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Hegemone (hə-jem'-ə-nee, IPA: /hɨˈdʒɛməni/; Greek Ἡγεμόνη), or Jupiter XXXIX, 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 2003, and given the temporary designation S/2003 J 8.[1][2]
Hegemone is about 3 kilometres in diameter, and orbits Jupiter at an average distance of 23,703 Mm in 745.500 days, at an inclination of 153° to the ecliptic (151° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.4077.
It was named in March 2005 after Hegemone, one of the Graces, and a daughter of Zeus (Jupiter).[3]
Hegemone 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
als:Hegemone (Mond)
br:Hegemone (loarenn) bg:Хегемона (спътник) da:Hegemone (måne) de:Hegemone (Mond) fr:Hégémone (lune) hr:Hegemona (mjesec) it:Egemone (astronomia) lt:Hegemonė (palydovas) nl:Hegemone (maan) ja:ヘゲモネ (衛星) nds:Hegemone (Maand) pl:Hegemone (księżyc) simple:Hegemone (moon) sk:Hegemone (mesiac) sl:Hegemona (luna) fi:Hegemone sv:Hegemone
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