The Edinburgh Journal of Science
The Edinburgh Journal of Science
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In our eReader you can find the full English version of the book. Read The Edinburgh Journal of Science Online - link to read the book on full screen. Our eReader also allows you to upload and read Pdf, Txt, ePub and fb2 books. In the Mini eReder on the page below you can quickly view all pages of the book - Read Book The Edinburgh Journal of Science
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* Morion, Retrograde. - On the 3d of June, at 8** 54' mean time at Seeberg, this comet will be in 201"^ 41' rigbt ascenBion^ and IBP 08' south declination^ and its distance i^om the earth will be 1.713.
6, First Comet of 1826, or the lost Comet of 1772, — This cornet^ discoTer- ed by M, Biela on the 27th February^ and by M. Gambard on the 9th March^ has been found by M,. Clausen to be the comet of 1805, anc^also thai qf\772, which has been so long lost sight of. He has found its ellip-i tical e...lements to be as follows : Mean Time.
Passage of Perihelion at Altona, 1826, March 18, 49297 Longitudeof Perihelion, r Mean Equinox,^ 109* 53' 29^^.7 LcmgitttdeofNode, 1 Jan. 0.1826, j 251 27 \M Log. Perihelion Distance, .... 0.5496086 Eccentricity. - - = Sun. (48* 12' 28^75) Inclination of Orbit, '- - - 13 32 52 Revolution, ... 2438 Days.
Motion, Direct It is necessary only to suppose a revolution of 2470 days to establish the identity of this comet with that of 1772. We should then have five re- volutions between 1772 and 1805, and three revolutions between 1805 and 1826.
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To quickly assess the difficulty of the text, read a short excerpt:
* Morion, Retrograde. - On the 3d of June, at 8** 54' mean time at Seeberg, this comet will be in 201"^ 41' rigbt ascenBion^ and IBP 08' south declination^ and its distance i^om the earth will be 1.713.
6, First Comet of 1826, or the lost Comet of 1772, — This cornet^ discoTer- ed by M, Biela on the 27th February^ and by M. Gambard on the 9th March^ has been found by M,. Clausen to be the comet of 1805, anc^also thai qf\772, which has been so long lost sight of. He has found its ellip-i tical e...lements to be as follows : Mean Time.
Passage of Perihelion at Altona, 1826, March 18, 49297 Longitudeof Perihelion, r Mean Equinox,^ 109* 53' 29^^.7 LcmgitttdeofNode, 1 Jan. 0.1826, j 251 27 \M Log. Perihelion Distance, .... 0.5496086 Eccentricity. - - = Sun. (48* 12' 28^75) Inclination of Orbit, '- - - 13 32 52 Revolution, ... 2438 Days.
Motion, Direct It is necessary only to suppose a revolution of 2470 days to establish the identity of this comet with that of 1772. We should then have five re- volutions between 1772 and 1805, and three revolutions between 1805 and 1826.
What to read after The Edinburgh Journal of Science?
You can find similar books in the "Read Also" column, or choose other free books by David Brewster to read onlineMoreLess
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