- Sao (moon)
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Sao Discovery [1][2] Discovered by - M.Holman
- JJ Kavelaars
- T. Grav
- W. Fraser
- D. Milisavljevic
Discovered August 14, 2002 Mean Orbital elements [3] Epoch June 10, 2003 Semi-major axis 22.228 Gm Eccentricity 0.1365 Inclination 53.483° * Orbital period 2912.72 days
(7.97 yr)Physical characteristics Mean diameter 44 km[4] ** Rotation period ? Albedo 0.04 assumed[4] Color ? Spectral type ? *to the ecliptic **based on the albedo Sao ( /ˈseɪ.oʊ/ say-oh; Greek: Σαώ) is a prograde irregular satellite of Neptune. It was discovered by Matthew J. Holman et al. on August 14, 2002.[5]
Sao orbits Neptune at a distance of about 22.4 million km and is about 44 kilometers in diameter (assuming an albedo of 0.04).[4]
Sao follows an exceptionally inclined and moderately 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.
The satellite is in so-called Kozai resonance, i.e. its inclination and eccentricity are coupled (the inclination of the orbit decreases while eccentricity increases and vice versa).[5]
Sao, or Neptune XI, like many of the outer satellites of Neptune, is named after one of the Nereids; Sao was associated with sailing and is referred to as "The rescuer" or "Safety". Before the announcement of its name on February 3, 2007 (IAUC 8802), Sao was known provisionally as S/2002 N 2.
References
- ^ JPL (2011-07-21). "Planetary Satellite Discovery Circumstances". Jet Propulsion Laboratory. http://ssd.jpl.nasa.gov/?sat_discovery. Retrieved 2011-10-24.
- ^ Green, Daniel W. E. (January 13, 2003). "Satellites of Neptune". IAU Circular 8047. http://www.cbat.eps.harvard.edu/iauc/08000/08047.html. Retrieved 2011-10-24.
- ^ Jacobson, R. A. (2008). "NEP078 – JPL satellite ephemeris". Planetary Satellite Mean Orbital Parameters. http://ssd.jpl.nasa.gov/?sat_elem. Retrieved 2009-09-23.
- ^ 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.
- ^ a b 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. https://www.cfa.harvard.edu/~mholman/nature_final.pdf. Retrieved 2011-10-24.
External links
Moons of Neptune Generally listed in increasing distance from NeptuneRegular (inner) Triton Irregular See also Neptune Discovery Characteristics - Rings
- Great Dark Spot
- Small Dark Spot
- The Scooter
- Kuiper belt
Moons Exploration Trojans Miscellaneous Categories:- Moons of Neptune
- Irregular satellites
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