Bianca (moon)
- There is also an asteroid called 218 Bianca.
| Discovery | |
|---|---|
| Discovered by | Bradford A. Smith / Voyager 2 |
| Discovery date | January 23, 1986 |
| Designations | |
Designation | Uranus VIII |
| Pronunciation | /biˈæŋkə/[1] |
| Adjectives | Biancan[2] |
| Orbital characteristics[3] | |
| 59165.550±0.045 km | |
| Eccentricity | 0.00092 ± 0.000118 |
| 0.434578986 ± 0.000000022 d | |
| Inclination | 0.19308 ± 0.054° (to Uranus's equator) |
| Satellite of | Uranus |
| Physical characteristics | |
| Dimensions | 64 × 46 × 46 km[4][note 1] |
| ~8400 km2[a] | |
| Volume | 70900 km3 ± 29.9%[5] |
| Mass | (6.38±1.91)×1016 kg[5] |
Mean density | 0.5–1.2 g/cm3[6] 0.9 g/cm3 (assumed)[5] |
| synchronous[4] | |
| zero[4] | |
| Albedo | 0.08 ± 0.01[7] 0.07[8][9] |
| 22.52 (at opposition) | |
| |
Bianca is an inner satellite of Uranus. It was discovered from the images taken by Voyager 2 on January 23, 1986, and was given the temporary designation S/1986 U 9.[10] It was named after the sister of Katherina in Shakespeare's play The Taming of the Shrew. It is also designated Uranus VIII.[11]
Bianca belongs to the Portia group of satellites, which also includes Cressida, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda, and Perdita.[7] These satellites have similar orbits and photometric properties.[7] Other than its orbit,[3] size of 64 km × 46 km (40 mi × 29 mi),[4] and geometric albedo of 0.08,[7] little is known about it.
In Voyager 2 images Bianca appears as an elongated object, with its major axis pointing towards Uranus. The ratio of axes of Bianca's prolate spheroid is 0.7±0.2.[4] Its surface is grey in color.[4]
See also
Notes
- ^ Calculated on the basis of other parameters.
References
- ^ Benjamin Smith (1903). The Century Dictionary and Cyclopedia.
- ^ Ruud (2008). Critical companion to Dante: a literary reference to his life and work.
- ^ 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. Bibcode:1998AJ....115.1195J. doi:10.1086/300263. S2CID 118616209.
- ^ a b c d e f 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.
- ^ a b c French, Richard G.; Hedman, Matthew M.; Nicholson, Philip D.; Longaretti, Pierre-Yves; McGhee-French, Colleen A. (2024-03-15). "The Uranus system from occultation observations (1977–2006): Rings, pole direction, gravity field, and masses of Cressida, Cordelia, and Ophelia". Icarus. 411 115957. arXiv:2401.04634. doi:10.1016/j.icarus.2024.115957. ISSN 0019-1035.
- ^ French, Robert S.; Showalter, Mark R. (August 2012). "Cupid is Doomed: An Analysis of the Stability of the Inner Uranian Satellites". Icarus. 220 (2): 911–921. arXiv:1408.2543. Bibcode:2012Icar..220..911F. doi:10.1016/j.icarus.2012.06.031.
- ^ a b c d 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.
- ^ "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 24 October 2008. Archived from the original on 17 January 2009. Retrieved 12 December 2008.
- ^ Williams, Dr. David R. (23 November 2007). "Uranian Satellite Fact Sheet". NASA (National Space Science Data Center). Retrieved 12 December 2008.
- ^ Smith, B. A. (1986-01-27). "Satellites and Rings of Uranus". IAU Circular. 4168. Retrieved 2011-10-31.
- ^ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 6 August 2006.