Biographies of Distinguished Scientific Men eBook

This eBook from the Gutenberg Project consists of approximately 471 pages of information about Biographies of Distinguished Scientific Men.

Biographies of Distinguished Scientific Men eBook

This eBook from the Gutenberg Project consists of approximately 471 pages of information about Biographies of Distinguished Scientific Men.

It was Buffon, I think, who first attempted to explain this singular feature of our solar system.  Having wished, in the explanation of phenomena, to avoid all recourse to causes which were not warranted by nature, the celebrated academician investigated a physical origin of the system in what was common to the movements of so many bodies differing in magnitude, in form, and in distance from the principal centre of attraction.  He imagined that he discovered such an origin by making this triple supposition:  a comet fell obliquely upon the sun; it pushed before it a torrent of fluid matter; this substance transported to a greater or less distance from the sun according to its mass formed by concentration all the known planets.

The bold hypothesis of Buffon is liable to insurmountable difficulties.  I proceed to indicate, in a few words, the cosmogonic system which Laplace substituted for that of the illustrious author of the Histoire Naturelle.

According to Laplace, the sun was at a remote epoch the central nucleus of an immense nebula, which possessed a very high temperature, and extended far beyond the region in which Uranus revolves in the present day.  No planet was then in existence.

The solar nebula was endued with a general movement of revolution directed from west to east.  As it cooled it could not fail to experience a gradual condensation, and, in consequence, to rotate with greater and greater rapidity.  If the nebulous matter extended originally in the plane of the equator as far as the limit at which the centrifugal force exactly counterbalanced the attraction of the nucleus, the molecules situate at this limit ought, during the process of condensation, to separate from the rest of the atmospheric matter and form an equatorial zone, a ring revolving separately and with its primitive velocity.  We may conceive that analogous separations were effected in the higher strata of the nebula at different epochs, that is to say, at different distances from the nucleus, and that they give rise to a succession of distinct rings, included almost in the same plane and endued with different velocities.

This being once admitted, it is easy to see that the indefinite stability of the rings would have required a regularity of structure throughout their whole contour, which is very improbable.  Each of them accordingly broke in its turn into several masses, which were plainly endued with a movement of rotation, coinciding in direction with the common movement of revolution, and which in consequence of their fluidity assumed spheroidal forms.

In order, then, that one of those spheroids might absorb all the others belonging to the same ring, it will be sufficient to assign to it a mass greater than that of any other spheroid.

Each of the planets, while in the vaporous condition to which we have just alluded, would manifestly have a central nucleus gradually increasing in magnitude and mass, and an atmosphere offering, at its successive limits, phenomena entirely similar to those which the solar atmosphere, properly so called, had exhibited.  We here witness the birth of satellites, and that of the ring of Saturn.

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Biographies of Distinguished Scientific Men from Project Gutenberg. Public domain.