The Hubble Space Telescope captured tiny Rosalind orbiting Uranus in 1997
Discovery
Discovered by
Stephen P. Synnott / Voyager 2
Discovery date
January 13, 1986
Designations
Designation
Uranus XIII
Pronunciation
/ˈrɒzələnd/[1]
Adjectives
Rosalindian /rɒzəˈlɪndiən/[2]
Orbital characteristics
Mean orbit radius
69,926.795 ± 0.053 km[3]
Eccentricity
0.00011 ± 0.000103[3]
Orbital period
0.558459529 ± 0.000000019 d[3]
Inclination
0.27876 ± 0.045° (to Uranus' equator)[3]
Satellite of
Uranus
Group
ring shepherd
Physical characteristics
Dimensions
72 × 72 × 72 km[4]
Mean radius
36 ± 6 km[4][5][6]
Surface area
~16,000 km2[lower-alpha 1]
Volume
~200,000 km3[lower-alpha 1]
Mass
~2.5×1017 kg[lower-alpha 1]
Mean density
~1.3 g/cm3 (assumed)[5]
surface gravity
~0.012 m/s2[lower-alpha 1]
escape velocity
~0.031 km/s[lower-alpha 1]
Rotation period
synchronous[4]
Axial tilt
zero[4]
Albedo
0.08 ± 0.01[7]
Physics
~64 K[lower-alpha 1]
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.[8] 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.[9]
Rosalind belongs to Portia group of satellites, which also includes Bianca, Cressida, Desdemona, Portia, Juliet, Cupid, Belinda and Perdita.[7] These satellites have similar orbits and photometric properties.[7] Other than its orbit,[3] radius of 36 km[4] and geometric albedo of 0.08[7] 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.[10]
See also
Moons of Uranus
References
Explanatory notes
↑ 1.01.11.21.31.41.5 Calculated on the basis of other parameters.
Citations
↑Benjamin Smith (1903) The Century Dictionary and Cyclopedia
↑Bertrand Evans (1966) Teaching Shakespeare in the high school, p. 213
↑ 3.03.13.23.33.4Jacobson, R. A. (1998). "The Orbits of the Inner Uranian Satellites From Hubble Space Telescope and Voyager 2 Observations". The Astronomical Journal115 (3): 1195–1199. doi:10.1086/300263. Bibcode: 1998AJ....115.1195J.
↑ 4.04.14.24.34.44.54.6Karkoschka, Erich (2001). "Voyager's Eleventh Discovery of a Satellite of Uranus and Photometry and the First Size Measurements of Nine Satellites". Icarus151 (1): 69–77. doi:10.1006/icar.2001.6597. Bibcode: 2001Icar..151...69K.
↑ 5.05.1"Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 24 October 2008. http://ssd.jpl.nasa.gov/?sat_phys_par.
↑Williams, Dr. David R. (23 November 2007). "Uranian Satellite Fact Sheet". NASA (National Space Science Data Center). http://nssdc.gsfc.nasa.gov/planetary/factsheet/uraniansatfact.html.
↑ 7.07.17.27.3Karkoschka, Erich (2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope". Icarus151 (1): 51–68. doi:10.1006/icar.2001.6596. Bibcode: 2001Icar..151...51K.
↑Smith, B. A. (1986-01-16). "Satellites of Uranus". IAU Circular4164. http://www.cbat.eps.harvard.edu/iauc/04100/04164.html#Item1. Retrieved 2011-11-01.
↑"Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. http://planetarynames.wr.usgs.gov/Page/Planets.
↑Murray, Carl D.; Thompson, Robert P. (1990-12-06). "Orbits of shepherd satellites deduced from the structure of the rings of Uranus". Nature348 (6301): 499–502. doi:10.1038/348499a0. ISSN 0028-0836. Bibcode: 1990Natur.348..499M.
External links
Rosalind Profile by NASA's Solar System Exploration
Uranus' Known Satellites (by Scott S. Sheppard)
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