|Discovered by||Henry G. Roe, Michael E. Brown, Kristina M. Barkume|
|Discovery date||September 22, 2004|
|MPC designation||(120347) 2004 SB60|
|Pronunciation||// or //|
|Epoch JD 2457000.5 (9 December 2014)|
|271.29 yr (99088 d)|
4.66±0.22)×1020 kg (system mass) (
Sidereal rotation period
120347 Salacia is a large planetoid of the Kuiper belt. It was discovered on September 22, 2004 by Henry G. Roe, Michael E. Brown and Kristina M. Barkume at the Palomar Observatory. It is probably a dwarf planet. Salacia's diameter is estimated to be 850 kilometres (530 mi) due to a low albedo. It has been observed 100 times, with precovery images back to 1982. Salacia orbits the Sun at an average distance slightly greater than that of Pluto.
Even though Salacia has an inclination of 24°, it is not a member of the Haumea family, since the near infrared spectrum is basically featureless and shows less than 5% water ice. The total mass of the Salacia–Actaea system is 4.66±0.22)×1020 kg. From the relative diameters, about 96% of this mass should be in Salacia itself. Salacia has the lowest (albedo and density known of any TNO that big.
Salacia has one natural satellite, Actaea, that orbits its primary every 5.494 days at a distance of 5619±87 km and with an eccentricity of 0.0084±0.0076. It has a diameter of 286±24 km to 303±35 km. It was discovered on 21 July 2006 by Keith S. Noll, Harold Levison, Denise Stephens and Will Grundy with the Hubble Space Telescope.
- sal-AY-shee-ə, sə-LAY-shə
- "MPEC 2009-R09 :Distant Minor Planets (2009 SEPT. 16.0 TT)". IAU Minor Planet Center. 2009-09-04. Retrieved 2011-07-05.
- Marc W. Buie. "Orbit Fit and Astrometric record for 120347" (2007-08-12 using 62 of 73 observations). SwRI (Space Science Department). Retrieved 2009-10-04.
- "JPL Small-Body Database Browser: 120347 Salacia (2004 SB60)" (2010-11-05 last obs). Retrieved 2015-02-13.
- S. Fornasier, E. Lellouch, T. Müller, P. Santos-Sanz, P. Panuzzo, C. Kiss, T. Lim, M. Mommert, D. Bockelée-Morvan, E. Vilenius, J. Stansberry, G.P. Tozzi, S. Mottola, A. Delsanti, J. Crovisier, R. Duffard, F. Henry, P. Lacerda, A. Barucci, & A. Gicquel (2013). TNOs are Cool: A survey of the trans-Neptunian region. VIII. Combined Herschel PACS and SPIRE observations of 9 bright targets at 70–500 µm.
- J.A. Stansberry (2012). "Physical Properties of Trans-Neptunian Binaries (120347) Salacia–Actaea and (42355) Typhon–Echidna". Elsevier. Retrieved 2012-04-27.
- MPC 73984
- Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Retrieved 2011-08-25.
- E.L. Schaller and M.E. Brown (2008). "Detection of Additional Members of the 2003 EL61 Collisional Family via Near-Infrared Spectroscopy". Astrophysical Journal. arXiv:0808.0185. Bibcode:2008ApJ...684L.107S. doi:10.1086/592232.
- "Planetary Names: Planet and Satellite Names and Discoverers". Gazetteer of Planetary Nomenclature. International Astronomical Union (Working Group for Planetary System Nomenclature). Retrieved 10 June 2012.
- NASA. "List of Dwarf Planets". Retrieved 2012-06-09.
- "IAUC 8751: (120347) 2004 SB_60; 2006gi, 2006gj; V733 Cep". Cbat.eps.harvard.edu. Retrieved 2014-06-14.
- Orbital simulation from JPL (Java) / Horizons Ephemeris
- Salacia: As big as Ceres, but much farther away (Emily Lakdawalla - 2012/06/26)