- Megaclite (moon)
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Megaclite ( /ˌmɛɡəˈklaɪtiː/ meg-ə-kly-tee; Latin: Megaclītē; Greek: Μεγακλειτη), also known as Jupiter XIX, is a natural satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2000, and given the temporary designation S/2000 J 8.[1][2][3]
Megaclite is about 5.4 kilometres in diameter, and orbits Jupiter at an average distance of 24.687 million kilometers in 792.437 days, at an inclination of 150° to the ecliptic (148° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.308.
It was named in October 2002 after Megaclite, mother by Zeus (Jupiter) of Thebe and Locrus (although both of these are assigned a different mother by other authors).[4][5]
It belongs to the Pasiphaë group, irregular retrograde moons orbiting Jupiter at distances ranging between 22.8 and 24.1 Gm, and with inclinations ranging between 144.5° and 158.3°.
References
- ^ IAUC 7555: Satellites of Jupiter 2001 January 5 (discovery)
- ^ MPEC 2001-A29: S/2000 J 7, S/2000 J 8, S/2000 J 9, S/2000 J 10, S/2000 J 11 2001 January 15 (discovery and ephemeris)
- ^ MPEC 2001-T59: S/2000 J 8, S/2000 J 9, S/2000 J 10 2001 October 15 (revised ephemeris)
- ^ IAUC 7998: Satellites of Jupiter 2002 October 22 (naming the moon "Magaclite")
- ^ IAUC 8023: Satellites of Jupiter 2002 November 29 (correcting the name)
Moons of Jupiter Listed in increasing distance from Jupiter. Temporary names in italics. Inner moons Galilean moons Themisto group Himalia group Carpo group Ananke group coreperipheralCarme group Pasiphaë group - Eurydome
- S/2003 J 23
- Hegemone
- Pasiphaë
- Sponde
- Cyllene
- Megaclite
- S/2003 J 4
- Callirrhoe
- Sinope
- Autonoe
- Aoede
- Kore
- S/2010 J 1
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