The Moon: A Popular TreatiseServiss, Garrett Putman
Science
The Moon: A Popular Treatise
Serviss, Garrett Putman
Moon
“I was saying,” I resumed, “that another interesting thing in addition
to the cause of the moon’s changing phases is represented here. You
observe that a little cross stands on each of the four circles
representing the moon, and that, in every case, the cross is in the
center of that side of the moon which faces the earth. In fact the
position of the cross upon the moon is fixed and invariable, and it
always points toward the earth because the moon makes exactly one
rotation on her axis in the course of one revolution around her orbit,
or, as it is often called, one lunation. We know that this is so because
we always see the same features of the lunar surface, no matter where
the moon may be situated. This is true although, in consequence of the
phases, we cannot see the whole face of the moon except when she is
full. But whether it is the New Moon, or First Quarter, or Full Moon, or
Last Quarter, or Old Moon, that we look at, the mountains and plains
visible are identically the same. If the moon did not turn once on her
axis in going once around the earth we would see all of her sides in
succession, although only at Full Moon could we see an entire hemisphere
illuminated by the sun. At Old and New Moon the side presented to the
earth would be just the opposite to that presented at Full Moon. At Last
Quarter the side facing the earth would be the opposite to that facing
the earth at First Quarter.”
“But, tell me,” said my friend, “how did the moon ever come to so
humiliating a pass that she must be forever turning on her heel to face
the earth?”
“That,” I replied, “is a result of the same forces which originally
separated her from the earth and gradually pushed her off to her present
distance. In a word it is due to ‘tidal friction.’ Before the moon had
solidified, the attraction of the earth raised huge tides in her molten
mass. These tides acted on the rotating moon like brakes on a wheel, and
at length they slowed down her rotation until its period became
identical with that of her revolution around the earth. For the
mathematical calculations on which all this is based you must go to
Professor Darwin’s book on ‘The Tides,’ or some similar technical
treatise; but I imagine you will never do that.”
“Not just at present, I assure you. I do not know what unexpected
ambition for the acquirement of scientific knowledge may arise after I
have seen those wonders that you have promised to show me in the moon,
but, for the moment, I am content to accept your statement of the simple
fact.”
Public-domain text, read in full here on John Shaqi.
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