A Text-Book of AstronomyComstock, George C. (George Cary)
Science
A Text-Book of Astronomy
Comstock, George C. (George Cary)
Astronomy
The attraction of the earth for the moon has very slightly pulled the
latter out of shape (§ 42), so that the particular diameter, which
points toward the earth, is a little longer than any other, and thus
serves as a handle which the earth lays hold of and pulls down into its
lowest possible position--i. e., the position in which it points toward
the center of the earth. Just how long this handle is, remains unknown,
but it may be shown from the law of gravitation that less than a hundred
yards of elongation would suffice for the work it has to do.
100. THE MOON AS A WORLD.--Thus far we have considered the moon as a
satellite of the earth, dependent upon the earth, and interesting
chiefly because of its relation to it. But the moon is something more
than this; it is a world in itself, very different from the earth,
although not wholly unlike it. The most characteristic feature of the
earth's surface is its division into land and water, and nothing of this
kind can be found upon the moon. It is true that the first generation of
astronomers who studied the moon with telescopes fancied that the large
dark patches shown in Fig. 55 were bodies of water, and named them
oceans, seas, lakes, and ponds, and to the present day we keep those
names, although it is long since recognized that these parts of the
moon's surface are as dry as any other. Their dark appearance indicates
a different kind of material from that composing the lighter parts of
the moon, material with a different albedo, just as upon the earth we
have light-colored and dark-colored rocks, marble and slate, which seen
from the moon must present similar contrasts of brightness. Although
these dark patches are almost the only features distinguishable with the
unaided eye, it is far otherwise in the telescope or the photograph,
especially along the ragged edge where great numbers of rings can be
seen, which are apparently depressions in the moon and are called
craters. These we find in great number all over the moon, but, as the
figure shows, they are seen to the best advantage near the
_terminator_--i. e., the dividing line between day and night, since the
long shadows cast here by the rising or setting sun bring out the
details of the surface better than elsewhere. Carefully examine Fig. 55
with reference to these features.
[Illustration: FIG. 55.--The moon at first and last quarter. Lick
Observatory photographs.]
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