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From Wikipedia, the free encyclopedia
Eukelade /juːˈkɛlədiː/, 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.[4][5][6]
Discovery | |
---|---|
Discovered by | Scott S. Sheppard et al. |
Discovery date | 2003 |
Designations | |
Designation | Jupiter XLVII |
Pronunciation | /juːˈkɛlədiː/ |
Named after | Ευκελάδη Eykeladē |
S/2003 J 1 | |
Adjectives | Eukeladean /ˌjuːkɪləˈdiːən/ |
Orbital characteristics [1] | |
23661000 km | |
Eccentricity | 0.272 |
−693.02 days[2] | |
98.4° | |
Inclination | 165.5° |
206.3° | |
325.6° | |
Satellite of | Jupiter |
Group | Carme group |
Physical characteristics | |
4 km | |
Spectral type | B–V = 0.79 ± 0.07, V–R = 0.50 ± 0.07[3] |
22.6 | |
15.9[2] | |
Eukelade is about 4 kilometres in diameter, and orbits Jupiter at an average distance of 23,484,000 km in 693.02 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 - according to John Tzetzes, listed by some (unnamed) Greek writers as one of the Muses.[7]
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°.
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