๐”– Bobbio Scriptorium
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Names of the satellites of mars

โœ Scribed by A. Hall


Publisher
John Wiley and Sons
Year
1878
Tongue
English
Weight
77 KB
Volume
92
Category
Article
ISSN
0004-6337

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๐Ÿ“œ SIMILAR VOLUMES


On the satellites of mars
โœ A. Marth ๐Ÿ“‚ Article ๐Ÿ“… 1879 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 455 KB ๐Ÿ‘ 2 views

J denoting the inclination of the plane of the satellite's orbit ta the plane of the equator of the epoch, N the rightascension of the node, uo the longitude of the satellite in its orbit reckoned from the node and n the daily. motion. The eccentricities are here disregarded on account of their unce

Observations of the Satellites of Mars
โœ A. Hall ๐Ÿ“‚ Article ๐Ÿ“… 1878 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 121 KB ๐Ÿ‘ 1 views

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Satellites of Mars 1881
โœ A. A. Common ๐Ÿ“‚ Article ๐Ÿ“… 1882 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 88 KB ๐Ÿ‘ 1 views
Photometric Observations of the Satellit
โœ Edward C. Pickering ๐Ÿ“‚ Article ๐Ÿ“… 1882 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 175 KB ๐Ÿ‘ 1 views

The following observatians were made by Mr. 0. C. reading of the photometer, the corresponding difference in Wendell and myself, with the photometer described under magnitude between Mars and the satellite, the average dethe name of Photometer I in Vol. XI of the Annals of the Observatory, attached

Satellites of Mars in 1881
โœ A. Hall ๐Ÿ“‚ Article ๐Ÿ“… 1882 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 74 KB ๐Ÿ‘ 1 views

Diese sowie verschiedene folgende Mittheilungen sind hier druckt ; es ist deshalb unnothig, die Beilage aufzubewahren. An hour later, I thought Phobus was visible, also near the computed position, but could not be certain of it. These satellites can be observed therefore for nearly two months duri

Observations of the Satellites of Mars i
โœ A. Hall ๐Ÿ“‚ Article ๐Ÿ“… 1882 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 141 KB ๐Ÿ‘ 1 views

I 3 19.4 10 3.8 1 0 29.3 '3 22.3 Ce phenomkne est donc completement analogue P celui qui se produit lors des passages des planetes inferieures sur le disque solaire: et, les observations precedentes montrent que le ligament noir n'est point, pour ainsi dire, une caracteristique de ces passages. On l