Ophelia

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(ō-fēl') pronunciation
n.
The satellite of Uranus that is second in distance from the planet.

[After Ophelia, daughter of Polonius in Hamlet by William Shakespeare.]



The second closest moon of Uranus, also known as Uranus VII; it was discovered in 1986 by Voyager 2. Ophelia has a diameter of 32 km and moves in a nearly circular orbit 53,760 km from (the center of) the planet. It appears to be the outer shepherd moon of Uranus's Epsilon ring.
Ophelia, in astronomy, one of the natural satellites, or moons, of Uranus.


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There is also an asteroid called 171 Ophelia.
Ophelia
Ophelia
Discovery image of Ophelia (top of image, outside of rings)
Discovery
Discovered by Richard J. Terrile / Voyager 2
Discovery date January 20, 1986
Mean orbit radius 53,763.390 ± 0.847 km[1]
Eccentricity 0.00992 ± 0.000107[1]
Orbital period 0.37640039 ± 0.00000357 d[1]
Inclination 0.10362 ± 0.055° (to Uranus' equator)[1]
Satellite of Uranus
Physical characteristics
Dimensions 54 × 38 × 38 km[2]
Mean radius 21.4 ± 4 km[2][3][4]
Surface area ~6600 km²[a]
Volume ~41,000 km³[a]
Mass ~5.3×1016 kg[a]
Mean density ~1.3 g/cm³ (assumed)[3]
Equatorial surface gravity ~0.0070 m/s²[a]
Escape velocity ~0.018 km/s[a]
Rotation period synchronous[2]
Axial tilt zero[2]
Albedo
Temperature ~64 K[a]

Ophelia (play /ɵˈfliə/ o-FEE-lee-ə) is a moon of Uranus. It was discovered from the images taken by Voyager 2 on January 20, 1986, and was given the temporary designation S/1986 U 8.[6] It was not seen until the Hubble Space Telescope recovered it in 2003.[5][7] Ophelia was named after the daughter of Polonius, Ophelia, in William Shakespeare's play Hamlet. It is also designated Uranus VII.[8]

Other than its orbit,[1] radius of 21 km[2] and geometric albedo of 0.08[5] virtually nothing is known about it. At the Voyager 2 images Ophelia appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of the Ophelia's prolate spheroid is 0.7 ± 0.3.[2]

Ophelia acts as the outer shepherd satellite for Uranus' Epsilon ring.[9] The orbit of Ophelia is within the synchronous orbit radius of Uranus, and therefore the moon is slowly decaying due to tidal forces.[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 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. ^ Showalter, M. R.; Lissauer, J. J. (2003-09-03). "Satellites of Uranus". IAU Circular 8194. http://www.cbat.eps.harvard.edu/iauc/08100/08194.html. Retrieved 2011-10-31. 
  8. ^ "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. http://planetarynames.wr.usgs.gov/append7.html. Retrieved 6 August 2006. 
  9. ^ Esposito, L. W. (2002). "Planetary rings". Reports On Progress In Physics 65 (12): 1741–1783. Bibcode 2002RPPh...65.1741E. doi:10.1088/0034-4885/65/12/201.  edit

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