Discovery[1] | |
---|---|
Discovered by | Pan-STARRS 1 |
Discovery site | Haleakalā Obs. |
Discovery date | 8 October 2010 |
Designations | |
1995 SN55[2] 2014 OK394 | |
3:5 resonant[3] · TNO[4] · distant[2] | |
Orbital characteristics[4] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 2 | |
Observation arc | 25.14 yr (9,181 days) |
Earliest precovery date | 20 September 1995 (Spacewatch)[5] |
Aphelion | 49.153 AU |
Perihelion | 35.351 AU |
42.252 AU | |
Eccentricity | 0.16333 |
274.65 yr | |
30.889° | |
0° 0m 12.919s / day | |
Inclination | 4.140° |
128.384° | |
≈ 4 January 1997[6] | |
247.580° | |
Physical characteristics | |
160–280 km (est. 0.08–0.20)[7][8] | |
6.2[2][4] | |
(523731) 2014 OK394 (provisional designation 1995 SN55) is a trans-Neptunian object that orbits in the outer Solar System beyond the orbit of Neptune. First observed as 1995 SN55 by Spacewatch on 20 September 1995, it was a lost minor planet with an insufficiently defined orbit with only 36 days of observations.[9] On 8 October 2010, it was rediscovered by the Pan-STARRS 1 survey and later announced as 2014 OK394 in July 2016.[1] It was not until November 2020 when amateur astronomers S. Deen and K. Ly identified 2014 OK394 and 1995 SN55 as the same object.[10] This identification was confirmed and announced by the Minor Planet Center in January 2021.[11]
Once thought to be a centaur crossing the orbits of the gas giants,[9] 1995 SN55 is now known to be a trans-Neptunian object in a 3:5 orbital resonance with Neptune.[4] With an estimated diameter between 160–280 kilometers (99–170 miles), it was formerly considered one of the largest centaurs.[7][12][13]
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