The Edinburgh New Philosophical Journal, Vol. XLIX: April-October 1850Various
Science
The Edinburgh New Philosophical Journal, Vol. XLIX: April-October 1850
Various
Science -- Periodicals
The fact of axial rotations being the groundwork of Kirkwood's analogy
seems fatal to it, for gravitation takes no more account of the time
of rotation of a planet than it does of specific gravity; all
calculations of the movement of the body in space are equally
independent of the one and the other.
Under these circumstances, the degree of accuracy with which it may be
found to apply is the only saving clause. Messrs Walker and Gould
investigating the subject independently, and with better constants of
mass and distance than Kirkwood had been able to procure, declare that
it appears _perfectly_! We are sorry that the late hour at which we
have received this paper has prevented us either from giving it in
full, or from testing the theory rigidly.
It will be observed that, according to Kirkwood's theory, in order to
compute the time of axial rotations of any planet, it is necessary to
have its mass and mean distance, together with the same quantities for
the planets on either side of it. Now, these quantities are only
obtainable for Venus, the Earth, Saturn, and Uranus (a planet being
lost between Mars and Jupiter); and the rotation of Uranus not having
been obtained as yet, there remains only the three first by which the
theory can be tested.
In a preliminary calculation which we have instituted, we do not find
the results so accordant as we had been led to expect, but still
sufficiently so to give a certain probability of the approach to
truth, in a case where the quantity had not been observed.
Viewed in this light, some very interesting results are obtained.
_1st_, The idea entertained by Bianchini and other observers, that the
rotation of Venus is nearly 24 times as long as hitherto supposed, is
utterly untenable.
_2d_, The time of rotation of Uranus, a quantity never yet observed
(but doubtless capable of being observed by a telescope of Lord
Rosse's calibre, _removed to a table-land in a tropical country_) is
given; and appears so very different from any other yet observed,
especially so from those of its neighbours Saturn and Jupiter, being =
1·396779, earth's = 0·997270 (sidereal rotation in mean solar days.)
_3d_, Knowing the rotations of Jupiter and Mars, we may supply, by
using the analogy conversely, the _diameters of their spheres of
attraction_, and thus get at the elements of the lost planet between
Mars and Jupiter, and these appear to be:--mean distance = 2·9085111
(earth unity), mass in terms of Sun 1/1353240, sidereal rotation in
earth's mean solar days 2·406104, and diameter of sphere of attraction
0·830951, in terms of earth's distance. The size is thus a little
larger than Mars. The slowness of rotation is remarkable, especially
in the case of a planet which is supposed since to have burst into
pieces: the Americans have called it Kirkwood. P. S.
SCIENTIFIC INTELLIGENCE.
METEOROLOGY.
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