Worlds in the making: The evolution of the universeArrhenius, Svante
Science
Worlds in the making: The evolution of the universe
Arrhenius, Svante
Cosmogony
Since, now, the temperature of the earth-crust would much more quickly
sink from 100° to 55° than it had fallen from 1000° to 100°, we may
imagine that only a few thousands of years may have intervened between
the formation of the first crust of the earth and the cooling down
to a temperature such as would sustain life. Since that time the
temperature has probably never been so low that the larger portion
of the earth’s surface would not have been able to support organisms,
although there have been several glacial ages in which the arctic
districts inaccessible to life must have extended much farther than
at present. The ocean will also have been free of ice over much the
greatest portion of its surface at all times, and may therefore have
been inhabited by organisms in all ages. The interior of the earth
cools continually, though slowly, because heat passes from the inner,
warmer portions to the other, cooler portions through the crust of the
earth.
The earth is able to serve as the abode of living beings because its
outer portions are cooled to a suitable temperature (below 55°) by
radiation, and because the cooling does not proceed so far that the
open sea would continually be frozen over, and that the temperature on
the Continent would always remain below freezing-point. We owe this
favorable intermediate stage to the fact that the radiation from the
sun balances the loss of heat by radiation into space, and that it is
capable of maintaining the greater portion of the surface of the earth
at a temperature above the freezing-point of water. The temperature
conditioning life on a planet is therefore maintained only because,
on the one side, light and heat are received by radiation from the
sun in sufficient quantities, while on the other side an equivalent
radiation of heat takes place into space. If the heat gain and the heat
loss were not to balance each other, the term of suitable conditions
would not last long. The temperature of the earth-crust could sink
in a few hundreds or thousands of years from 1000° to 100°, because
when the earth was at this high temperature its radiation into space
predominated over the radiation received from the sun. On the other
hand, about a hundred million years have passed, according to Joly,
since the age when the ocean originated. The temperature of the earth,
therefore, required this long space of time in order to cool down from
365° (at which temperature water vapor can first be condensed to liquid
water) to its present temperature. The cooling afterwards proceeded at
a slower rate, because the difference between the radiations inward and
outward was lessened with the diminishing temperature of the earth.
Various methods have been applied in estimating these periods. Joly
based his estimate on the percentage of salt in the sea and in the
rivers. If we calculate how much salt there is in the sea, and how much
salt the rivers can supply to it in the course of a year, we arrive at
Public-domain text, read in full here on John Shaqi.
Reviews
Reviews
No reviews yet
Be the first to share your thoughts on this work.
Join the Discussion
Join the discussion
Sign in to leave a comment or review.
Sign InorCreate an account