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Setebos (moon)

From Wikipedia, the free encyclopedia
Moon of Uranus
Setebos
Discovery image of Setebos (encircled)
Discovery
Discovered by
Discovery dateJuly 18, 1999
Designations
Designation
Uranus XIX
Pronunciation/ˈsɛtɛbʌs/,[1]/-bɒs/[2]
AdjectivesSetebosian/ˌsɛtɛˈbsiən/[3]
Orbital characteristics
Mean orbitradius
17,418,000 km[4][5]
Eccentricity0.5914[5]
2225.21 d
Inclination158° (to theecliptic)[4]
Satellite ofUranus
Physical characteristics
24 km (estimate)[6]
<50 km[7]
~7200 km2 (estimate)
Volume~58,000 km3 (estimate)
Mass~7.5×1016kg (estimate)
~1.3 g/cm3 (assumed)
~0.0063m/s2 (estimate)
~0.0204 km/s (estimate)
4.255 ± 0.017 h[7]
?
Albedo0.04 (assumed)[6]
Temperature~65K (estimate)

Setebos/ˈsɛtɛbʌs/ is one of the outermostretrogradeirregular satellites ofUranus. It was discovered on 18 July 1999 byJohn J. Kavelaarset al. and provisionally designatedS/1999 U 1.[8]

Animation of discovery images taken in July 1999

Confirmed asUranus XIX, it is named after the godSetebos worshipped byCaliban andSycorax inWilliam Shakespeare's playThe Tempest.

The orbital parameters suggest that it may belong to the same dynamic cluster asSycorax andProspero, suggesting common origin.[9] However, this suggestion does not appear to be supported by the observed colours. The satellite appears neutral (grey) invisible light (colour indicesB−V = 0.77 ,R−V = 0.35 ),[10] similar to Prospero but different from Sycorax (which is light red).

A crater onUmbriel is also named after Setebos, but with the spellingSetibos.

See also

[edit]

References

[edit]
  1. ^Shakespeare Recording Society (1995)The Tempest (audio CD)
  2. ^Benjamin Smith (1903)The Century Dictionary and Cyclopedia
  3. ^Campbell, Pyre, Weaver (1932)Poetry and criticism of the romantic movement
  4. ^abSheppard, Jewitt & Kleyna 2005, p. 523, Table 3.
  5. ^abYeomans, Donald K. (2007-06-28)."Planetary Satellite Mean Orbital Parameters". JPL/NASA. Retrieved2008-01-19.
  6. ^abSheppard, Jewitt & Kleyna 2005, p. 523, Table 3 ... ri (km) ... 24 ...i Radius of satellite assuming a geometric albedo of 0.04.
  7. ^abFarkas-Takács, A.; Kiss, Cs.; Pál, A.; Molnár, L.; Szabó, Gy. M.; Hanyecz, O.; et al. (September 2017)."Properties of the Irregular Satellite System around Uranus Inferred from K2, Herschel, and Spitzer Observations".The Astronomical Journal.154 (3): 13.arXiv:1706.06837.Bibcode:2017AJ....154..119F.doi:10.3847/1538-3881/aa8365.S2CID 118869078. 119.
  8. ^Gladman, B. J.;Kavelaars, J. J.;Holman, M. J.,Petit, J.-M.;Scholl, H.;Nicholson, P. D.; and Burns, J. A.;The Discovery of Uranus XIX, XX, and XXI, Icarus,147 (2000), pages 320–324
  9. ^Grav, Tommy; Holman, Matthew J.; Gladman, Brett J.; andAksnes, Kaare;Photometric survey of the irregular satellites, Icarus,166, (2003), pages 33–45.arXiv:astro-ph/0301016
  10. ^Grav, Holman & Fraser 2004.

External links

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  • Listed in approximately increasing distance fromUranus
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