Worlds in the making: The evolution of the universe — John Shaqi
Worlds in the making: The evolution of the universeArrhenius, Svante
Science
Worlds in the making: The evolution of the universe
Arrhenius, Svante
Cosmogony
[Footnote 4: According to the opinion of a colleague of mine,
a botanist, the results of the experiments of Phipson must be
regarded as very doubtful, and some oxygen would appear to be
indispensable for the growth of plants. We have to imagine the
development somewhat as follows: As the earth separated from
the solar nebula, its temperature was very high at first in its
outer portions. At this temperature it was not able to retain
the lighter gases, like hydrogen and helium, for a long period;
the heavy gases, like nitrogen and oxygen, remained. The
original excess of hydrogen and helium disappeared, therefore,
before the crust of the earth had been formed, and the
atmosphere of the earth immediately after the formation of the
crust contained some oxygen, besides much nitrogen, carbonic
acid, and water vapor. The main bulk of the actual atmospheric
oxygen would therefore have been reduced from carbon dioxide by
the intermediation of plants. The view that celestial bodies
may lose part of their atmosphere is due to Johnstone Stoney.
The atmospheric gases escape the more rapidly the lighter their
molecules and the smaller the mass of the celestial bodies. On
these lines we explain that the smaller celestial bodies like
the moon and Mercury, have lost almost all their atmosphere,
while the earth has only lost hydrogen and helium, which again
have been retained by the sun.]
This oxygen is an essential element for the production of animal life.
As animal life stands above vegetable life, so animal life could only
originate at a later stage than plant life. Plants require, in addition
to suitable temperature, only carbonic acid and water, and these
gases will probably be found in the atmospheres of all the planets
as exhalations of their inner incandescent masses which are slowly
cooling. The presence of water vapor has directly been established, by
means of the spectroscope, in the atmospheres of other planets—Venus,
Jupiter, and Saturn—and indirectly by the observation of a snow-cap on
Mars. The spectroscope further gives us indication of the presence of
other gases. There is an intense band in the red part of the spectra of
Jupiter and Saturn, of wave-length 0.000618 mm. Other new constituents
of unknown nature have been discerned in the spectra of Uranus and
Neptune. On the other hand, there is hardly any, or at any rate only
a quite insignificant, atmosphere on the moon and on Mercury. This
is easily understood. The temperature on that side of Mercury which
is turned away from the sun is near absolute zero. All the gases of
the planetary atmosphere would collect and condense there. If, then,
Mercury had originally an atmosphere, it must have lost it as it lost
its own rotation, compelling it to turn always the same face towards
the sun. Similar reasons may account for the absence of a lunar
atmosphere.
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