The story of the sun, moon, and stars — John Shaqi
The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
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.
CHAPTER II
THE HEAD OF OUR FAMILY.
People began very early in the history of the world to pay close
attention to the sun. And no wonder. We owe so much to his heat and
light that the marvel would be if men had not thought much about him.
Was the sun really any larger than he looked, and if so, how much
larger was he? And what was his distance from the earth? These were two
of the questions which puzzled our ancestors the longest. If once they
could have settled exactly how far off the sun really was, they could
easily have calculated his exact size; but this was just what they
could not do.
So one man supposed that the sun must be quite near, and very little
larger than he looked. Another thought he might be seventy-five miles
in diameter. A third ventured to believe that he was larger than the
country of Greece. A fourth was so bold as to imagine that he might
even outweigh the earth herself.
After a while many attempts were made to measure the distance of the
sun; and a great many different answers to this difficult question
were given by different men, most of them very wide of the mark. It
is only of late years that the matter has been clearly settled. And,
indeed, it was found quite lately that a mistake of no less than three
millions of miles had been made, notwithstanding all the care and all
the attention given. But though three millions of miles sounds a great
deal, yet it is really very little--only a tiny portion of the whole.
For the distance of the sun from the earth is no less than about
NINETY-THREE MILLIONS OF MILES. Ninety-three millions of miles! Can
you picture that to yourself? Try to think what is meant by a thousand
miles. Our earth is eight thousand miles in diameter. In other words,
if you were to thrust a gigantic knitting-needle through her body,
from the North Pole to the South Pole, it would have to be about eight
thousand miles long.
Public-domain text, read in full here on John Shaqi.
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