The Science of the StarsMaunder, E. Walter (Edward Walter)
History
The Science of the Stars
Maunder, E. Walter (Edward Walter)
Astronomy
But Mars compares badly with the Earth in another respect. It receives
less light and heat from the Sun in the proportion of three to seven.
This we may express by saying that Mars, on the whole, is almost as
much worse off than the Earth as a point on the Arctic Circle is worse
off than a point on the Equator. The mean temperature of the Earth is
taken as about 60° of the Fahrenheit thermometer (say, 15° Cent.); the
mean temperature of Mars must certainly be considerably below
freezing-point, probably near 0° F. Here on our Earth the
boiling-point of water is 212°, and, since the mean temperature is 60°
and water freezes at 32°, it is normally in the liquid state. On Mars
it must normally be in the solid state--ice, snow, or frost, or the
like. But with so rare an atmosphere water will boil at a low
temperature, and it is not impossible that under the direct rays of the
Sun--that is to say, at midday of the torrid zone of Mars--ice may not
only melt, but water boil by day, condensing and freezing again during
the night. NEWCOMB, the foremost astronomer of his day, concluded
"that during {66} the night of Mars, even in the equatorial regions,
the surface of the planet probably falls to a lower temperature than
any we ever experienced on our globe. If any water exists, it must not
only be frozen, but the temperature of the ice must be far below the
freezing point.... The most careful calculation shows that if there
are any considerable bodies of water on our neighbouring planet, they
exist in the form of ice, and can never be liquid to a depth of more
than one or two inches, and that only within the torrid zone and during
a few hours each day." With regard to the snow caps of Mars, Newcomb
thought it not possible that any considerable fall of snow could ever
take place. He regarded the white caps as simply due to a thin deposit
of hoar frost, and it cannot be deemed wonderful that such should
gradually disappear, when it is remembered that each of the two poles
of Mars is in turn presented to the Sun for more than 300 consecutive
days. Newcomb's conclusion was: "Thus we have a kind of Martian
meteorological changes, very slight indeed, and seemingly very
different from those of our Earth, but yet following similar lines on
their small scale. For snowfall substitute frostfall; instead of (the
barometer reading) feet or inches say fractions of a millimetre, and
instead of storms or wind substitute little motions of an air thinner
than that on the top of the Himalayas, and we shall have a general
description of Martian meteorology."
We conclude, then, that Mars is not so inert a world as the Moon, but,
though some slight changes of climate or weather take place upon it, it
is quite unfitted for the nourishment and development of the different
forms of organic life.
Public-domain text, read in full here on John Shaqi.
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