120347 Salacia

120347 Salacia
Keck Telescope image of Salacia (center) and its moon Actaea (left), taken by the NIRC2 near-infrared camera on 3 August 2010.
Discovery
Discovered byH. G. Roe
M. E. Brown
K. M. Barkume
Discovery sitePalomar Obs.
Discovery date22 September 2004
Designations
(120347) Salacia
Pronunciation/səˈlʃə/ (sə-LAY-shə)
Named after
Salacia (Roman mythology)
2004 SB60 (provisional designation)
TNO · classical (hot)
extended
AdjectivesSalacian
Symbol or (rare)
Orbital characteristics
Epoch 31 May 2020 (JD 2459000.5)
Uncertainty parameter 3
Observation arc37.16 yr (13,572 days)
Earliest precovery date25 July 1982
Aphelion46.670 AU
Perihelion37.697 AU
42.184 AU
Eccentricity0.10636
273.98 yr (100,073 days)
123.138°
0° 0m 12.951s / day
Inclination23.921°
279.880°
312.294°
Known satellites1 (Actaea)
Physical characteristics
  • 838±44 km (2025)
  • 846±21 km (2019)
  • 866±37 km (2017)
Mass4.861+0.076
−0.074
×1020 kg
(System mass)
Mean density
1.50±0.12 g/cm3
1.26±0.16 g/cm3
5.49403±0.00016 d (synchronous)
0.041±0.004 (2025)
0.042±0.004 (2017)
20.7
4.360±0.011 (Salacia+Actaea)
4.476±0.013 (Salacia)
4.15

Salacia (minor-planet designation: 120347 Salacia) is a large trans-Neptunian object (TNO) and possible dwarf planet in the Kuiper belt that is probably between 800 km (500 mi) and 875 km (544 mi) in diameter. It was discovered on 22 September 2004 by American astronomers Henry Roe, Michael Brown and Kristina Barkume at the Palomar Observatory in California, United States. Salacia orbits the Sun at an average distance that is slightly greater than that of Pluto. It was named after the Roman goddess Salacia and has a single known moon, Actaea. Salacia and Actaea form a binary system where both bodies are tidally locked to the other, similar to Pluto and Charon.