A Popular History of Astronomy During the Nineteenth Century: Fourth EditionClerke, Agnes M. (Agnes Mary)
History
A Popular History of Astronomy During the Nineteenth Century: Fourth Edition
Clerke, Agnes M. (Agnes Mary)
Astronomy -- History -- 19th century
The fact that comets contract in approaching the sun had been noticed by
Hevelius; Pingré admitted it with hesitating perplexity;[245] the
example of Encke's comet rendered it conspicuous and undeniable. On the
28th of October, 1828, the diameter of the nebulous matter composing
this body was estimated at 312,000 miles. It was then about one and a
half times further from the sun than the earth is at the time of the
equinox. On the 24th of December following, its distance being reduced
by nearly two-thirds, it was found to be only 14,000 miles across.[246]
That is to say, it had shrunk during those two months of approach to
1/11000th part of its original volume! Yet it had still seventeen days'
journey to make before reaching perihelion. The same curious
circumstance was even more markedly apparent at its return in 1838. Its
bulk, or the actual space occupied by it, appeared to be reduced, as it
drew near the hearth of our system, in the enormous proportion of
800,000 to 1. A corresponding expansion accompanied on each occasion its
retirement from the sphere of observation. Similar changes of volume,
though rarely to the same astounding extent, have been perceived in
other comets. They still remain unexplained; but it can scarcely be
doubted that they are due to the action of the same energetic internal
forces which reveal themselves in so many splendid and surprising
cometary phenomena.
Another question of singular interest was raised by Encke's acute
inquiries into the movements and disturbances of the first known "comet
of short period." He found from the first that its revolutions were
subject to some influence besides that of gravity. After every possible
allowance had been made for the pulls, now backward, now forward,
exerted upon it by the several planets, there was still a surplus of
acceleration left unaccounted for. Each return to perihelion took place
about two and a half hours sooner than received theories warranted.
Here, then, was a "residual phenomenon" of the utmost promise for the
disclosure of novel truths. Encke (in accordance with the opinion of
Olbers) explained it as due to the presence in space of some such
"subtle matter" as was long ago invoked by Euler[247] to be the agent of
eventual destruction for the fair scheme of planetary creation. The
apparent anomaly of accounting for an accelerative effect by a retarding
cause disappears when it is considered that any check to the motion of
bodies revolving round a centre of attraction causes them to draw closer
to it, thus shortening their periods and quickening their circulation.
If space were filled with a resisting medium capable of impeding, even
in the most infinitesimal degree, the swift course of the planets, their
orbits should necessarily be, not ellipses, but very close elliptical
spirals along which they would slowly, but inevitably, descend into the
burning lap of the sun. The circumstance that no such tendency can be
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