Neso (moon)

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Neso
Discovery [1][2]
Discovered by
Discovered August 14, 2002
Mean Orbital elements [3]
Epoch June 10, 2003
Semi-major axis 49.285 Gm
Eccentricity 0.5714
Inclination 136.439° *
Orbital period 9740.73 d
(26.67 a)
Physical characteristics
Mean diameter 60 km[4] **
Rotation period ?
Albedo 0.04 assumed[4]
Color ?
Spectral type ?

*to the ecliptic

**based on the albedo

Neso (/ˈns/ NEE-soh; Greek: Νησώ), also known as Neptune XIII, is the outermost irregular natural satellite of Neptune. It was discovered by Matthew J. Holman, Brett J. Gladman, et al. on August 14, 2002, though it went unnoticed until 2003.[2][5]

Irregular satellites of Neptune.

Neso orbits Neptune at a distance of more than 48 Gm (million km), making it (as of 2013) the most distant known moon of any planet[A] (about as far as Earth is from Venus at its closest point) and the moon with the longest orbital period (26.67 years). It follows a highly inclined and highly eccentric orbit 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.

Neso is about 60 km (37 mi) in diameter based on an assumed albedo, and assuming a mean density of 1.5 g/cm3,[6] its mass is estimated at 2×1017 kg.

Given the similarity of the orbit's parameters with Psamathe (S/2003 N 1), it was suggested that both irregular satellites could have a common origin in the break-up of a larger moon.[4]

Neso is named after one of the Nereids. Before the announcement of its name on February 3, 2007 (IAUC 8802), Neso was known by its provisional designation, S/2002 N 4.

References[edit]

Notes

  1. ^ Such distances are of the order of magnitude of heliocentric distances of inner planets rather than moons; at apocenter the satellite is more than 72 Gm (72 million km) from the planet to compare with Mercury's aphelion of ~70 Gm!

Citations

  1. ^ JPL (2011-07-21). "Planetary Satellite Discovery Circumstances". Jet Propulsion Laboratory. Retrieved 2011-10-24. 
  2. ^ a b Green, Daniel W. E. (October 1, 2003). "S/2001 U 2 and S/2002 N 4". IAU Circular 8213. Retrieved 2011-10-24. 
  3. ^ Jacobson, R. A. (2008). "NEP078 – JPL satellite ephemeris". Planetary Satellite Mean Orbital Parameters. Retrieved 2009-09-23. 
  4. ^ a b c Sheppard, Scott S.; Jewitt, David C.; Kleyna, Jan (2006). "A Survey for "Normal" Irregular Satellites around Neptune: Limits to Completeness". The Astronomical Journal 132: 171–176. arXiv:astro-ph/0604552. Bibcode:2006AJ....132..171S. doi:10.1086/504799.  edit
  5. ^ Holman, 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. Retrieved 2011-10-24.  edit
  6. ^ Physical parameters from JPL

External links[edit]