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Halimede (moon)

From Wikipedia, the free encyclopedia
Moon of Neptune
Halimede
Halimede imaged by theVery Large Telescope during follow-up observations on 3 September 2002
Discovery[1][2]
Discovered by
Discovery dateAugust 14, 2002
Designations
Designation
Neptune IX
Pronunciation/hæləˈmd/[3]
Named after
ἉλιμήδηHalimēdē
S/2002 N 1
AdjectivesHalimedean/ˌhæləməˈdən/
Orbital characteristics[4]
Epoch June 10, 2003
16,611,000 km
Eccentricity0.2646
1,879.08 d (5.1446 a)
(retrograde)
Inclination134.1°
Physical characteristics
62 km(for albedo 0.04)[5]
Albedo0.04(assumed)[5]
Spectral type
neutral (grey)
B-V=0.73 R-V=0.35[6]

Halimede/hæləˈmd/, orNeptune IX, is aretrogradeirregular satellite ofNeptune. It was discovered byMatthew J. Holman,John J. Kavelaars,Tommy Grav, Wesley C. Fraser andDan Milisavljevic on August 14, 2002.[7]

Name

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

Orbit

[edit]
Irregular satellites of Neptune.

Halimede has the second mosteccentric and third mostinclined orbit around Neptune.[8] This is illustrated on the diagram in relation to other irregular satellites of Neptune. The satellites above the horizontal axis areprograde, the satellites beneath it areretrograde. The yellow segments extend from thepericentre to theapocentre, showing the eccentricity. It is also worth mentioning thatSao andLaomedeia are similar to Halimede but they both have prograde orbits unlike Halimede which has a retrograde orbit.[9]

Physical characteristics

[edit]

Halimede is about 62 kilometers in diameter (assuming analbedo of 0.04)[5] and appears neutral (grey) in thevisible light. Given the very similar colour of the satellite to that ofNereid together with the high probability (41%[7]) of collision in the past lifespan of the Solar System, it has been suggested that the satellite could be a fragment of Nereid.[6]

References

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  1. ^JPL (2011-07-21)."Planetary Satellite Discovery Circumstances".Jet Propulsion Laboratory. Retrieved2011-10-24.
  2. ^Green, Daniel W. E. (January 13, 2003)."Satellites of Neptune".IAU Circular.8047. Retrieved2011-10-24.
  3. ^Noah Webster (1884)A Practical Dictionary of the English Language
  4. ^Jacobson, R. A. (2008)."NEP078 – JPL satellite ephemeris".Planetary Satellite Mean Orbital Parameters. Retrieved2009-09-23.
  5. ^abcSheppard, Scott S.;Jewitt, David C.;Kleyna, Jan (2006). "A Survey for "Normal" Irregular Satellites around Neptune: Limits to Completeness".The Astronomical Journal.132 (1):171–176.arXiv:astro-ph/0604552.Bibcode:2006AJ....132..171S.doi:10.1086/504799.S2CID 154011.
  6. ^abGrav, Tommy;Holman, Matthew J.; Fraser, Wesley C. (2004-09-20). "Photometry of Irregular Satellites of Uranus and Neptune".The Astrophysical Journal.613 (1):L77–L80.arXiv:astro-ph/0405605.Bibcode:2004ApJ...613L..77G.doi:10.1086/424997.S2CID 15706906.
  7. ^abHolman, M. J.;Kavelaars, J. J.; Grav, T.; et al. (2004)."Discovery of five irregular moons of Neptune"(PDF).Nature.430 (7002):865–867.Bibcode:2004Natur.430..865H.doi:10.1038/nature02832.PMID 15318214.S2CID 4412380. Retrieved24 October 2011.
  8. ^Williams, Dr. David R. (2008-01-22)."Neptunian Satellite Fact Sheet".NASA (National Space Science Data Center). Retrieved2011-11-03.
  9. ^"In Depth | Halimede".NASA Solar System Exploration. Retrieved2020-11-10.

External links

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Wikimedia Commons has media related toHalimede (moon).
Listed in approximately increasing distance fromNeptune
Regular (inner)
Irregular
Triton
Nereid (1)
Halimede (1)
Sao group (3)
Neso group (3)
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