Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
We have, then, a relatively narrow range of temperatures which seems to
be essential to his comfortable existence and development: we may call
it 150 degrees in extent. Had not the surface temperature of the earth
been maintained within this range for indefinite ages, in the regions
where the human race has developed, quite certainly man would not be
here. How this equability of temperature has been maintained does not
now matter. Clearly the earth must have existed through indefinite ages
in the process of cooling down from temperatures of at least 6,000
degrees.
During this stage the temperature of the surface was earth-controlled.
Then this period merged very gradually into the stage where life became
possible, and the temperature of the surface became, as it now is,
sun-controlled. How many years are embraced in this span of periods, or
ages, we have no means of knowing. But of the sequence of periods and
the secular diminution of temperature, we may be certain.
Then there is the equally important consideration of water necessary for
the origination, support, and development of life. We cannot conceive of
life existing without it. On the earth water is superabundant, and has
been for indefinite ages in the past. There is little evidence that the
oceans are drying up; although the commonly accepted view is that the
waters of the earth will very gradually disappear. Water can exist in
the fluid state, which is essential to life, at all temperatures between
32 degrees and 680 degrees F.
Air to breathe is essential to life also. The atmosphere which envelops
the earth is at least 100 miles in depth, and its own weight compresses
it to a tension of nearly 15 pounds to the square inch at sea level.
This atmosphere and its physical properties have had everything to do
with the development of animal life on the planet. Without it and its
remarkable property of selective absorption, which imprisons and
diffuses the solar heat, it is inconceivable that the necessary
equability of surface temperature could be maintained. This appears to
be quite independent of the chemical constituents of the atmosphere, and
is perhaps the most important single consideration affecting the
existence of life on a planet. If the surface of a planet is partly
covered with water, it will possess also an atmosphere containing
aqueous vapor.
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