Kale

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The moon of Jupiter – Kale (XXXVII) – was previously temporarily designated as S/2001 J8. It was discovered in mid-December 2001 by the following team of astronomers: S.S. Sheppard, D.C. Jewitt i J. Kleyna. This discovery was achieved by the 3.6-m Canada-France-Hawaii telescope atop Mauna Kea (Hawaii). You can read additional details in Minor Planet Electronic Circular (MPEC).
    Kale is one of eleven new satellites discovered since the →Voyager-2 Jupiter system fly-by which occured 22 years ago (1979). With this moon, the team discovered also: Autonoe, Thyone, Hermippe, Eurydome, Sponde, Pasithee, Euanthe, Orthosie, Euporie and Aitne.
    The name of that moon is of mythological origin. Kale was daughter of Zeus, one of the Charites (gr. Chárites), better known as the Roman Graces, personifications of charm and joy. Most authors name three of them being the famous Three Graces: Euphrosyne ("Mirth"), Aglaea ("Splendor") and Thalia ("Good Cheer"). They were often depicted in sculptures and paintings as three naked beauties already since the Hellenistic Times... Some mythologists speculate that she may have been the wife of Hephaistos (god of smiths and smith of the gods) since she was an allegory of the beauty of that sort of craftmanship (according to other traditions his wife was Aphrodite).  
    The moon by this name is in elliptical retrograde orbit (→eccentricity e = 0.2599) with a →semimajor axis a = 23,217,000 km. At pericenter (closest to the planet) Kale is separated from the Jupiter a distance of q = 17,182,902 km. At apocenter (furthest from the planet) this moon is separated from the Jupiter a distance of Q = 29,251,098 km. In future these parameters may vary due to a large orbital distance from Jupiter and the orbital motion being disturbed by the Sun and other factors. Perhaps it is a captured asteroid (with a microscopic mass: ~1.4987×10¹³ kg – it equals 490 times less than a mountain like Giewont!), and in future will possibly return to heliocentric orbit.