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ახალი გვერდი: '''Euporie''' {{IPAc-en|ˈ|j|uː|p|ə|r|iː}}, also known as '''{{nowrap|Jupiter XXXIV}}''', 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 2001, and given the temporary designation '''{{nowrap|S/2001 J 10}}'''.<ref>{{cite web |author=Daniel W. E. Green |url=http://www.cbat.eps.harvard.edu/iauc/07900/07900.html |title=IAUC 7900: Satellites of Jupiter |...
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11:52, 14 ოქტომბერი 2024-ის ვერსია

Euporie /ˈjpər/, also known as Jupiter XXXIV, 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 2001, and given the temporary designation S/2001 J 10.[1][2]

Euporie is about 2 kilometres in diameter, and orbits Jupiter at an average distance of 19.266 million km in 550.69 days, at an inclination of 145.7° to the ecliptic, in a retrograde direction and with an eccentricity of 0.148.[3] It is affected by the Kozai mechanism.[4]

It was named in August 2003 after Euporie, a Greek goddess of abundance and one of the Horae in Greek mythology (and thus a daughter of Zeus).[5] It is a member of the Ananke group.

  1. Daniel W. E. Green. (16 May 2002) IAUC 7900: Satellites of Jupiter. International Astronomical Union.
  2. Brian G. Marsden. (15 May 2002) MPEC 2002-J54: Eleven New Satellites of Jupiter. International Astronomical Union Minor Planet Center.
  3. Planetary Satellite Mean Elements. ციტირების თარიღი: 2024-01-19
  4. Brozović, Marina; Jacobson, Robert A. (2017-03-09). „The Orbits of Jupiter's Irregular Satellites“. The Astronomical Journal. 153 (4): 8. Bibcode:2017AJ....153..147B. doi:10.3847/1538-3881/aa5e4d. ISSN 0004-6256.
  5. Daniel W. E. Green. (9 August 2002) IAUC 8177: Satellites of Jupiter, Saturn, Uranus. International Astronomical Union. დაარქივებულია ორიგინალიდან — 27 March 2012.