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'''Eukelade''' ''(ew-kel'-ə-dee,'' {{IPA2|jʊˈkɛlədi}}; Greek ''Ευκελαδη),'' or '''Jupiter XLVII''', is a [[retrograde motion|retrograde]] [[irregular satellite]] of [[Jupiter (planet)|Jupiter]].
'''Eukelade''' ''(ew-kel'-ə-dee,'' {{IPA2|jʊˈkɛlədi}}; Greek ''Ευκελαδη),'' or '''{{nowrap|Jupiter XLVII}}''', is a [[retrograde motion|retrograde]] [[irregular satellite]] of [[Jupiter (planet)|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 '''{{nowrap|S/2003 J 1}}'''.<ref>[http://cfa-www.harvard.edu/iauc/08000/08087.html IAUC 8087: ''Satellites of Jupiter''] [[2003]] [[March 4]] (discovery)</ref><ref>[http://cfa-www.harvard.edu/iau/mpec/K03/K03E11.html MPEC 2003-E11: ''S/2003 J 1, 2003 J 2, 2003 J 3, 2003 J 4, 2003 J 5, 2003 J 6, 2003 J 7''] [[2003]] [[March 4]] (discovery and ephemeris)</ref><ref>[http://cfa-www.harvard.edu/mpec/K03/K03E29.html MPEC 2003-E29: ''S/2003 J 9, 2003 J 10, 2003 J 11, 2003 J 12; S/2003 J 1, 2003 J 6''] [[2003]] [[April 3]] (revised ephemeris)</ref>
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&nbsp;J&nbsp;1'''.


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 motion|retrograde]] direction and with an [[eccentricity (orbit)|eccentricity]] of 0.2829.
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 motion|retrograde]] direction and with an [[eccentricity (orbit)|eccentricity]] of 0.2829.


It was named in March 2005 after [[Eukelade]], described by some Greek writers as one of the [[Muse]]s, and thus a daughter of [[Zeus]] (Jupiter). [http://www.educnet.education.fr/musagora/muses/musesfr/scholies.pdf]
It was named in March 2005 after [[Eukelade]], described by some Greek writers as one of the [[Muse]]s, and thus a daughter of [[Zeus]] (Jupiter).<ref>[http://cfa-www.harvard.edu/iauc/08500/08502.html IAUC 8502: ''Satellites of Jupiter''] [[2005]] [[March 30]] (naming the moon)</ref><ref>[http://www.educnet.education.fr/musagora/muses/musesfr/scholies.pdf ''Scholies d’Hésiode''] (in Greek and French, translation by Michel Tichit), EducNet MusAgora: [http://www.educnet.education.fr/musagora/muses/musesfr/textes.htm ''Les Muses dans la littérature grecque ancienne'']</ref>


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°.
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==
==References==
<references/>
* [http://cfa-www.harvard.edu/iauc/08000/08087.html IAUC 8087: ''Satellites of Jupiter''] [[2003]] [[March 4]] (discovery)
* [http://cfa-www.harvard.edu/iau/mpec/K03/K03E11.html MPEC 2003-E11: ''S/2003 J 1, 2003 J 2, 2003 J 3, 2003 J 4, 2003 J 5, 2003 J 6, 2003 J 7''] [[2003]] [[March 4]] (discovery and ephemeris)
* [http://cfa-www.harvard.edu/mpec/K03/K03E29.html MPEC 2003-E29: ''S/2003 J 9, 2003 J 10, 2003 J 11, 2003 J 12; S/2003 J 1, 2003 J 6''] [[2003]] [[April 3]] (revised ephemeris)
* [http://cfa-www.harvard.edu/iauc/08500/08502.html IAUC 8502: ''Satellites of Jupiter''] [[2005]] [[March 30]] (naming the moon)


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Revision as of 17:41, 27 April 2007

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


... | Cyllene | Eukelade | S/2003 J 4 | ...