The Book of History (Vol. 1 of 18): A History of All Nations from the Earliest Times to the PresentVarious
History
The Book of History (Vol. 1 of 18): A History of All Nations from the Earliest Times to the Present
Various
World history
It is now believed that the amount of atmosphere possessed by a
planet is due mainly, perhaps entirely, to the planet’s mass, and its
consequent gravitative power. Spectrum-analysis has shown that vast
masses of gaseous matter exist in the universe, and it is probable
that, in a state of extreme tenuity, these are very widely diffused.
Just as meteoric dust is constantly attracted to the earth, and
periodically in larger quantities, so are gases, and supposing the
aggregations of free gaseous matter to have been distributed with some
approach to uniformity, then, as planets grew in size, they would also
tend to secure a larger amount of the diffused gases, thus forming
deeper atmospheres. The observed facts agree with this view. The
largest planets, Jupiter and Saturn, have such a depth of atmosphere as
permanently to obscure any solid interior they may possess. The only
planet closely approaching the earth in size and density--Venus--has
an atmosphere which appears to be loftier than ours, but it may be
composed of different gases. Mars, which has only one-ninth the mass
of the earth, has a lofty but very tenuous atmosphere, and probably no
water, the Polar snows being due probably to the freezing of some dense
gas. The climate and physical condition of Mars is, however, still a
subject of much controversy, which I hope to discuss in a separate work
dealing with the arguments of Professor Lowell [see page 105]. In that
volume the reader will find, fully set forth my reasons, on scientific
grounds, against the supposed habitability of Mars.
[Sidenote: The Earth Selects and Uses Gas]
But, besides attracting cosmic masses of gaseous matter to form its
atmosphere, there is another equally important function of the mass of
a planet--its selective power on the kind of gases it can permanently
retain in a free state. The molecules of gases are in a condition of
rapid motion in all directions, which explains the elastic force they
exhibit. The speed of this motion has been determined for all the chief
gases, and also the gravitative force necessary to prevent them from
continually escaping into space from the upper limit of the atmosphere.
Thus the moon, which has a mass only one-eightieth that of the earth,
can retain no free gas whatever on its surface. Mars can retain only
the very heavy gases, but neither hydrogen nor water-vapour. The earth,
however, has force enough to retain all the gases except hydrogen,
which is just beyond its limit; and this may explain why it is that
there is no free hydrogen in the atmosphere, although this gas is
continually produced in small quantities by submarine volcanoes, is
emitted sometimes from fissures in volcanic regions, and is a product
of decaying vegetation. Once united with oxygen to form water, it
becomes amenable to gravity in the form of invisible aqueous vapour,
and is thenceforth a permanent possession for us in its most valuable
form.
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