Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1Humboldt, Alexander von
History
Cosmos: A Sketch of the Physical Description of the Universe, Vol. 1
Humboldt, Alexander von
Astronomy; Cosmography; Physical geography; Science -- History
I apply the term 'volcanic', in the widest sense of the word, to every
action exercised by the interior of a planet on its external crust. The
surface of our globe, and that of the moon, manifest traces of this action,
which in the former, at least, has varied during the course of ages. Those
who are ignorant of the fact that the internal heat of the earth increases
so rapidly with the increase of depth that granite is in a state of fusion
about twenty or thirty geographical miles below the surface,* can not have a
clear conception of the causes, and the simultaneous occurrence of volcanic
eruptions at places widely removed from one another, or of the extent and
intersection of 'circles of commotion' in earthquakes, or of the uniformity
of temperature, and equality of chemical composition observed in thermal
springs during a long course of years.
[Footnote] * The determinations usually given of the point of fusion are in
general much too high for refracting substances. According to the very
accurate researches of Mitscherlich, the melting point of granite can hardly
exceed 2372 degrees F.
[Dr. Mantell states in 'The Wonders of Geology', 1848, vol. i., p. 34, that
this increase of temperature amounts to 1 degree of Fahrenheit for every
fifty-four feet of vertical depth.] -- Tr.
The quantity of heat peculiar to a planet is, however, a matter of such
importance -- being the result of its primitive condensation, and varying
according to the nature and duration of the radiation -- that the study of
this subject may throw some degree of light on the history of the
atmosphere, and the distribution of the organic bodies imbedded in the solid
crust of the earth. This study enables us to understand how a tropical
temperature, independent of latitude (that is, of the distance from the
poles), may have been produced by deep fissures remaining open, and exhaling
heat from the interior
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of the globe, at a period when the earth's crust was still furrowed and
rent, and only in a state of semi-solidification; and a primordial condition
is thus revealed to us, in which the temperature of the atmosphere, and
climates generally, were owing rather to a liberation of caloric and of
different gaseous emanations (that is to say, rather to the energetic
reaction of the interior on the exterior) than to the position of the earth
with respect to the central body, the sun.
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