The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
One more mighty chasm of nine hundred millions of miles, for the same
distance which separates the pathway of Saturn from the pathway of
Uranus, separates also the pathway of Uranus from the pathway of
Neptune. Cold, and dark, and dreary indeed seems to us the orbit on
which this banished member of our family circle creeps round the sun,
in the course of one hundred and sixty-five years, at the sluggish rate
of three miles a second.
On the planet Saturn, the quantity of light and heat received from
the sun is not much more than a hundredth part of that which we are
accustomed to receive on earth. But by the time we reach Neptune, the
great sun has faded and shrunk in the distance until to our eyes he
looks only like an exceedingly brilliant and dazzling star.
We know little of this far-off brother, Neptune, except that he is
rather larger than Uranus, being one hundred and five times as big as
the earth; that he has at least one moon; and also that, like Uranus,
he is made of materials lighter than those of earth, but heavier than
those of Jupiter or Saturn.
After all, it is no easy matter to gain clear ideas as to sizes and
distances from mere statements of “so many miles in diameter,” and “so
many millions of miles away.” A “million miles” carries to the mind a
very dim notion of the actual reality.
Now if we can in imagination bring down all the members of the Solar
System to a small size, keeping always the same proportions, we may
find it a help. “Keeping the same proportions” means that all must be
lessened alike, all must be altered in the same degree. Whatever the
supposed size of the earth may be, Venus must be still about the same
size as the earth, Saturn seven hundred times as large, and so on.
Also, whatever the distance of the earth from the sun, in miles, or
yards, or inches, Mercury must still be one-third as far, Jupiter still
five times as far, and thus with the rest.
First, as to size alone. Suppose the earth is represented by a small
globe, exactly three inches in diameter. It will be a very small globe.
Not only men and houses, but mountains, valleys, seas, will all have to
be reduced to so minute a size, as to be quite invisible to the naked
eye.
Fairly to picture the other members of the Solar System, in due
proportion, you will have them as follows:
Mercury and Mars will be balls smaller than the earth, and Venus nearly
the same size of the earth. Uranus and Neptune will be each somewhere
about a foot in diameter. Saturn will be twenty-eight inches and
Jupiter thirty-two inches in diameter. The sun will be a huge dazzling
globe, _twenty-six feet_ in diameter. No wonder he weighs seven hundred
and fifty times as much as all his planets put together.
Next let us picture the system more exactly on another and smaller
scale. First, think of the sun as a brilliant globe, about nine feet,
or three yards, in diameter, floating in space.
Public-domain text, read in full here on John Shaqi.
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