Popular lectures on scientific subjects : $b Second series, with an autobiography of the authorHelmholtz, Hermann von
Science
Popular lectures on scientific subjects : $b Second series, with an autobiography of the author
Helmholtz, Hermann von
Science; Universities and colleges -- Germany
In the course of the eighteenth century the power of mathematical
analysis, and the methods of astronomical observation, increased
so far that all the complicated actions, which take place between
all the planets, and all their satellites, in consequence of
the mutual action of each upon each, and which astronomers call
disturbances--disturbance, that is to say, of the simpler elliptical
motions about the sun, which each one would produce if the others were
absent--that all these could be theoretically predicted from Newton’s
law, and be accurately compared with what actually takes place in the
heavens. The development of this theory of planetary motion in detail
was, as has been said, the merit of Laplace. The agreement between this
theory, which was developed from the simple law of gravitation, and the
extremely complicated and manifold phenomena which follow therefrom,
was so complete and so accurate, as had never previously been attained
in any other branch of human knowledge. Emboldened by this agreement,
the next step was to conclude that where slight defects were still
constantly found, unknown causes must be at work. Thus, from Bessel’s
calculation of the discrepancy between the actual and the calculated
motion of Uranus, it was inferred that there must be another planet.
The position of this planet was calculated by Leverrier and Adams,
and thus Neptune, the most distant of all known at that time, was
discovered.
But it was not merely in the region of the attraction of our sun that
the law of gravitation was found to hold. With regard to the fixed
stars, it was found that double stars moved about each other in
elliptical paths, and that therefore the same law of gravitation must
hold for them as for our planetary system. The distance of some of
them could be calculated. The nearest of them, α, in the constellation
of the Centaur, is 270,000 times further from the sun than the earth.
Light, which has a velocity of 186,000 miles a second, which traverses
the distance from the sun to the earth in eight minutes, would take
four years to travel from α Centauri to us. The more delicate methods
of modern astronomy have made it possible to determine distances which
light would take thirty-five years to traverse; as, for instance, the
Pole Star; but the law of gravitation is seen to hold, ruling the
motion of the double stars, at distances in the heavens, which all the
means we possess have hitherto utterly failed to measure.
Public-domain text, read in full here on John Shaqi.
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