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1 See also  





2 References  





3 External links  














Psamathe (moon)






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Psamathe
Discovery images of Psamathe by the Subaru Telescope in 2003
Discovery[1][2]
Discovered by
  • David C. Jewitt
  • J. Kleyna
  • Discovery date19 August 2003
    Designations

    Designation

    Neptune X
    Pronunciation/ˈsæməθ/

    Named after

    Ψαμάθη Psamathē

    Alternative names

    S/2003 N 1
    AdjectivesPsamathean /sæməˈθən/
    Orbital characteristics
    Epoch 1 January 2000 (Proper orbital element)
    Observation arc20.97 yr (7,660 days)[3]

    Mean anomaly

    183.3° (proper)
    Satellite ofNeptune
    GroupNeso group
    Proper orbital elements[4]

    Proper semi-major axis

    47,615,100 km = 0.318 AU

    Proper eccentricity

    0.414

    Proper inclination

    127.8°

    Proper mean motion

    14.371255 deg / yr

    Proper orbital period

    25.05 yr
    (9149.514 d)

    Precession of perihelion

    874.6486 arcsec / yr

    Precession of the ascending node

    972.3189 arcsec / yr
    Physical characteristics

    Mean diameter

    40 km (for albedo 0.04)[5]
    Albedo0.04 (assumed)[5]

    Psamathe /ˈsæməθ/, also known as Neptune X, is a retrograde irregular satellite of Neptune. It is named after Psamathe, one of the Nereids. Psamathe was discovered by Scott S. Sheppard and David C. Jewitt in 2003 using the 8.2 meter Subaru Telescope.[5] Before it was officially named on February 3, 2007 (IAUC 8802), it was known by the provisional designation S/2003 N 1.[6]

    Animation of Psamathe moving in images by Very Large Telescope on 13 July 2010

    Psamathe is about 38 kilometers in diameter. It orbits Neptune at a distance of between 25.7 and 67.7 million km (for comparison, the Sun-Mercury distance varies between 46 million and 69.8 million km) and requires almost 25 Earth years to make one orbit. The orbit of this satellite is close to the theoretical stable separation from Neptune for a body in a retrograde orbit. Given the similarity of Psamathe's orbital parameters with Neso (S/2002 N 4), it was suggested that both irregular satellites could have a common origin in the breakup of a larger moon.[5] Both are farther from their primary than any other known moon in the Solar System.[7]

    See also[edit]

    References[edit]

    1. ^ JPL (2011-07-21). "Planetary Satellite Discovery Circumstances". Jet Propulsion Laboratory. Retrieved 2011-10-24.
  • ^ Green, Daniel W. E. (September 3, 2003). "Satellites of Neptune". IAU Circular. 8193. Retrieved 2011-10-24.
  • ^ "Natural Satellites Ephemeris Service". Minor Planet Center. Retrieved 3 March 2024. Selection of Objects → "All Neptunian outer irregular satellites" → Check "I require Orbital Elements" → Get Information
  • ^ Jacobson, R. A. (2008). "NEP078 - JPL satellite ephemeris". Planetary Satellite Mean Orbital Parameters. Retrieved 2009-09-23.
  • ^ a b c d Sheppard, 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.
  • ^ Marsden, Brian G. (2003). "MPEC 2003-R19 : S/2003 N 1". Minor Planet Center, Smithsonian Astrophysical Observatory. Retrieved 2011-01-08.
  • ^ Schmude, Richard Jr. (2008). Uranus, Neptune, Pluto and How to Observe Them. Springer. p. 106. ISBN 978-0-387-76601-0.
  • External links[edit]


    Retrieved from "https://en.wikipedia.org/w/index.php?title=Psamathe_(moon)&oldid=1230829887"

    Categories: 
    Neso group
    Moons of Neptune
    Irregular satellites
    Discoveries by Scott S. Sheppard
    Astronomical objects discovered in 2003
    Moons with a retrograde orbit
    Hidden categories: 
    Articles with short description
    Short description matches Wikidata
    Commons category link is on Wikidata
     



    This page was last edited on 24 June 2024, at 23:23 (UTC).

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