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
Data for computing the position of the satellites of mars 1879
โ Scribed by A. Marth
- Publisher
- John Wiley and Sons
- Year
- 1879
- Tongue
- English
- Weight
- 252 KB
- Volume
- 96
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
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
. 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
Ephemerides of the fiye inner Satellites of Saturn 1879. By A. Murth. Longitudes of the satellites reckoned in their orbits from the points which are in superior conjunction with the planet's centre.