Are the Planets Inhabited?Maunder, E. Walter (Edward Walter)
Science
Are the Planets Inhabited?
Maunder, E. Walter (Edward Walter)
Life on other planets
But if we turn back to the Table, we see that Jupiter at its mean distance
from the Sun is 5·2 times that of the Earth; that is to say, it receives
only 1/27th of the light and heat that we receive. But in Chapter VIII, we
learnt from Mars that as this receives only 3/7ths of the Earth's light
and heat, its mean temperature would sink to -30°C.; the Earth's being
16°C. Mars is therefore almost always a frozen planet; frozen except on
its mere surface when this is exposed to the full rays of the Sun. No sea
there would ever be melted to a depth of more than a few inches, even at
noonday in midsummer. And yet Mars has at least ten times the advantages
of Jupiter. Jupiter, then, must be a frozen planet through and through; no
liquid of any sort can exist on its surface; no vapour of any substance
can exist in its atmosphere. It must be icebound even at its summer
noonday.
Yet, from the description given by Prof. Keeler, it is manifestly not so;
and another item in the Table emphasizes that it cannot be so. The density
of the Sun is 1·4 that of water, Jupiter's is 1·33, showing that but a
very small proportion (if any) of its bulk can be solid; the rest must be
vaporous, or at least fluid. How then can we reconcile these
inconsistencies?
It is in the dimensions of Jupiter that we find the answer. The mass of
the planet is 317 times that of the Earth; it is indeed nearly three times
as great as that of all the other planets put together. But the
aggregation of so vast an amount of material is of itself a source of
heat; the chief source at the present time of the enormous output of heat
from the Sun is ascribed to its gradual contraction; the slow falling of
its substance, if we may so express it, a little nearer to its centre. The
great mass of Jupiter points to its inherent store of heat being much
greater than that of any other planet. And of two bodies equally hot, the
larger must cool more slowly than the smaller. If, therefore, all the
members of the solar system had at one and the same moment possessed the
same surface temperature, that equality would have ceased directly they
began to radiate their heat into space; the temperature of the smaller
bodies falling more rapidly than those of the larger. This is another
example of the principle that has already been noted, that the properties
of a small world are not those of a large world divided by a constant
factor. It is not possible to conceive a model of the solar system in
which all the significant factors should be true to the same scale. If the
diameters and distances were all made on a one-tenth scale, the surfaces
would be one-hundredth of reality, the volumes one-thousandth.
But a radiating body radiates from its surface, while the store of heat
from which that radiation is kept up is supplied by its volume. It
follows, therefore, that a large and heavy world must differ from a small
light world, not merely in scale, but also in kind.
Public-domain text, read in full here on John Shaqi.
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