Rosalind (moon)
Rosalind is a closer moon to Uranus. It was found from the images taken by Voyager 2 on January 13, 1986, and was given the designation S/1986 U 4.[5] It was named after the daughter of the banished Duke in William Shakespeare's play As You Like It. It is also designated Uranus XIII.[6]
| Discovery | |
|---|---|
| Discovered by | Stephen P. Synnott / Voyager 2 |
| Discovery date | January 13, 1986 |
| Orbital characteristics | |
Mean orbit radius | 69,926.795 ± 0.053 km[1] |
| Eccentricity | 0.00011 ± 0.000103[1] |
| 0.558459529 ± 0.000000019 d[1] | |
| Inclination | 0.27876 ± 0.045° (to Uranus' equator)[1] |
| Satellite of | Uranus |
| Physical characteristics | |
| Dimensions | 72 × 72 × 72 km[2] |
Mean radius | 36 ± 6 km[2] |
| ~16,000 km²[3] | |
| Volume | ~200,000 km³[3] |
| Mass | ~2.5×1017 kg[3] |
Mean density | ~1.3 g/cm³ assumed |
| ~0.012 m/s2[3] | |
| ~0.031 km/s[3] | |
| synchronous[2] | |
| zero[2] | |
| Albedo | 0.08 ± 0.01[4] |
| Temperature | ~64 K[3] |
Rosalind belongs to Portia Group of moons, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Belinda and Perdita.[4] These moons have similar orbits and photometric properties.[4] Unfortunately, other than its orbit,[1] radius of 36 km[2] and geometric albedo of 0.08[4] almost nothing is known about it.
At the Voyager 2 images Rosalind appears as an almost spherical object. The ratio of axises of the Rosalind's prolate spheroid is 1.0-0.8.[2] Its surface is grey in color.[2]
References
change- ↑ 1.0 1.1 1.2 1.3 1.4 Jacobson, R.A. (1998). "The Orbits of the Inner Uranian Satellites From Hubble Space Telescope and Voyager2 Observations". The Astronomical Journal. 115 (3): 1195–1199. Bibcode:1998AJ....115.1195J. doi:10.1086/300263. S2CID 118616209.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 Karkoschka, Erich (2001). "Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites". Icarus. 151 (1): 69–77. Bibcode:2001Icar..151...69K. doi:10.1006/icar.2001.6597.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 Calculated on the basis of other parameters
- ↑ 4.0 4.1 4.2 4.3 Karkoschka, Erich (2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope". Icarus. 151 (1): 51–68. Bibcode:2001Icar..151...51K. doi:10.1006/icar.2001.6596.
- ↑ Smith, B. A. (January 16, 1986). "IAU Circular No. 4164". Retrieved 2006-08-06.
- ↑ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 2006-08-06.
Other websites
change- Rosalind Profile Archived 2007-08-01 at the Wayback Machine by NASA's Solar System Exploration
