Rosalind (moon)

Rosalind
	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/
Adjectives	Rosalindian /rɒzəˈlɪndiən/
Orbital characteristics
Mean orbit radius	69,926.795 ± 0.053 km
Eccentricity	0.00011 ± 0.000103
Orbital period	0.558459529 ± 0.000000019 d
Inclination	0.27876 ± 0.045° (to Uranus' equator)
Satellite of	Uranus
Group	ring shepherd
Physical characteristics
Dimensions	72 × 72 × 72 km
Mean radius	36 ± 6 km
Surface area	~16,000 km2
Volume	~200,000 km3
Mass	~2.5×1017 kg
Mean density	~1.3 g/cm3 (assumed)
surface gravity	~0.012 m/s2
escape velocity	~0.031 km/s
Rotation period	synchronous
Axial tilt	zero
Albedo	0.08 ± 0.01
Physics	~64 K

Short description: Moon of Uranus

There is also an asteroid called 900 Rosalinde.

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]

References

Explanatory notes

↑ ^1.0 ^1.1 ^1.2 ^1.3 ^1.4 ^1.5 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
↑ ^3.0 ^3.1 ^3.2 ^3.3 ^3.4 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. doi:10.1086/300263. Bibcode: 1998AJ....115.1195J.
↑ ^4.0 ^4.1 ^4.2 ^4.3 ^4.4 ^4.5 ^4.6 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. doi:10.1006/icar.2001.6597. Bibcode: 2001Icar..151...69K.
↑ ^5.0 ^5.1 "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.
↑ ^7.0 ^7.1 ^7.2 ^7.3 Karkoschka, Erich (2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope". Icarus 151 (1): 51–68. doi:10.1006/icar.2001.6596. Bibcode: 2001Icar..151...51K.
↑ Smith, B. A. (1986-01-16). "Satellites of Uranus". IAU Circular 4164. 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". Nature 348 (6301): 499–502. doi:10.1038/348499a0. ISSN 0028-0836. Bibcode: 1990Natur.348..499M.

External links

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Original source: https://en.wikipedia.org/wiki/Rosalind (moon). Read more

[calculated-7] 1.0 ^1.1 ^1.2 ^1.3 ^1.4 ^1.5 Calculated on the basis of other parameters.

[1] Benjamin Smith (1903) The Century Dictionary and Cyclopedia

[2] Bertrand Evans (1966) Teaching Shakespeare in the high school, p. 213

[Jacobson_1998-3] 3.0 ^3.1 ^3.2 ^3.3 ^3.4 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. doi:10.1086/300263. Bibcode: 1998AJ....115.1195J.

[Karkoschka,_Voyager_2001-4] 4.0 ^4.1 ^4.2 ^4.3 ^4.4 ^4.5 ^4.6 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. doi:10.1006/icar.2001.6597. Bibcode: 2001Icar..151...69K.

[JPL-SSD-sat_phys-5] 5.0 ^5.1 "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 24 October 2008. http://ssd.jpl.nasa.gov/?sat_phys_par.

[Williams_2007_nssdc-6] 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.

[Karkoschka,_Hubble_2001-8] 7.0 ^7.1 ^7.2 ^7.3 Karkoschka, Erich (2001). "Comprehensive Photometry of the Rings and 16 Satellites of Uranus with the Hubble Space Telescope". Icarus 151 (1): 51–68. doi:10.1006/icar.2001.6596. Bibcode: 2001Icar..151...51K.

[IAUC_4164-9] Smith, B. A. (1986-01-16). "Satellites of Uranus". IAU Circular 4164. http://www.cbat.eps.harvard.edu/iauc/04100/04164.html#Item1. Retrieved 2011-11-01.

[Gazetteer-10] "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. http://planetarynames.wr.usgs.gov/Page/Planets.

[Murray_Thompson_1990-11] 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. doi:10.1038/348499a0. ISSN 0028-0836. Bibcode: 1990Natur.348..499M.

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v t e Moons of Uranus
Generally listed in increasing distance from Uranus
Inner	Rings of Uranus Cordelia Ophelia Bianca Cressida Desdemona Juliet Portia Rosalind Cupid Belinda Perdita Puck Mab
Major (spheroid)	Miranda Ariel Umbriel Titania Oberon
Outer (irregular)	Francisco Caliban Stephano Trinculo Sycorax Margaret Prospero Setebos Ferdinand
Geological features	Arielian Kachina Chasmata Yangoor Mirandian Verona Rupes Oberonian Hamlet Mommur Chasma Puckian Titanian Gertrude Messina Chasmata Ursula Rousillon Rupes Umbrielian Wunda Vuver Skynd

v t e Natural satellites of the Solar System
Planetary satellites	Terrestrial Martian Jovian Saturnian Uranian Neptunian
Dwarf-planet satellites	Plutonian Haumean Makemakean Eridian OR₁₀ Quaoaran Orcean
Minor-planet moons	Main belt binaries: Antiope Frostia Berna Tokai Ostro Balam Doppler Pauling Iwamoto Wolff Bettig Christophedumas Trojans: Patroclus–Menoetius Hektor–Skamandrios Iphthime Eurydamas TNOs: Huya Typhon–Echidna Lempo–Paha–Hiisi 2002 UX₂₅ Logos–Zoe Ceto–Phorcys Borasisi–Pabu Sila–Nunam Teharonhiawako–Sawiskera Salacia–Actaea 2002 WC₁₉ Altjira Varda–Ilmarë 2003 AZ₈₄ Gǃkúnǁʼhòmdímà–Gǃòʼé ǃHú Mors–Somnus Manwë–Thorondor ǂKá̦gára–ǃHãunu 2013 FY27
Ranked by size	Planetary-mass moon Ganymede largest: 5268 km / 0.413 Earths Titan Callisto Io Moon Europa Triton Titania Rhea Oberon Iapetus Charon Umbriel Ariel Dione Tethys Dysnomia Enceladus Miranda Vanth Proteus Mimas Ilmarë Nereid Hiʻiaka Actaea Hyperion ...
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Rosalind (moon)

Topic: Astronomy

See also

References

External links

Discovery
The Hubble Space Telescope captured tiny Rosalind orbiting Uranus in 1997
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]}