Man and the Glacial PeriodWright, G. Frederick (George Frederick)
History
Man and the Glacial Period
Wright, G. Frederick (George Frederick)
Glacial epoch; Prehistoric peoples
While it is impossible absolutely to disprove this hypothesis, it labors
under the difficulty of having little positive evidence in its favor,
and thus contravenes a fundamental law of scientific reasoning, that we
must have a real cause upon which to rest our theories. In endeavouring
to explain the unknown, we should have something known to start with.
But in this case we are not sure that there are any such variations in
the temperature of the space through which the solar system moves. This
theory, therefore, cannot come in for serious consideration until all
others have been absolutely disproved. As we shall also more fully see,
in the subsequent discussion, the distribution of the ice during the
Glacial period was not such as to indicate a gradual extension of it from
the north pole, but rather the accumulation upon centres many degrees to
the south.
Closely allied with the preceding theory is the supposition broached
by some astronomers that the sun is a variable star, dependent to some
extent for its heat upon the impact of meteorites, or to the varying
rapidity with which the contraction of its volume is proceeding.
It is well known that when two solid bodies clash together, heat is
produced proportionate to the momentum of the two bodies. In other
words, the motion which is arrested is transformed into heat. Mr. Croll,
in his last publication[DR] upon the subject, ingeniously attempted to
account for the gaseous condition of the nebulæ and the heat of the sun
and other fixed stars by supposing it to be simply transformed motion.
According to this theory, the original form of force imparted to the
universe was that exerted in setting in motion innumerable dark bodies,
which from time to time have collided with each other. The effects of
such collisions would be to transform a large amount of motion into
heat and its accompanying forms of molecular force. The violence of the
compact of two worlds would be so great as to break them up into the
original atoms of which they are composed, and the heat set free would
be sufficient to keep the masses in a gaseous condition and cause them
to swell out into enormous proportions. From that time on, as the heat
radiated into space, there would be the gradual contraction which we
suppose is going on in all the central suns, accompanied, of course, with
a gradual decline of the heat-energy in the system.
[Footnote DR: Stellar Evolution and its Relation to Geological Time.]
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