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 we carefully watch the heavens we notice that the background of the
sky, with all the brilliant objects which sparkle in it, appears to turn
once round us in about twenty-four hours; and that the pivot upon which
this movement takes place is situated somewhere near what is known to us
as the _Pole Star_. This was one of the earliest facts noted with regard
to the sky; and to the men of old it therefore seems as if the heavens
and all therein were always revolving around the earth. It was natural
enough for them to take this view, for they had not the slightest idea
of the immense distance of the celestial bodies, and in the absence of
any knowledge of the kind they were inclined to imagine them
comparatively near. It was indeed only after the lapse of many
centuries, when men had at last realised the enormous gulf which
separated them from even the nearest object in the sky, that a more
reasonable opinion began to prevail. It was then seen that this
revolution of the heavens about the earth could be more easily and more
satisfactorily explained by supposing a mere rotation of the solid earth
about a fixed axis, pointed in the direction of the polar star. The
probability of such a rotation on the part of the earth itself was
further strengthened by the observations made with the telescope. When
the surfaces of the sun and planets were carefully studied these bodies
were seen to be rotating. This being the case, there could not surely
be much hesitation in granting that the earth rotated also; particularly
when it so simply explained the daily movement of the sky, and saved men
from the almost inconceivable notion that the whole stupendous vaulted
heaven was turning about them once in every twenty-four hours.
Public-domain text, read in full here on John Shaqi.
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