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Eukelade (moon)

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Eukelade (ew-kel'-ə-dee, IPA: /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


als:Eukelade (Mond)

br:Eukelade (loarenn) bg:Евкелада (спътник) da:Eukelade (måne) de:Eukelade (Mond) fr:Eukéladé (lune) hr:Eukelada (mjesec) it:Eucelade (astronomia) lt:Eukeladė (palydovas) nl:Eukelade (maan) ja:エウケラデ (衛星) nds:Eukelade (Maand) pl:Eukelade (księżyc) simple:Eukelade (moon) sk:Eukelade (mesiac) sl:Evkelada (luna) fi:Eukelade sv:Eukelade

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