Eukelade

Eukelade /jˈkɛləd/, also known as 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.[2][3][4]

Eukelade
Discovery
Discovered byScott S. Sheppard
Discovery date2003
Designations
Designation
Jupiter XLVII
Pronunciation/jˈkɛləd/
Named after
Ευκελάδη Eykeladē
S/2003 J 1
AdjectivesEukeladean /ˌjuːkɪləˈdən/
Orbital characteristics[1]
23661000 km
Eccentricity0.272
−746.4 days
98.4°
Inclination165.5°
206.3°
325.6°
Satellite ofJupiter
GroupCarme group
Physical characteristics
Mean diameter
4 km
22.6

    Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484,000 km 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 Eucelade, described by some Greek writers as one of the Muses, and thus a daughter of Zeus (Jupiter).[5][6]

    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

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