Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
Kant was illustrious as a metaphysician, but he was a great physicist or
natural philosopher as well, and he set down his ideas regarding the
cosmogony with precision. Learned in the philosophy of the ancients, he
did not follow their speculative conceptions, but merely assumed that
all the materials from which the bodies of the solar system have been
fashioned were resolved into their original elements at the beginning,
and filled all that part of space in which they now move. True, this is
pretty near the chaos of the Greeks, but Kant knew of the operation of
the Newtonian law of gravitation, which the Greeks did not.
As a natural result of gravitative processes, Kant inferred that the
denser portions of the original mass would draw upon themselves the less
dense portions, whirling motions would be everywhere set up, and the
process would continue until many spherical bodies, each with a gaseous
exterior in process of condensation, had taken the place of the original
elements which filled space. In this manner Kant would explain the
sameness in direction of motion, both orbital and axial, of all the
planets and satellites of our system. But many philosophers are of the
opinion that Kant's hypothesis would result, not in the formation of
such a collection of bodies as the solar system is, but rather in a
single central sun formed by common gravitation toward a single center.
From quite another viewpoint the work of the elder Herschel is important
here. No one knew the nebulæ from actual observation better than he did;
but, while his ideas about their composition were wrong, he nevertheless
conceived of them as gradually condensing into stars or clusters of
stars. And it was this speculative aspect of the nebulæ, not as a
possible means of accounting for the birth and development of the solar
system, which constitutes Herschel's chief contribution to the nebular
hypothesis. Classifying the nebulæ which he had carefully studied with
his great telescopes, it seemed obvious to him that they were actually
in all the different stages of condensation, and subsequent research has
strongly tended to substantiate the Herschelian view.
Public-domain text, read in full here on John Shaqi.
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