(505448) 2013 SA100, provisional designation 2013 SA100 and also known as o3l79,[2] is a trans-Neptunian object from the classical Kuiper belt in the outermost region of the Solar System. It was discovered on 5 August 2013, by astronomer with the Outer Solar System Origins Survey at the Mauna Kea Observatories, Hawaii, in the United States.[1] The classical Kuiper belt object belongs to the hot population and is a weak dwarf planet candidate, approximately 260 kilometers (160 miles) in diameter.
Discovery[1] | |
---|---|
Discovered by | OSSOS |
Discovery site | Mauna Kea Obs. |
Discovery date | 5 August 2013 |
Designations | |
(505448) 2013 SA100 | |
2013 SA100 · o3l79[2] | |
TNO[3] · cubewano[4] p-DP[5] · distant[1] | |
Orbital characteristics[3] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 4 · 3[1] | |
Observation arc | 4.07 yr (1,486 d) |
Aphelion | 53.810 AU |
Perihelion | 38.607 AU |
46.209 AU | |
Eccentricity | 0.1645 |
314.12 yr (114,732 d) | |
249.56° | |
0° 0m 11.16s / day | |
Inclination | 8.4892° |
27.788° | |
114.99° | |
Physical characteristics | |
Mean diameter | 255 km (est.)[5] 267 km (est.)[4] |
0.08 (assumed)[5] 0.09 (assumed)[4] | |
g–r = 0.61[2] r–z = 0.47[2] | |
6.1[1][3] | |
It orbits the Sun at a distance of 38.6–53.8 AU once every 314 years and 1 month (114,732 days; semi-major axis of 46.21 AU). Its orbit has an eccentricity of 0.16 and an inclination of 8° with respect to the ecliptic.[3] The body's observation arc begins with its official discovery observation at Mauna Kea Observatories in August 2013.[1]
As a cubewano, also known as classical Kuiper belt object,[4] 2013 SA100 is located in between the resonant plutino and twotino populations and has a low-eccentricity orbit. With an inclination above 8°, it belongs to the "stirred" hot population rather than to the cold population with lower inclinations.[2]
This minor planet was numbered by the Minor Planet Center on 4 November 2017 and received the number 505448 in the minor planet catalog (M.P.C. 107067).[6] As of 2018, it has not been named.[1]
According to the American astronomer Michael Brown, 2013 SA100 measures 255 kilometers in diameter based on an assumed albedo of 0.08.[5] On his website, Brown lists this object as a "possible" dwarf planet (200–400 km), which is the category with the lowest certainty in his 5-class taxonomic system.[5] Similarly, Johnston's archive estimates a diameter 267 kilometers using an albedo of 0.09.[4]
Spectroscopic measurements by the OSSOS team at the Gemini Observatory and with the Subaru Telescope gave a g–r and r–z color index of 0.61 and 0.47, respectively.[2] As of 2018, no rotational lightcurve has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[3][7]