Sinope (moon)
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Sinope (sə-noe'-pee, IPA: /sɨˈnoʊpi/; Greek Σινώπη) is a retrograde irregular satellite of Jupiter discovered by Seth Barnes Nicholson at Lick Observatory in 1914,[3] and is named after Sinope of Greek mythology. Sinope did not receive its present name until 1975[4][5]; before then, it was simply known as Jupiter IX. It was sometimes called "Hades"[6] between 1955 and 1975. Sinope was the outermost known moon of Jupiter until the discovery of Megaclite in 2000. The most distant moon of Jupiter now known is S/2003 J2.
OrbitImage:TheIrregulars JUPITER Pasiphae CORE.svg
Pasiphae group.
Sinope orbits Jupiter on a high eccentricity and high inclination retrograde orbit. The orbital elements are as of January 2000.[2] They are continuously changing due to Solar and planetary perturbations. It is often believed to belong to the Pasiphaë group.[7] However, given its mean inclination and different colour, Sinope could be also an independent object, captured independently, unrelated to the collision and break-up at the origin of the group.[8] The diagram illustrates Sinope's orbital elements in relation to other satellites of the group.
Physical characteristicsSinope has an estimated diameter of 38 km (assuming an albedo of 0.04)[7] The satellite is red (colour indices B-V=0.84, R-V=0.46).[8] unlike Pasiphae which is grey. Its infrared spectrum is similar to D-type asteroids also different from Pasiphae.[10] These dissimilarities of the physical parameters suggest a different origin from the core members of the group. See also
References
External links
bs:Sinopa (mjesec) br:Sinope (loarenn) bg:Синопа (спътник) co:Sinope da:Sinope (måne) de:Sinope (Mond) fr:Sinopé (lune) hr:Sinopa (mjesec) it:Sinope (astronomia) lt:Sinopė (palydovas) nl:Sinope (maan) ja:シノーペ (衛星) nn:Jupitermånen Sinope pl:Sinope (księżyc) sk:Sinope (mesiac) sl:Sinopa (luna) sr:Синопе fi:Sinope (kuu) sv:Sinope (måne) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||


