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<v Speaker 1>Section twenty two of Sun, Moon and Stars Astronomy for Beginners.

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<v Speaker 1>This is a LibriVox recording. All LibriVox recordings are in

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<v Speaker 1>the public domain. For more information or to volunteer, please

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<v Speaker 1>visit LibriVox dot org. Read by Kyle Johnson. Sun Moon

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<v Speaker 1>and Stars Astronomy for Beginners by Agnes Geburn, Part three,

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<v Speaker 1>Chapter one, Many Suns, I even my hands have stretched

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<v Speaker 1>out the heavens and all their host have I commanded

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<v Speaker 1>Isaiah forty five twelve. Once more we have to wing

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<v Speaker 1>our flight far far away from the busy Solar system

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<v Speaker 1>where we live, away from whirling planets, moons, meteorites, all

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<v Speaker 1>shining with reflected light, away from the great central Sun himself,

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<v Speaker 1>our own particular bright star. Once more we have in

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<v Speaker 1>imagination to cross the vast black empty space. Is it black?

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<v Speaker 1>And is it empty? Had we sight to see things

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<v Speaker 1>as they are separating our Sun from other suns, our

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<v Speaker 1>star from other stars. For the Sun is a star

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<v Speaker 1>only a star, and stars are suns, big blazing suns.

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<v Speaker 1>One is near and the others far away. That is

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<v Speaker 1>the main difference. We have no longer to do with

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<v Speaker 1>bodies merely reflecting another's light, always dark on one side

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<v Speaker 1>and bright on the other. But with burning bodies shining

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<v Speaker 1>all around by their own light, we have no longer

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<v Speaker 1>to picture just one single star with his surrounding worlds.

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<v Speaker 1>But we have to fix our thoughts upon the great

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<v Speaker 1>universe of stars or suns in countless millions. The Sun

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<v Speaker 1>is center and ruler and king in his own system,

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<v Speaker 1>but as a star, he is only one among many stars,

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<v Speaker 1>some greater, some less than himself. Thought travels fast, faster

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<v Speaker 1>than a comet, faster than light. A rushing comet would,

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<v Speaker 1>it is believed, take eight millions of years to cross

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<v Speaker 1>the chasm between the nearest known fixed star and us.

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<v Speaker 1>Light flashing along at the rate of about one hundred

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<v Speaker 1>eighty six thousand, three hundred miles. A second will perform

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<v Speaker 1>the same journey in four years and one third, But

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<v Speaker 1>Thought overleaps the boundary in less than four minutes. Each

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<v Speaker 1>star that we see in the heavens is, to our

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<v Speaker 1>eye sight, simply one point of light. The brighter stars

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<v Speaker 1>are said to be of greater magnitude, and the fainter

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<v Speaker 1>stars of lesser magnitude. Yet one and all, they have

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<v Speaker 1>no apparent size. The most powerful telescope, though it can

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<v Speaker 1>increase their brilliancy, cannot add to their size. A planet,

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<v Speaker 1>which to the naked eye may look like a star,

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<v Speaker 1>will under a telescope show a disc, the breadth of

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<v Speaker 1>which can be measured or divided. But no star has

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<v Speaker 1>any real sensible disc in the most powerful telescope yet constructed.

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<v Speaker 1>The reason of this is the enormous distance of the

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<v Speaker 1>stars far off as many of the planets lie, Yet

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<v Speaker 1>the farthest of them is a member of our own

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<v Speaker 1>household compared with the nearest star. I have already tried

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<v Speaker 1>to make clear the fact of their vast distance. Light,

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<v Speaker 1>which comes to us from the Sun in less than

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<v Speaker 1>nine minutes, takes four years and four months to reach

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<v Speaker 1>us from Alpha Centauri. From this four years and a

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<v Speaker 1>half length of journey between Alpha Centauri and other Earth,

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<v Speaker 1>the numbers rise rapidly to twenty years, fifty years, hundreds

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<v Speaker 1>of years, even thousands of years. The distances of most

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<v Speaker 1>of the stars are completely beyond our power to measure

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<v Speaker 1>the whole orbit of our Earth. Nay, the whole wide

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<v Speaker 1>orbit of the far off Neptune would dwindle down to

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<v Speaker 1>one single point if seen from the greater number of

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<v Speaker 1>the stars it used to be believed that taking the

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<v Speaker 1>stars generally, there was probably no very marked difference in

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<v Speaker 1>their size, their kind, their brightness. Some of course would

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<v Speaker 1>be rather larger, and others rather smaller. Still, it was

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<v Speaker 1>supposed that they might be roughly classed as formed much

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<v Speaker 1>on the same scale and the same plan. But of

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<v Speaker 1>late years this notion has been utterly given up. A

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<v Speaker 1>very similar idea used to be held with regard to

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<v Speaker 1>the solar system. The wonderful variety of form and richness

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<v Speaker 1>in numbers now known to abound within its limits are

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<v Speaker 1>discoveries of later years. And now the same variety in

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<v Speaker 1>kind and size is found also among the stars. The

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<v Speaker 1>more we look into the heavens, the more we see

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<v Speaker 1>that dull, blank uniformity is not to be found there.

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<v Speaker 1>It is the same upon earth. Man builds his little

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<v Speaker 1>rows of box like houses side by side, each one

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<v Speaker 1>exactly like all the rest, Or dresses his thousand soldiers

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<v Speaker 1>in coats of the same cut and color, or repeats

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<v Speaker 1>a neat leaf design hundreds of times on carpets or wallpapers.

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<v Speaker 1>But God never makes two leaves or two blades of

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<v Speaker 1>grass alike wholesale, turning out of things after one pattern

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<v Speaker 1>is quite a human idea, not divine. We know so

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<v Speaker 1>much about the stars as that some are at least

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<v Speaker 1>considerably larger and some considerably smaller than others. When one

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<v Speaker 1>star is seen to shine brightly and another beside it

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<v Speaker 1>shines dimly, we are apt to think that the brightest

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<v Speaker 1>must be the nearest. Yet it is often impossible for

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<v Speaker 1>us to say how much of the difference is owing

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<v Speaker 1>to the greater distance of one or the other, or

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<v Speaker 1>to the greater size of one or the other, or

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<v Speaker 1>to the greater brilliancy of one or the other. In

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<v Speaker 1>many instances we do not know enough to be quite

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<v Speaker 1>sure that there is a great difference not only in

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<v Speaker 1>the distance of the stars, but in their size, their kind,

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<v Speaker 1>their brightness. The stars have been sometimes classified into four

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<v Speaker 1>distinct orders or degrees, partly depending on their color. The

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<v Speaker 1>first class is that of the white suns. These are

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<v Speaker 1>generally held to be the grandest and mightiest of all

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<v Speaker 1>the stars. Serious belongs to the order of white suns.

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<v Speaker 1>Secondly comes the class of golden suns. To these blazing

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<v Speaker 1>orbs of yellow light, said to be second only to

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<v Speaker 1>the white light stars, belongs our own sun. Thirdly, there

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<v Speaker 1>are numbers of stars called variable stars, the light of

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<v Speaker 1>which is constantly changing, now becoming greater, now becoming less. Fourthly,

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<v Speaker 1>there is the class of small red suns, about which

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<v Speaker 1>not so much is known. These four orders or divisions

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<v Speaker 1>do not, by any means include all the stars, or

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<v Speaker 1>even all the single stars. Roughly speaking, however, the greater

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<v Speaker 1>number of single stars, and many also of the double stars,

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<v Speaker 1>belong to one or another of the above classes. When

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<v Speaker 1>we talk of the different sizes of the different stars,

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<v Speaker 1>it should be plainly understood that we have no means

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<v Speaker 1>of directly measuring them. A point of light showing no disk,

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<v Speaker 1>no surface, no breadth, cannot be measured, for there is

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<v Speaker 1>nothing to measure. In certain cases, we are not entirely

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<v Speaker 1>without the power of judging. The distances of some of

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<v Speaker 1>the stars from us have been found out. Knowing how

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<v Speaker 1>far off any particular star is, astronomers are able to

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<v Speaker 1>calculate exactly how bright our own sun would look at

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<v Speaker 1>that same distance. If they find that our sun would

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<v Speaker 1>shine just as the star in question shines, there is

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<v Speaker 1>some reason for supposing that our sun and yonder star

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<v Speaker 1>may be of the same size. If our sun would

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<v Speaker 1>shine more brightly than the star shines, there is some

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<v Speaker 1>reason for supposing that the star may be smaller than

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<v Speaker 1>our sun. If our sun would shine more dimly than

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<v Speaker 1>the star shines, there is some reason for supposing that

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<v Speaker 1>the star may be larger than our sun. Other matters, however,

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<v Speaker 1>have to be considered. Suppose we find a star at

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<v Speaker 1>a certain distance shining twice as brilliantly as our own

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<v Speaker 1>sun would shine at that same distance. Naturally, then we

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<v Speaker 1>say that star must be much larger than our sun.

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<v Speaker 1>The reasoning may be mistaken. We do not know the fact.

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<v Speaker 1>What if, instead of being a much larger sun, it

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<v Speaker 1>is only a much brighter sun. This is more than possible.

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<v Speaker 1>Some doubts have been indeed expressed whether the surface of

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<v Speaker 1>any star could exceed that of our sun in radiance.

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<v Speaker 1>But we have really no reason to suppose that our

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<v Speaker 1>son is a king of sons in brilliance, since certainly

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<v Speaker 1>he is not so inside in speed. When we picture

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<v Speaker 1>to ourselves the star depths the boundless reaches of heavenly space.

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<v Speaker 1>With these countless blazing suns scattered broadcast throughout, we have

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<v Speaker 1>not to picture a universe in repose. On the contrary,

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<v Speaker 1>all is life, stir energy, Just as in the busy

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<v Speaker 1>whirl of our solar system knows such thing as rest

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<v Speaker 1>is to be found, so also it seems to be

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<v Speaker 1>in the wide universe. Every star is in motion, fixed

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<v Speaker 1>as we call them. They are not fixed invisible, as

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<v Speaker 1>their movements are to our eyes through immensity of distance.

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<v Speaker 1>Yet all are moving. Those silent, placid, twinkling specks of

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<v Speaker 1>light are in reality huge, roaring, seething, tumultuous furnaces of

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<v Speaker 1>fire and flame, heat and radiance. Each too is hurrying

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<v Speaker 1>along his appointed pathway in space. Some move faster, some

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<v Speaker 1>move more slowly. One mile per second, ten miles per second,

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<v Speaker 1>twenty fifty hundreds of miles per second. Thus varying are

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<v Speaker 1>their rates of speed, but rather fast or whether slowly still?

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<v Speaker 1>Onward and ever onward they press. Some are rushing towards us,

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<v Speaker 1>Some are rushing away from us. Some are speeding to

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<v Speaker 1>the right, some are speeding to the left. Where are

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<v Speaker 1>they going? Does any single star ever return to his

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<v Speaker 1>starting point? Wherever that starting point may have been? Do

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<v Speaker 1>they journey in vast circles or ellipses round some far

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<v Speaker 1>distant center. What controls them all? Is it the mighty

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<v Speaker 1>power of some such center, Or does each star, by

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<v Speaker 1>his faint and distant attraction, help to contryro all his

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<v Speaker 1>brother stars, to guide them on their appointed path, to

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<v Speaker 1>preserve the delicate balance of a universe. How little we

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<v Speaker 1>know about the matter, Only so much we can tell

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<v Speaker 1>that the controlling and restraining hand of God is over

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<v Speaker 1>the whole, Whether by the attraction of one great center

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<v Speaker 1>or by the united influences of a thousand fainter attractions.

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<v Speaker 1>He steers each radiant sun upon its heavenly path, upholding

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<v Speaker 1>all things by the word of His power. There is

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<v Speaker 1>no blundering, no confusion, no entanglement. All is perfect order,

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<v Speaker 1>calm arrangement, restrained energy. End of Section twenty two.
