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
Have the rotation of the planets, and the different degrees of velocity
which the individual zones acquire, according to their respective distances
from the equator, any influence on the distribution of magnetism? Must we
seek the seat of these currents, that is to say, of the disturbed
electricity, in the atmosphere, in the regions of planetary space, or in the
polarity of the Sun and Moon? Galileo, in his celebrated 'Dialogo', was
inclined to ascribe the parallel direction of the axis of the Earth to a
magnetic point of attraction seated in universal space.
If we represent to ourselves the interior of the Earth as fused and
undergoing an enormous pressure, and at a degree of temperature the amount
of which we are unable to assign,
p 190
we must renounce all idea of a magnetic nucleus of the Earth. All magnetism
is certainly not lost until we arrive at a white heat,* and it is manifested
when iron is at a dark red heat, however different, therefore, the
modifications may be which are excited in substances in their molecular
state, and in the coercive force depending upon that condition in
experiments of this nature, there will still remain a considerable thickness
of the terrestrial stratum, which might be assumed to be the seat of
magnetic currents.
[footnote] *Barlow, in the 'Philos. Trans.' for 1822, Pt. i., p. 117; Sir
David Brewster, 'Treatise on Magnetism', p. 129. Long before the times of
Gilbert and Hooke, it was taught in the Chinese work 'Ow-thea-tsou' that
heat diminished the directive force of the magnetic needle. (Klaproth,
'Lettre a M. A. de Humboldt, sur l'Invention de la Boussole', p. 96.)
The old explanation of the horary variations of declination by the
progressive warming of the Earth in the apparent revolution of the Sun from
east to west must be limited to the uppermost surface, since thermometers
sunk into the Earth, which are now being accurately observed at so many
different places, show how slowly the solar heat penetrates even to the
inconsiderable depth of a few feet. Moreover, the thermic condition of the
surface of water, by which two thirds of our planet is covered, is not
favorable to such modes of explanation, when we have reference to an
immediate action and not to an effect of induction in the aërial and
aqueous investment of our terrestrial globe.
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