The Hubble Space Telescope captured tiny Rosalind orbiting Uranus in 1997
|
|
|
Discovery
|
|
|---|---|
| Discovered by | Stephen P. Synnott / Voyager 2 |
| Discovery date | January 13, 1986 |
| Mean orbit radius | 69,926.795 ± 0.053 km[1] |
| Eccentricity | 0.00011 ± 0.000103[1] |
| Orbital period | 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][3][4] |
| Surface area | ~16,000 km²[a] |
| Volume | ~200,000 km³[a] |
| Mass | ~2.5×1017 kg[a] |
| Mean density | ~1.3 g/cm³ (assumed)[3] |
| Equatorial surface gravity | ~0.012 m/s²[a] |
| Escape velocity | ~0.031 km/s[a] |
| Rotation period | synchronous[2] |
| Axial tilt | zero[2] |
| Albedo | 0.08 ± 0.01[5] |
| Temperature | ~64 K[a] |
Rosalind (
/ˈrɒzəlɨnd/ ROZ-ə-lind) is an inner satellite of Uranus. It was discovered from the images taken by Voyager 2 on 13 January 1986, and was given the temporary designation S/1986 U 4.[6] 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.[7]
Rosalind belongs to Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Belinda and Perdita.[5] These satellites have similar orbits and photometric properties.[5] Other than its orbit,[1] radius of 36 km[2] and geometric albedo of 0.08[5] virtually nothing is known about Rosalind.
In the Voyager 2 images Rosalind appears as an almost spherical object. The ratio of axes of Rosalind's prolate spheroid is 0.8-1.0.[2] Its surface is grey in color.[2]
Rosalind is very close to a 3:5 orbital resonance with Cordelia.[8]
Explanatory notes
Citations
|
|||||||||||||||||||||||
|
|||||||||||||||||
This entry is from Wikipedia, the leading user-contributed encyclopedia. It may not have been reviewed by professional editors (see full disclaimer)