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
If we extend the course which we have proposed, following in the exposition
of the physical description of the earth to the sidereal part of the science
of the Cosmos, the delineation of the regions of space and the bodies by
which they are occupied, we shall find our task simplified in no common
degree. If, according to ancient but unphilosophical forms of nomenclature,
we would distinguish between 'physics', that is to say, general
considerations on the essence of matter, and the forces by which it is
actuated, and 'chemistry', which treats of the nature of substances, their
elementary composition, and those attractions that are not determined solely
by the relations of mass, we must admit that the description of the earth
comprises at
p 63
once 'physical' and 'chemical' actions. In addition to gravitation, which
must be considered as a primitive force in nature, we observe that
attractions of another kind are at work around us, both in the interior of
our planet and on its surface. These forces, to which we apply the term
'chemical affinity', act upon molecules in contact, or at infinitely minute
distances from one another,* and which, being differently modified by
electricity, heat, condensation in porous bodies, or by the contact of an
intermediate substance, animate equally the inorganic world and animal and
vegetable tissues.
[footnote] * On the question already discussed by Newton, regarding the
difference existing between the attraction of masses and molecular
attraction, see Laplace, 'Exposition du Systeme du Monde', p. 384, and
supplement to book x. of the 'Mecanique Celeste', p. 3, 4; Kant, 'Metaph.
Anfangegrunde der Naturwissenschaft, Säm. Werke', 1839, bd. v., s. 309
(Metaphysical Principles of the Natural Sciences); Pectet, 'Physique', 1838,
vol. i., p. 59-63.
If we except the small asteroids, which appear to us under the forms of
aerolites and shooting stars, the regions of space have hitherto presented
to our direct observation physical phenomena alone; and in the case of
these, we know only with certainty the effects depending upon the
quantitative relations of matter of the distribution of masses. The
phenomena of the regions of space may consequently be considered as
influenced by simple dynamical laws -- the laws of motion.
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