Eukelade
Discovery | |
---|---|
Discovered by | Scott S. Sheppard |
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 |
−746.4 days | |
98.4° | |
Inclination | 165.5° |
206.3° | |
325.6° | |
Satellite of | Jupiter |
Group | Carme group |
Physical characteristics | |
4 km | |
22.6 | |
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.[2][3][4]
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
- ^ S.S. Sheppard (2019), Moons of Jupiter, Carnegie Science, on line
- ^ IAUC 8087: Satellites of Jupiter 2003 March 4 (discovery)
- ^ 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)
- ^ 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)
- ^ IAUC 8502: Satellites of Jupiter 2005 March 30 (naming the moon)
- ^ Scholies d’Hésiode Archived 2006-12-06 at the Wayback Machine (in Greek and French, translation by Michel Tichit), EducNet MusAgora: Les Muses dans la littérature grecque ancienne Archived 2007-08-27 at the Wayback Machine