Sao (moon)
| Discovery [1][2] | |
|---|---|
| Discovered by |
|
| 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. Retrieved 2011-10-24.
- ↑ Green, Daniel W. E. (January 13, 2003). "Satellites of Neptune". IAU Circular 8047. Retrieved 2011-10-24.
- ↑ Jacobson, R. A. (2008). "NEP078 – JPL satellite ephemeris". Planetary Satellite Mean Orbital Parameters. Retrieved 2009-09-23.
- ↑ 4.0 4.1 4.2 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.
- ↑ 5.0 5.1 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.
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