Desdemona (moon)
Desdemona 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 6.[10] Desdemona is named after the wife of Othello in William Shakespeare's play Othello. It is also designated Uranus X.[11]
- There is also a minor planet called 666 Desdemona.
Discovery image of Desdemona | |
Discovery | |
---|---|
Discovered by | Stephen P. Synnott / Voyager 2 |
Discovery date | January 13, 1986 |
Designations | |
Designation | Uranus X |
Pronunciation | /dɛzdɛˈmoʊnə/[1] |
Adjectives | Desdemonan,[2] Desdemonian,[3] Desdemonean[4] /dɛzdɛˈmoʊn(i)ən/ |
Orbital characteristics | |
Mean orbit radius | 62,658.364 ± 0.047 km[5] |
Eccentricity | 0.00013 ± 0.000070[5] |
0.473649597 ± 0.000000014 d[5] | |
Inclination | 0.11252 ± 0.037° (to Uranus' equator)[5] |
Satellite of | Uranus |
Physical characteristics | |
Dimensions | 90 × 54 × 54 km[6] |
Mean radius | 32.0 ± 4 km[6][7][8] |
~14,500 km²[lower-alpha 1] | |
Volume | ~164,000 km³[lower-alpha 1] |
Mass | ~1.8×1017 kg[lower-alpha 1] |
Mean density | ~1.3 g/cm³ (assumed)[7] |
~0.011 m/s2[lower-alpha 1] | |
~0.027 km/s[lower-alpha 1] | |
synchronous[6] | |
zero[6] | |
Albedo | |
Temperature | ~64 K[lower-alpha 1] |
Desdemona belongs to Portia Group of satellites, which also includes Bianca, Cressida, Juliet, Portia, Rosalind, Cupid, Belinda and Perdita.[9] These satellites have similar orbits and photometric properties.[9] Other than its orbit,[5] radius of 32 km[6] and geometric albedo of 0.08[9] virtually nothing is known about Desdemona.
At the Voyager 2 images Desdemona appears as an elongated object, the major axis pointing towards Uranus. The ratio of axes of Desdemona's prolate spheroid is 0.6 ± 0.3.[6] Its surface is grey in color.[6]
Desdemona may collide with one of its neighboring moons Cressida or Juliet within the next 100 million years.[12]
See also
References
Explanatory notes
- Calculated on the basis of other parameters.
Citations
- Benjamin Smith (1903) The Century Dictionary and Cyclopedia
- Harris & Lazzari (1997) Shakespearean criticism
- Daileader (2005) Racism, misogyny, and the Othello myth
- Genova (1997) Power, gender, values
- 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.
- 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.
- "Planetary Satellite Physical Parameters". JPL (Solar System Dynamics). 24 October 2008. 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.
- 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.
- Smith, B. A. (January 16, 1986). "Satellites of Uranus". IAU Circular. 4164. Archived from the original on 5 November 2011. Retrieved 29 October 2011.
- "Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. USGS Astrogeology. July 21, 2006. Retrieved 6 August 2006.
- Duncan, Martin J.; Lissauer, Jack J. (1997). "Orbital Stability of the Uranian Satellite System". Icarus. 125 (1): 1–12. Bibcode:1997Icar..125....1D. doi:10.1006/icar.1996.5568.