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Bianca (moon)

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There is also an asteroid called 218 Bianca.
Bianca
Discovery
Discovered byBradford A. Smith / Voyager 2
Discovery dateJanuary 23, 1986
Designations
Designation
Uranus VIII
Pronunciation/biˈæŋkə/[1]
AdjectivesBiancan[2]
Orbital characteristics[3]
Epoch 2004 August 25 12:00 ET
(JED 2453243.0)
59165.5621±0.0057 km
Eccentricity0.000274±0.000172
0.43457902±0.00000006 d
9.90 km/s
828.387887±0.000121 °/d
Inclination0.1811°±0.0182° (to Uranus's equator)
Satellite ofUranus
Physical characteristics
Dimensions64 × 46 × 46 km[a]
25.4±2.2 km[b]
Volume70900 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 (assumed)
zero (assumed)
Albedo0.065 ± 0.010 (geometric)[7]
0.026 ± 0.005 (Bond)[8]
22.42–22.61 (± 0.24)
(at opposition)[9]
9.71–9.90 (± 0.24)[9]

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.[12] These satellites have similar orbits and photometric properties.[12] Other than its orbit,[3] size of 64 km × 46 km (40 mi × 29 mi),[4] and geometric albedo of 0.065,[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.[13]

See also

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Notes

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  1. ↑ The satellite's shape was modelled as a prolate spheroid (a × b × b); thus, only constraints for two axes were determined (a × b = 32 × 23 km).[4]
  2. ↑ This is the geometric mean of the three axes (), calculated from = 27±2 km and = 0.7±0.2.[4] However, various sources use 27±2 km or 32 × 23 km as the radius value or cross section size instead.

References

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  1. ↑ Benjamin Smith (1903). The Century Dictionary and Cyclopedia.
  2. ↑ Ruud (2008). Critical companion to Dante: a literary reference to his life and work.
  3. 1 2 Showalter & Lissauer 2006, Supporting Online Material, Table S3.
  4. 1 2 3 4 Karkoschka, Voyager 2001, Table V.
  5. 1 2 3 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. Bibcode:2024Icar..41115957F. doi:10.1016/j.icarus.2024.115957. ISSN 0019-1035.
  6. ↑ 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.
  7. 1 2 Showalter & Lissauer 2006, Supporting Online Material, Table S2.
  8. ↑ Karkoschka, Hubble 2001, Table VII.
  9. 1 2 Karkoschka, Hubble 2001, Table IV.
  10. ↑ Smith, B. A. (1986-01-27). "Satellites and Rings of Uranus". IAU Circular (4168). Retrieved 2011-10-31.
  11. ↑ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 6 August 2006.
  12. 1 2 Karkoschka, Hubble 2001.
  13. ↑ Karkoschka, Voyager 2001.

Bibliography

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