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.
Ephemerides of the five inner satellites of Saturn (continued) and of the outer satellite Japetus 1881-1882
โ Scribed by A. Marth
- Publisher
- John Wiley and Sons
- Year
- 1881
- Tongue
- English
- Weight
- 97 KB
- Volume
- 100
- Category
- Article
- ISSN
- 0004-6337
No coin nor oath required. For personal study only.
โฆ Synopsis
Ephemerides of the five inner Satellites of Sntiirn (continued) and of the ontei. Satellite Japetus 1881-1882. Hy A. i v a ~t h .
The longitudes of Mimas are deduced from the elements adopted in last years ephemeris without alteration as the conflicting statements of several observers respecting the place of the satellite cannot at present be reconciled and the true correction required is uncertain. T h e three conjunctions of Mimas with the ends of the ring, observed at Toulouse and published in Comptes Kendus of 9 Mai 1881 p. 1099, show the differences: Sept. 28 I I" 01"33' sp Baillaud 302087 + 8028 29 9 5 1 I I sp B 306.53 + 4.62 Nov. 25 10 23 5 0 zf Fabre 1 3 2 . 1 5 -1.00, the assumed length of the ring being that indicated by conjunctions of the other satellites observed at Toulouse in 1876 and 77. An uncertainty of 4 or 5 minutes in the estimated time of a conjunction of Mimas corresponds to an uncertainty of 1006 or 1ยฐ33 in the longi-1880 Tonl. m. t. Obsen er Calc. elong. Obs. -Elih.
๐ SIMILAR VOLUMES
## 328 welcher nur St6rungsglieder der zweiten Ordnung. ent,htilt, eine solclie Darstellung, dass er aus Quadraten besteht, welche bestiindige Coeffizienten haben. Zunachst ist : X i) -2 = (g + 2 e cos v y -$. Die rorige Gleichung geht dann 16 Wir setzen nun 4 fiber in: Differentiirt man die Glei
Nphemerides of the fiye inner Satellites of Saturn. 1878. By A. Martis. (Fortsetzung.) Greenwioc mean time. 1878. Aug. 10 6h2 Te. nf.