last seen oii Jan. 2 2 , but it was so fai:it :tiid 50 far from the computed poiition that it was :lo: observed. Its estimated paition on this day at 8" m . t . was fi -. I 61'13"'27b d \_: + 2 4 p 24' 8. 0 1 1 accoiint of the very unfavorablz wentiler, thc past winter beii:g the severeit linown in
Observations of the Satellites of Mars in the opposition of 1881
โ Scribed by A. Hall
- Publisher
- John Wiley and Sons
- Year
- 1882
- Tongue
- English
- Weight
- 141 KB
- Volume
- 102
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
โฆ Synopsis
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 le rencontre dans d'autres cas, comme le cas actuel, ou evidemment la theorie de la diffraction peut seule l'expliquer.
๐ SIMILAR VOLUMES
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
. 4
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
At the o!iliosition of 1879-80, I measured with the large filar-micrometer of our refractor, a series of groups of the diameters of Mars. These were reduced by Prof. Henry S. Pritchett, (now of Washington University, Saint 1,ouis) and were published in A. N. 2309. At the next opposition, I measured