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
Perhaps the most remarkable thing which one notices about the moon is
that she always turns the same side towards us, and so we never see her
other side. One might be led from this to jump to the conclusion that
she does not rotate upon an axis, as do the other bodies which we see;
but, paradoxical as it may appear, the fact that she turns one face
always towards the earth, is actually a proof that she _does_ rotate
upon an axis. The rotation, however, takes place with such slowness,
that she turns round but once during the time in which she revolves
around the earth (see Fig. 15). In order to understand the matter
clearly, let the reader place an object in the centre of a room and walk
around it once, _keeping his face turned towards it the whole time_,
While he is doing this, it is evident that he will face every one of the
four walls of the room in succession. Now in order to face each of the
four walls of a room in succession one would be obliged _to turn oneself
entirely round_. Therefore, during the act of walking round an object
with his face turned directly towards it, a person at the same time
turns his body once entirely round.
In the long, long past the moon must have turned round much faster than
this. Her rate of rotation has no doubt been slowed down by the action
of some force. It will be recollected how, in the course of the previous
chapter, we found that the tides were tending, though exceedingly
gradually, to slow down the rotation of the earth upon its axis. But, on
account of the earth's much greater mass, the force of gravitation
exercised by it upon the surface of the moon is, of course, much more
powerful than that which the moon exercises upon the surface of the
earth. The tendency to tidal action on the moon itself must, therefore,
be much in excess of anything which we here experience. It is, in
consequence, probable that such a tidal drag, extending over a very long
period of time, has resulted in slowing down the moon's rotation to its
present rate.
The fact that we never see but one side of the moon has given rise from
time to time to fantastic speculations with regard to the other side.
Some, indeed, have wished to imagine that our satellite is shaped like
an egg, the more pointed end being directed away from us. We are here,
of course, faced with a riddle, which is all the more tantalising from
its appearing for ever insoluble to men, chained as they are to the
earth. However, it seems going too far to suppose that any abnormal
conditions necessarily exist at the other side of the moon. As a matter
of fact, indeed, small portions of that side are brought into our view
from time to time in consequence of slight irregularities in the moon's
movement; and these portions differ in no way from those which we
ordinarily see. On the whole, we obtain a view of about 60 per cent. of
the entire lunar surface; that is to say, a good deal more than
one-half.
Public-domain text, read in full here on John Shaqi.
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