Halimede (moon)

From Wikipedia, the free encyclopedia

Halimede
Discovery [1]
Discovered by M.Holman
JJ Kavelaars
T. Grav, W. Fraser
D. Milisavljevic
Discovered August 14, 2002
Mean Orbital elements [2]
Epoch June 10, 2003
Semi-major axis 15.728 Gm
Eccentricity 0.5711
Inclination 134° *
Orbital period 1879.7 d
(5.15 a)
Physical characteristics
Mean diameter 62 km[2] **
Rotation period ?
Albedo 0.04 assumed[2]
Color neutral (grey)
B-V=0.73 R-V=0.35[3]
Spectral type ?
*to the ecliptic **based on the albedo
This box: view  talk  edit
Halimede is encircled in these 2 photographs
Halimede is encircled in these 2 photographs

Halimede (pronounced /ˈhælɪˈmiːdi/; Greek Αλιμήδη) is a retrograde irregular satellite of Neptune. It was discovered by Matthew J. Holman et al. on August 14, 2002.[4]

Irregular satellites of Neptune.
Irregular satellites of Neptune.

Halimede has the second most eccentric and third most inclined orbit around Neptune.[5] This is illustrated on the diagram in relation to other irregular satellites of Neptune. The satellites above the horizontal axis are prograde, the satellites beneath it are retrograde. The yellow segments extend from the pericentre to the apocentre, showing the eccentricity.

Halimede is about 62 kilometres in diameter (assuming an albedo of 0.04).[2] and appears neutral (grey) in the visible light. Given the very similar colour of the satellite to that of Nereid together with a high probability (41%[4]) of their collision in the lifespan of the Solar system, it has been suggested that the satellite could be a fragment of Nereid.[3]

Halimede, or Neptune IX, like many of the outer satellites of Neptune, is named after one of the Nereids, the fifty daughters of Nereus and Doris. Before the announcement of its name on February 3, 2007 (IAUC 8802), Halimede was known by the provisional designation S/2002 N 1.


[edit] See also

[edit] References

  1. ^ Discovery Circumstances from JPL
  2. ^ a b c d S. Sheppard, D. Jewitt and J. Kleyna A Survey for "Normal" Irregular Satellites Around Neptune: Limits to Completeness, The Astronomical Journal, 132 (2006), pp. 171–176. Preprint.
  3. ^ a b T. Grav, M. Holman and W. Fraser Photometry of Irregular Satellites of Uranus and Neptune, The Astrophysical Journal, 613 (2004), pp.L77–L80. Preprint
  4. ^ a b M. Holman, JJ Kavelaars, B. Gladman, T. Grav, W. Fraser, D. Milisavljevic, P. Nicholson, J. Burns, V. Carruba, J.-M. Petit, P. Rousselot, O. Mousis, B. Marsden, R. Jacobson, Discovery of five irregular moons of Neptune, Nature, 430 (2004), pp. 865-867. Final preprint(pdf)
  5. ^ Williams, Dr. David R. (23 November 2006). Neptunian Satellite Fact Sheet. NASA. Retrieved on 2008-01-16.

[edit] External links