(byäng'kä, bē-äng') pronunciation
n.
The satellite of Uranus that is third in distance from the planet.

[After Bianca, sister of Katherine in The Taming of the Shrew by William Shakespeare.]


Bianca

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The third moon of Uranus, also known as Uranus VIII; it was discovered in 1986 on images sent back by Voyager 2. Bianca has a diameter of 44 km and moves in a nearly circular orbit 59,170 km from (the center of) the planet.
Bianca, in astronomy, one of the natural satellites, or moons, of Uranus.


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There is also an asteroid called 218 Bianca.
Bianca
Bianca
Discovery
Discovered by Bradford A. Smith / Voyager 2
Discovery date January 23, 1986
Mean orbit radius 59,165.550 ± 0.045 km[1]
Eccentricity 0.00092 ± 0.000118[1]
Orbital period 0.434578986 ± 0.000000022 d[1]
Inclination 0.19308 ± 0.054° (to Uranus' equator)[1]
Satellite of Uranus
Physical characteristics
Dimensions 64 × 46 × 46 km[2]
Mean radius 25.7 ± 2 km[2][3][4]
Surface area ~8300 km²[a]
Volume ~71,000 km³[a]
Mass ~9.2×1016 kg[a]
Mean density ~1.3 g/cm³ (assumed)[3]
Equatorial surface gravity ~0.0086 m/s²[a]
Escape velocity ~0.022 km/s[a]
Rotation period synchronous[2]
Axial tilt zero[2]
Albedo
Temperature ~64 K[a]

Bianca (play /biˈɑːŋkə/ bee-AHNG-kə) 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.[6] It was named after the sister of Katherine in Shakespeare's play The Taming of the Shrew. Originally, it was to be called Peaseblossom after a fairy in Shakespeare's A Midsummer Night's Dream, but due to a nomenclature conflict between the USA and the USSR the name Bianca was quietly chosen by the IAU a few years after the moon's discovery. It is also designated Uranus VIII.[7]

Bianca belongs to Portia Group of satellites, which also includes Cressida, Desdemona, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita.[5] These satellites have similar orbits and photometric properties.[5] Other than its orbit,[1] radius of 27 km,[2] and geometric albedo of 0.08[5] virtually nothing is known about it.

At the Voyager 2 images Bianca appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of the Bianca's prolate spheroid is 0.7 ± 0.2.[2] Its surface is grey in color.[2]

See also

References

Explanatory notes

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

Citations

  1. ^ a b c d e 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.  edit
  2. ^ a b c d e f g 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.  edit
  3. ^ a b c "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 24 October 2008. http://ssd.jpl.nasa.gov/?sat_phys_par. Retrieved 12 December 2008. 
  4. ^ a b 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. Retrieved 12 December 2008. 
  5. ^ 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.  edit
  6. ^ Smith, B. A. (1986-01-27). "Satellites and Rings of Uranus". IAU Circular 4168. http://www.cbat.eps.harvard.edu/iauc/04100/04168.html#Item1. Retrieved 2011-10-31. 
  7. ^ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. http://planetarynames.wr.usgs.gov/Page/Planets. Retrieved 6 August 2006. 

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