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Cyllene (sə-lee'-nee, IPA: /sɨˈliːni/; Greek Κυλλήνη), or Jupiter XLVIII, 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, receiving the temporary designation S/2003 J 13.[1][2]
Cyllene is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 23,396 Mm in 731.099 days, at an inclination of 140° to the ecliptic (140° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.4116.
It was named in March 2005 after Cyllene, a naiad (stream nymph) or oread (mountain nymph) associated with Mount Kyllini, Greece.[3] She was a daughter of Zeus (Jupiter).
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
als:Cyllene (Mond)
br:Cyllene (loarenn) bg:Силена (спътник) cs:Cyllene (měsíc) da:Cyllene (måne) de:Cyllene (Mond) fr:Cyllèné (lune) hr:Kilena (mjesec) it:Cillene (astronomia) lt:Kilenė (palydovas) nl:Cyllene (maan) ja:キュレーネ (衛星) nds:Cyllene (Maand) pl:Cyllene (księżyc) simple:Cyllene (moon) sk:Cyllene (mesiac) sl:Kilena (luna) fi:Cyllene sv:Cyllene
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