Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolitesKirkwood, Daniel
Science
Meteoric astronomy: A treatise on shooting-stars, fire-balls, and aerolites
Kirkwood, Daniel
Meteors
1. 1731, March 12th. At Halstead, Essex, England.
2. 1798, March 12th. At Salés, France.
3. 1806, March 15th. At Alais, France.
4. 1807, March 13th. At Timochin, Russia.
5. 1811, March 13th. At Kuleschofka, Russia.
6. 1813, March 13th-14th. The phenomena above described.
7. 1841, March 12th. At Grüneberg, Silesia.
Numerous fire-balls have appeared at the same epoch.
[20] The innermost or semi-transparent ring of Saturn appears to be
similarly constituted, as the body of the planet is seen through it
without any distortion whatever.
[21] Origin of the Stars, p. 173.
[22] Origin of the Stars, p. 184.
[23] Since the above was written Prof. Ennis has informed the author
that, without making any estimate of his own, he adopted the density of
Jupiter's first satellite as given in Lardner's _Handbook of Astronomy_.
[24] Origin of the Stars, p. 77.
[25] Youman's Correlation and Conservation of Forces, p. 244.
[26] Iowa Instructor and School Journal for November, 1866, p. 49.
[27] A recent hypothesis in regard to the temporary star of 1572 has
been proposed by Alexander Wilcocks, M.D., of Philadelphia. See Journ.
Acad. Nat. Sci. of Phila. for 1859.
[28] Gautier's Notice of Recent Researches relating to
Nebulæ.--Silliman's Journal for Jan. 1863, and March, 1864.
[29] Outlines of Astronomy, Art. 442.
[30] A learned and highly interesting examination of this hypothesis
will be found in a memoir "On the Secular Variations and Mutual
Relations of the Orbits of the Asteroids," communicated to the Am.
Acad. of Arts and Sciences, April 24th, 1860, by Simon Newcomb, Esq.
[31] For an explanation of the origin of the asteroids according to
the nebular hypothesis, see an article by David Trowbridge, A.M., in
Silliman's Journal for Nov. 1864, and Jan. 1865.
[32] H. C. Sorby, F.R.S.
[33] Harte's Trans. of Laplace's Syst. of the World, vol. ii., note vii.
[34] Grant's Hist. of Phys. Astr., p. 302.
[35] Nos. 1632 and 1633.
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