Rosalind (moon)

Source: Wikipedia, the free encyclopedia.
There is also an asteroid called 900 Rosalinde.
Rosalind
Synodic rotation period
synchronous[4]
zero[4]
Albedo0.08 ± 0.01[8]
Temperature~64 K[a]
  1. ^ Only two dimensions are known; the third dimension has been assumed to equal the other two.

Rosalind 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.[9] 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.[10]

Rosalind belongs to Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Belinda and Perdita.[8] These satellites have similar orbits and photometric properties.[8] Other than its orbit,[3] radius of 36 km[4] and geometric albedo of 0.08[8] 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.[4] Its surface is grey in color.[4]

Rosalind is very close to a 3:5 orbital resonance with Cordelia.[11]

See also

Notes

  1. ^ a b c d e f Calculated on the basis of other parameters.

References

  1. ^ Benjamin Smith (1903). The Century Dictionary and Cyclopedia.
  2. ^ Bertrand Evans (1966). Teaching Shakespeare in the high school. p. 213.
  3. ^ a b Jacobson, R. A. (1998). "The Orbits of the Inner Uranian Satellites From Hubble Space Telescope and Voyager 2 Observations". The Astronomical Journal. 115 (3): 1195–1199.
    S2CID 118616209
    .
  4. ^ a b c d e f .
  5. ^ "Planetary Satellite Physical Parameters".
    JPL (Solar System Dynamics). 24 October 2008. Retrieved 12 December 2008.{{cite web}}: CS1 maint: url-status (link
    )
  6. ^ Williams, Dr. David R. (23 November 2007). "Uranian Satellite Fact Sheet". NASA (National Space Science Data Center). Retrieved 12 December 2008.
  7. .
  8. ^ a b c d .
  9. ^ Smith, B. A. (1986-01-16). "Satellites of Uranus". IAU Circular. 4164. Retrieved 2011-11-01.
  10. ^ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 6 August 2006.
  11. ^ Murray, Carl D.; Thompson, Robert P. (1990-12-06). "Orbits of shepherd satellites deduced from the structure of the rings of Uranus". Nature. 348 (6301): 499–502.
    S2CID 4320268
    .

External links