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Iocaste (moon)

From Wikipedia, the free encyclopedia

Iocaste (eye'-ə-kas'-tee, IPA: [ˌaɪəˈkæsti]; Greek Ιοκάστη), or Jupiter XXIV, is a retrograde irregular satellite of Jupiter. It was discovered by a team of astronomers from the University of Hawaii led by Scott S. Sheppard in 2000, and given the temporary designation S/2000 J 3.

Iocaste orbits Jupiter at an average distance of 20,723 Mm in 609.427 days, at an inclination of 147° to the ecliptic (146° to Jupiter's equator) with an eccentricity of 0.2874.

It is named after Jocasta, the mother/wife of Oedipus in Greek mythology.

Iocaste belongs to the Ananke group, believed to be the remnants of a break-up of a captured heliocentric asteroid.[1][2]

The satellite is about 5 kilometres in diameter[3] and appears grey (colour indices B-V=0.63, R-V=0.36), similar to C-type asteroids.[4]

The moon Iocaste should be distinguished from the asteroid 899 Jokaste.

[edit] See also

[edit] External links

[edit] References

  1. ^ Scott S. Sheppard, David C. Jewitt An abundant population of small irregular satellites around Jupiter, Nature, 423 (May 2003), pp.261-263 (pdf)
  2. ^ David Nesvorný, Jose L. A. Alvarellos, Luke Dones, and Harold F. Levison Orbital and Collisional Evolution of the Irregular Satellites, The Astronomical Journal,126 (2003), pages 398–429. (pdf)
  3. ^ Scott S. Sheppard, David C. Jewitt, Carolyn Porco Jupiter's outer satellites and Trojans, In: Jupiter. The planet, satellites and magnetosphere. Edited by Fran Bagenal, Timothy E. Dowling, William B. McKinnon. Cambridge planetary science, Vol. 1, Cambridge, UK: Cambridge University Press, ISBN 0-521-81808-7, 2004, p. 263 - 280 (pdf).
  4. ^ Grav, Tommy; Holman, Matthew J.; Gladman, Brett J.; Aksnes, Kaare Photometric survey of the irregular satellites,Icarus, 166,(2003), pp. 33-45. Preprint
  • Ephemeris (IUA)[1]
  • Mean orbital parameters (NASA)[2]


... | Orthosie | Iocaste | S/2003 J 16 | ...
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