The Moon: A Popular TreatiseServiss, Garrett Putman
Science
The Moon: A Popular Treatise
Serviss, Garrett Putman
Moon
“I shall presently point out to you one of the most notable of those
other places,” I replied. “Let me now fulfill my promise to tell you
more about the lunar atmosphere. I have told you already that there are
strong reasons for supposing that the moon once had a far more dense
atmosphere than she possesses at present, and I have mentioned some of
the ways in which this atmosphere is supposed to have disappeared. I
think that it is worth our while to refer to them again. In the first
place the moon’s atmosphere may have been withdrawn into vast internal
cavities formed by the gigantic volcanic eruptions. Secondly, it may
have been absorbed both mechanically and chemically by the core of the
moon as it cooled off. We know that cooling rocks absorb immense
quantities of the gases constituting the air we breathe. In fact we may
look forward to a time, fortunately for us extremely remote, when the
interior rocks of the earth will, in this manner, absorb perhaps all of
its atmosphere.”
“But if the air of the moon has gone into great cavities in the
interior, why might not the living beings of the moon have followed it
there?”
“According to some of the theorists,” I answered, “that may really be
what has occurred, and thus the moon has become a ‘cavern world’ on a
gigantic scale. But science does not regard seriously these speculations
about ‘cave life’ in the moon. A third hypothesis is that which I have
mentioned concerning the escape of the atmospheric gases from the moon
on account of its attraction being insufficient permanently to retain
them. This process would be gradual, because the molecules of a gas fly
in _all_ directions, only a small proportion having their trajectories
directly away from the center of the globe on which they are held. But a
singular consequence of this theory is that interplanetary space must
contain an enormous number of such wandering molecules, and every
attracting body must draw more or less of them to its surface, thus
forming an atmosphere for itself. As Professor Young has remarked, if as
many of these molecules enter a planet’s atmosphere in a day as escape
from it there can be no decrease of the total amount of air. If more
escape than enter, the atmosphere will diminish. If more enter than
escape, the atmosphere will grow. Finally if none escape the atmosphere
may increase indefinitely. This, as far as the effect of gravitation is
concerned, should be the case on the sun, for the solar attraction is
more than sufficient to retain any gas known to us. In consequence, the
sun’s atmosphere may be increasing in extent and density. Even the
earth’s atmosphere may be slowly increasing from this cause, and herein
may lie the explanation of the enormous atmosphere surrounding the great
planet Jupiter.
Public-domain text, read in full here on John Shaqi.
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