Astronomy of To-day: A Popular Introduction in Non-Technical LanguageDolmage, Cecil Goodrich Julius
Science
Astronomy of To-day: A Popular Introduction in Non-Technical Language
Dolmage, Cecil Goodrich Julius
Astronomy
If the night sky be watched, it will be soon found that its apparent
turning movement seems to take place around a certain point, which
appears as if fixed. This point is known as the north pole of the
heavens; and a rather bright star, which is situated very close to this
hub of movement, is in consequence called the Pole Star. For the
dwellers in southern latitudes there is also a point in their sky which
appears to remain similarly fixed, and this is known as the south pole
of the heavens. Since, however, the heavens do not turn round at all,
but the earth does, it will easily be seen that these apparently
stationary regions in the sky are really the points towards which the
axis of the earth is directed. The positions on the earth's surface
itself, known as the North and South Poles, are merely the places where
the earth's axis, if there were actually such a thing, would be expected
to jut out. The north pole of the earth will thus be situated exactly
beneath the north pole of the heavens, and the south pole of the earth
exactly beneath the south pole of the heavens.
We have seen that the earth rotates upon its imaginary axis once in
about every twenty-four hours. This means that everything upon the
surface of the earth is carried round once during that time. The
measurement around the earth's equator is about 24,000 miles; and,
therefore, an object situated at the equator must be carried round
through a distance of about 24,000 miles in each twenty-four hours.
Everything at the equator is thus moving along at the rapid rate of
about 1000 miles an hour, or between sixteen and seventeen times as
fast as an express train. If, however, one were to take measurements
around the earth parallel to the equator, one would find these
measurements becoming less and less, according as the poles were
approached. It is plain, therefore, that the speed with which any point
moves, in consequence of the earth's rotation, will be greatest at the
equator, and less and less in the direction of the poles; while at the
poles themselves there will be practically no movement, and objects
there situated will merely turn round.
Public-domain text, read in full here on John Shaqi.
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