now!

[Illustration: THE SOLAR SYSTEM.]

For it is the earth that moves, and not the sun; it is the earth that

moves, and not the stars. The daily movements of sun and stars, rising

in the east, traveling over the sky, and setting in the west, are

no more real movements on their part than, when we travel in a rail

way-train, the seeming rush of hedges, telegraph posts, houses, and

fields is real. They are fixed and we are moving; yet the movement

appears to us to be not ours but theirs.

Still more strongly would this appear to be the case if there were no

noise, no shaking, no jarring and trembling, to make us feel that we

are not at rest. Sometimes when a train begins to move gently out of

a station, from among other trains, it is at the first moment quite

impossible to say whether the movement belongs to the train in which we

are seated or to a neighboring train. And in the motions of our earth

there is no noise, no shaking, no jarring--all are rapid, silent, and

even.

If you were rising through the air in a balloon, you would at first

only know your own movement by seeing the earth seem to drop away from

beneath you. And just so we can only know the earth’s movements by

seeing how worlds around us _seem_ to move in consequence.

When I speak of the Universe, I mean the whole of God’s mighty creation

as far as the stars reach. Sometimes the word is used in this sense,

and sometimes it is used only for a particular part of creation nearer

to us than other parts. At present, however, we will put aside all

thought of the second narrower meaning.

The wisest astronomer living can not tell us how far the stars reach.

We know now that there is no firm crystal covering over our heads,

dotted with bright points here and there; but only the wide open sky

or heaven, containing millions of stars, some nearer, some farther,

some bright enough to be seen by us all, some only visible through a

telescope.

People talk often of the stars being “set in space;” and the meaning of

“space” is simply “room.” Where you are must be space, or you could not

be there. But it is when we get away from earth, and travel in thought

through the wide fields of space, where God has placed his stars, that

we begin to feel how vast it is, and what specks we are ourselves--nay,

what a speck our very earth is, in this great and boundless creation.

For there is no getting to the borders of space. As one telescope after

another is made, each one stronger in power and able to reach farther

than the last, still more and more stars are seen, and yet more and

more behind and beyond, in countless millions.

It is the same all round the earth. The old notion about our world

being a flat plain has been long since given up. We know her now to be

a round globe, not fixed, but floating like the stars in space.

When you look _up_ into the sky, you are looking exactly in the

opposite direction from where you would be looking _up_ if you were

in Australia. For Australia’s “up” is our “down,” and our “down” is

Australia’s “up.” Or, to put it more truly, “up” is always in the

direction straight away from this earth, on whatever part of it you may

be standing; and “down” is always towards the center of the earth.

All round the globe, in north, south, east, west, whether you are in

Europe, Asia, Africa, or America, though you will see different stars

in certain different quarters of the earth, still overhead you will

find shining countless points of light.

And now, what are these stars? This is a matter on which people are

often confused, and on which it is well to be quite clear before going

one step farther.

Some of the stars you have most likely often noticed. The seven chief

stars of the Great Bear are known to a large number of people; and

there are few who have not admired the splendid constellation of Orion.

Perhaps you also know the W-shape of Cassiopeia, and the brilliant

shining of Sirius, and the soft glimmer of the Pleiades.

The different constellations or groups of principal stars have been

watched by men for long ages past. They are called the fixed stars, for

they do not change. How many thousands of years ago they were first

arranged by men into these groups, and who first gave them their names,

we can not tell.

True, night by night, through century after century, they rise, and

cross the sky, and set. But those are only seeming movements. Precisely

as the turning round of the earth upon her axis, once in every

twenty-four hours, makes the sun appear to rise and cross the sky and

set, in the day-time; so also the same turning of the earth makes the

stars appear to do the same in the night-time.

There is another seeming movement among the stars, which is only in

seeming. Some come into view in summer which can not be seen in

winter; and some come into view in winter which can not be seen in

summer. For the sun, moving on his pathway through the sky, hides those

stars which shine with him in the day-time. The zodiac is an imaginary

belt in the heavens, sixteen or eighteen degrees wide, containing the

twelve constellations through which the sun passes. And as he passes

from point to point of his pathway, he constantly conceals from us

fresh groups of stars by day, and allows fresh groups to appear by

night. Speaking generally, however, the stars remain the same year

after year, century after century. The groups may still be seen as of

old, fixed and unchanging.

[Illustration: THE PLEIADES.]

What are these stars? Stars and planets have both been spoken about.

There is a great difference between the two.

Perhaps if you were asked whether the sun is most like to a star or a

planet, you would be rather at a loss; and many who have admired the

brilliant evening star, Venus, often to be seen after sunset, would be

surprised to learn that the evening star is in reality no star at all.

A star is a sun. Our sun is nothing more nor less than a star. Each one

of the so-called “fixed stars,” that you see shining at night in the

sky, is a sun like our sun; only some of the stars are larger suns and

some are smaller suns than ours.

The main reason why our sun looks so much larger and brighter than the

stars is, that he is so very much nearer to us. The stars are one and

all at enormous distances from the earth. By and by we will go more

closely into the matter of their distance, compared with the distance

of the sun.

At present it is enough to say that if many of the stars were placed

just as near to us as our sun is placed, they would look just as large

and bright; while there are some that would look a great deal larger

and brighter. And if our sun were to travel away from us, to the

distance of the very nearest of the little twinkling stars, he would

dwindle down and down in size and brilliancy, till at last we should

not be able to tell him apart from the rest of the stars.

I have told you that the stars are called “fixed” because they keep

their places, and do not change from age to age. Though the movement

of the earth makes them seem all to sweep past every night in company,

yet they do not travel in and out among one another, or backwards

and forwards, or from side to side. At all events, if there be such

changes, they are so slow and so small as to be exceedingly difficult

to find out. Each group of stars keeps its own old shape, as for

hundreds of years back.

But among these fixed stars there are certain stars which do go to and

fro, and backwards and forwards. Now they are to be seen in the middle

of one constellation, and now in the middle of another. These restless

stars were long a great perplexity. Men named them Planets or Wanderers.

We know now that the planets are in reality not stars at all, and also

that they are not nearly so far away from us as the fixed stars. In

fact, they are simply members of our own family--the Solar System. They

are worlds, more or less like the world we live in; and they travel

round and round the sun as we do, each more or less near to him; and

they depend upon him for heat and light, in more or less the same

manner as ourselves.

Therefore, just as our sun is a star, and stars are suns, so our earth

or world is a planet, and planets are worlds. EARTH is the name we

give to that particular world or planet on which we live. Planets may

generally be known from stars by the fact that they do not twinkle.

But the great difference between the two lies in the fact that a star

shines by its own radiant, burning light, whereas a planet shines

merely by light reflected or borrowed from the sun.

But how were the earth and the other worlds made? Let us imagine an

immense gaseous mass placed in space. Attraction is a force inherent in

every atom of matter. The denser portion of this mass will insensibly

attract towards it the other parts, and in the slow fall of the more

distant molecules towards this more attractive region, a general motion

is produced, incompletely directed towards this center, and soon

involving the whole mass in the same motion of rotation. The simplest

form of all, even in virtue of this law of attraction, is the spherical

form. It is that which a drop of water takes, and a drop of mercury if

left to itself.

The laws of mechanics show that, as this gaseous mass condenses and

shrinks, the motion of rotation of the nebula is accelerated. In

turning, it becomes flattened at the poles, and gradually takes the

form of an immense lens-shaped mass of gas. It has begun to turn so

quickly as to develop at its exterior circumference a centrifugal force

superior to the general attraction of the mass, as when we whirl a

sling. The inevitable consequence of this excess is a rupture of the

equilibrium, which detaches an external ring. This gaseous ring will

continue to rotate in the same time and with the same velocity; but

the nebulous mother will be henceforth detached, and will continue to

undergo progressive condensation and acceleration of motion. The same

feat will be reproduced as often as the velocity of rotation surpasses

that by which the centrifugal force remains inferior to the attraction.

It may have happened also that secondary centers of condensation would

be formed even in the interior of the nebula.

In our system the rings of Saturn still subsist.

The successive formation of the planets, their situation near the

plane of the solar equator, and their motions of translation round the

same center, are explained by the theory which we are discussing. The

most distant known planet, Neptune, would be detached from the nebula

at the epoch when this nebula extended as far as the planet, out to

nearly three thousand millions of miles, and would turn in a slow

revolution requiring a period of 165 years for its accomplishment. The

original ring could not remain in the state of a ring unless it was

perfectly homogeneous and regular; but such a condition is, so to say,

unrealizable, and it did not delay in condensing itself into a sphere.

Successively, Uranus, Saturn, Jupiter, the army of small planets, Mars,

would thus be detached or formed in the interior of this same nebula.

Afterwards came the earth, of which the birth goes back to the epoch

when the sun had arrived at the earth’s present position. Venus and

Mercury would be born later. Will the sun give birth to a new world?

This is not probable.

The story of the sun, moon, and stars · 第 1 / 33 章