Thelxinoe (moon)
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Thelxinoe (thel-zin'-oe-ee, Template:IPA2; Greek Θελξινόη), or Jupiter XLII, 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 2004 from pictures taken in 2003, and originally received the temporary designation S/2003 J 22. The announcement is contained in the International Astronomical Union Circular (IAUC) 8276. [1] Thelxinoe is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 20,454 Mm in 597.607 days, at an inclination of 151° to the ecliptic (103° to Jupiter's equator), in a retrograde direction and with an eccentricity of 0.2685.
It is named after Thelxinoe, one of the four original Muses according to some Greek writers, and a daughter of Zeus (Jupiter) by Mnemosyne.
Thelxinoe belongs to the Ananke group, retrograde irregular moons which orbit Jupiter between 19.3 and 22.7 Gm, at inclinations of roughly 150°.
| edit Jupiter (satellites) |
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| Inner satellites | Galilean moons | Themisto | Himalia group | Carpo |
| S/2003 J 12 | Ananke group | Carme group | Pasiphaë group | S/2003 J 2 |
| See also: Pronunciation key | Rings of Jupiter |
bg:Телксиноя (спътник) da:Thelxinoe (måne) de:Thelxinoe (Mond) fr:Thelxinoé (lune) hr:Thelxinoe (mjesec) pt:Telxinoi (satélite) sk:Thelxinoe (mesiac) sv:Thelxinoe zh:木卫四十二