Outlines of the Earth's History: A Popular Study in PhysiographyShaler, Nathaniel Southgate
History
Outlines of the Earth's History: A Popular Study in Physiography
Shaler, Nathaniel Southgate
Physical geography
It is now time to give some account as to what is known concerning the
general conditions of the solar bodies--the planets and satellites of
our own celestial group. For our purpose we need attend only to the
general physical state of these orbs so far as it is known to us by
the studies of astronomers. The nearest planet to the sun is Mercury.
This little sphere, less than half the diameter of our earth, is so
close to the sun that even when most favourably placed for observation
it is visible for but a few minutes before sunrise and after sunset.
Although it may without much difficulty be found by the ordinary eye,
very few people have ever seen it. To the telescope when it is in the
_full moon_ state it appears as a brilliant disk; it is held by most
astronomers that the surface which we see is made up altogether of
clouds, but this, as most else that has been stated concerning this
planet, is doubtful. The sphere is so near to the sun that if it were
possessed of water it would inevitably bear an atmosphere full of
vapour. Under any conceivable conditions of a planet placed as
Mercury is, provided it had an atmosphere to retain the heat, its
temperature would necessarily be very high. Life as we know it could
not well exist upon such a sphere.
Next beyond Mercury is Venus, a sphere only a little less in diameter
than the earth. Of this sphere we know more than we do of Mercury, for
the reason that it is farther from the sun and so appears in the
darkened sky. Most astronomers hold that the surface of this planet
apparently is almost completely and continually hidden from us by what
appears to be a dense cloud envelope, through which from time to time
certain spots appear of a dark colour. These, it is claimed, retain
their place in a permanent way; it is, indeed, by observing them that
the rotation period of the planet has, according to some observers,
been determined. It therefore seems likely that these spots are the
summits of mountains, which, like many of our own earth, rise above
the cloud level.
Recent observations on Venus made by Mr. Percival Lowell appear to
show that the previous determinations of the rotation of that planet,
as well as regards its cloud wrap, are in error. According to these
observations, the sphere moves about the sun, always keeping the same
side turned toward the solar centre, just as the moon does in its
motion around the earth. Moreover, Mr. Lowell has failed to discover
any traces of clouds upon the surface of the planet. As yet these
results have not been verified by the work of other astronomers;
resting, however, as they do on studies made with an excellent
telescope and in the very translucent and steady air of the Flagstaff
Station, they are more likely to be correct than those obtained by
other students. If it be true that Venus does not turn upon its axis,
such is likely to be the case also with the planet Mercury.
Public-domain text, read in full here on John Shaqi.
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