Jump to content

Eukelade: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
PipepBot (talk | contribs)
m robot Adding: fi:Eukelade
No edit summary
Line 29: Line 29:
[[nds:Eukelade (Maand)]]
[[nds:Eukelade (Maand)]]
[[pl:Eukelade (księżyc)]]
[[pl:Eukelade (księżyc)]]
[[ru:Эвкеладе (спутник)]]
[[simple:Eukelade (moon)]]
[[simple:Eukelade (moon)]]
[[sk:Eukelade (mesiac)]]
[[sk:Eukelade (mesiac)]]

Revision as of 17:59, 11 April 2008

Eukelade (ew-kel'-ə-dee, /jʊˈkɛlədi/; Greek Ευκελαδη), or Jupiter XLVII, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2003, and received the temporary designation S/2003 J 1.[1][2][3]

Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484 Mm in 735.200 days, at an inclination of 164° to the ecliptic (165° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.2829.

It was named in March 2005 after Eukelade, described by some Greek writers as one of the Muses, and thus a daughter of Zeus (Jupiter).[4][5]

Eukelade belongs to the Carme group, made up of irregular retrograde moons orbiting Jupiter at a distance ranging between 23 and 24 Gm and at an inclination of about 165°.

References