The Certainty of a Future Life in Mars: Being the Posthumous Papers of Bradford Torrey DoddGratacap, L. P. (Louis Pope)
Science
The Certainty of a Future Life in Mars: Being the Posthumous Papers of Bradford Torrey Dodd
Gratacap, L. P. (Louis Pope)
Mars (Planet) -- Fiction; Science fiction
Accordingly, as far as we may be permitted to argue from the observed
facts, the climate of Mars must resemble that of a clear day upon a high
mountain. By day a very strong solar radiation, hardly mitigated at all
by mist or vapor; by night a copious radiation from the soil toward
celestial space, and because of that a very marked refrigeration. Hence
a climate of extremes, and great changes of temperature from day to
night, and from one season to another. And as on the earth at altitudes
of 5,000 and 6,000 meters (17,000 to 20,000 feet) the vapor of the
atmosphere is condensed only into the solid form, producing those
whitish masses of suspended crystals which we call cirrus clouds, so in
the atmosphere of Mars it would be rarely possible (or would even be
impossible) to find collections of cloud capable of producing rain of
any consequence. The variation of the temperature from one season to
another would be notably increased by their long duration, and thus we
can understand the great freezing and melting of the snow which is
renewed in turn at the poles at each complete revolution of the planet
around the sun.
As our chart demonstrates, in its general topography Mars does not
present any analogy with the earth. A third of its surface is occupied
by the great Mare Australe, which is strewn with many islands, and the
continents are cut up by gulfs, and ramifications of various forms. To
the general water system belongs an entire series of small internal
seas, of which the Hadriacum and the Tyrrhenum communicate with it by
wide mouths, whilst the Cimmerium, the Sirenum, and the Solis Lacus are
connected with it only by means of narrow canals. We shall notice in
the first four a parallel arrangement, which certainly is not
accidental, as also not without reason is the corresponding position of
the peninsulas of Ausonia, Hesperia, and Atlantis. The color of the seas
of Mars is generally brown, mixed with gray, but not always of equal
intensity in all places, nor is it the same in the same place at all
times. From an absolute black it may descend to a light-gray or to an
ash color. Such a diversity of colors may have its origin in various
causes, and is not without analogy also upon the earth, where it is
noted that the seas of the warm zone are usually much darker than those
nearer the pole. The water of the Baltic, for example, has a light,
muddy color that is not observed in the Mediterranean. And thus in the
seas of Mars we see the color become darker when the sun approaches
their zenith, and summer begins to rule in that region.
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