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F r o m W i k i p e d i a , t h e f r e e e n c y c l o p e d i a
Setebos is one of the outermost retrograde irregular satellites of Uranus . It was discovered on 18 July 1999 by John J. Kavelaars et al. and provisionally designated S/1999 U 1 .[8]
Animation of discovery images taken in July 1999
Confirmed as Uranus XIX , it is named after the god worshipped by Caliban and Sycorax in William Shakespeare 's play The Tempest .
The orbital parameters suggest that it may belong to the same dynamic cluster as Sycorax and Prospero , suggesting common origin.[9] However, this suggestion does not appear to be supported by the observed colours. The satellite appears neutral (grey) in visible light (colour indices B−V = 0.77 , R−V = 0.35 ), similar to Prospero but different from Sycorax (which is light red).
A crater on Umbriel is also named after Setebos, but with the spelling Setibos .
See also [ edit ]
References [ edit ]
^ Shakespeare Recording Society (1995) The Tempest (audio CD)
^ Benjamin Smith (1903) The Century Dictionary and Cyclopedia
^ Campbell, Pyre, Weaver (1932) Poetry and criticism of the romantic movement
^ a b
Yeomans, Donald K. (2007-06-28). "Planetary Satellite Mean Orbital Parameters" . JPL/NASA. Retrieved 2008-01-19 .
^ a b
Sheppard, Jewitt & Kleyna 2005 , p. 523, Table 3 ... ri (km ) ... 24 ... i Radius of satellite assuming a geometric albedo of 0.04.
^ a b Farkas-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.
^
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), pp. 320–324
^
Grav, Tommy ; Holman, Matthew J.; Gladman, Brett J.; and Aksnes, Kaare ; Photometric survey of the irregular satellites , Icarus, 166 , (2003), pp. 33–45. arXiv :astro-ph/0301016
Sheppard, S.S.; Jewitt, D.; Kleyna, J. (2005). "An ultradeep survey for irregular satellites of Uranus: Limits to completeness". The Astronomical Journal . 129 (1 ): 518–525. arXiv :astro-ph/0410059 . Bibcode :2005AJ....129..518S . doi :10.1086/426329 . S2CID 18688556 .
External links [ edit ]
t
e
Listed in approximately increasing distance from Uranus
Inner
Major (spheroid)
Outer (irregular)
Geological features
R e t r i e v e d f r o m " https://en.wikipedia.org/w/index.php?title=Setebos_(moon)&oldid=1211553563 "
C a t e g o r i e s :
● M o o n s o f U r a n u s
● I r r e g u l a r s a t e l l i t e s
● D i s c o v e r i e s b y M a t t h e w J . H o l m a n
● D i s c o v e r i e s b y B r e t t J . G l a d m a n
● A s t r o n o m i c a l o b j e c t s d i s c o v e r e d i n 1 9 9 9
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H i d d e n c a t e g o r i e s :
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● S h o r t d e s c r i p t i o n m a t c h e s W i k i d a t a
● T h i s p a g e w a s l a s t e d i t e d o n 3 M a r c h 2 0 2 4 , a t 0 4 : 2 3 ( U T C ) .
● T e x t i s a v a i l a b l e u n d e r t h e C r e a t i v e C o m m o n s A t t r i b u t i o n - S h a r e A l i k e L i c e n s e 4 . 0 ;
a d d i t i o n a l t e r m s m a y a p p l y . B y u s i n g t h i s s i t e , y o u a g r e e t o t h e T e r m s o f U s e a n d P r i v a c y P o l i c y . W i k i p e d i a ® i s a r e g i s t e r e d t r a d e m a r k o f t h e W i k i m e d i a F o u n d a t i o n , I n c . , a n o n - p r o f i t o r g a n i z a t i o n .
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