The story of the sun, moon, and starsGiberne, Agnes
Science
The story of the sun, moon, and stars
Giberne, Agnes
Astronomy -- Juvenile literature
If such a journey to the moon as the one described two chapters back
were indeed possible, the voyage aloft would hardly be so easily and
safely performed as is there taken for granted. Putting aside the
thought of other difficulties, such as lack of conveyance and lack of
air, there would be the danger of passing through a very considerable
storm of missiles--a kind of “celestial cannonade”--which, to say the
least, would prove very far from agreeable.
These “starlets” and “meteor planets,” as they have been called, are
not visible in a normal condition, because of their minuteness. But on
entering our atmosphere they are rendered luminous, owing to the heat
evolved by the sudden and violent compression of the air in front of
the moving body. According to this view, shooting-stars, which simply
dart across the heavens, may be regarded as coming within the limits of
the atmosphere, and carried out of it again, by their immense velocity,
passing on in space. Meteoric showers may result from an encounter with
a group of these bodies, while aërolites are those which come so far
within the sphere of the earth’s attraction as to fall to its surface.
More than two thousand years ago the Greeks venerated a famous stone
which fell from the heavens on the river Ægos.
[Illustration: METEOR EMERGING FROM BEHIND A CLOUD (NOV. 23, 1877).]
It will scarcely be believed what numbers of these shooting-stars or
meteorites constantly fall to the earth. As she travels on her orbit,
hurrying along at the rate of nineteen miles each second, she meets
them by tens of thousands. They too, like the earth, are journeying
round the great center of our family. But they are so tiny, and
the earth by comparison is so immense, that her strong attraction
overpowers one after another, drags it from its pathway, and draws it
to herself.
And then it falls, flashing like a bright star across the sky, and
the little meteorite has come to his end. His myriads of companions,
hastening still along their heavenly track--for the meteorites seem to
travel commonly in vast flocks or companies--might, had they sense,
mourn in vain for the lost members of their family.
Any one taking the trouble to watch carefully some portion of the sky
after dark, may expect to see each hour about four to eight of these
shooting-stars--except in the months of August and November, when the
number is much larger. About six in an hour does not sound a great
deal. But that merely means that there have been six in one direction,
and near enough for you to see. Somebody else, watching, may have
seen six in another direction; and somebody else, a few miles away,
may have seen six more. It is calculated that, in the course of every
twenty-four hours, about four hundred millions of meteorites fall to
earth, including those visible only through telescopes.
Public-domain text, read in full here on John Shaqi.
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