Discovery[1] | |
---|---|
Discovered by | NEAT (644) |
Discovery site | Palomar Mountain |
Discovery date | 15 October 2002 |
Designations | |
(55636) 2002 TX300 | |
Orbital characteristics[1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 2 | |
Observation arc | 22380 days (61.27 yr) |
Aphelion | 48.365 AU (7.2353 Tm) |
Perihelion | 37.8672 AU (5.66485 Tm) |
43.116 AU (6.4501 Tm) | |
Eccentricity | 0.12174 |
283.12 yr (103408 d) | |
73.7618° | |
0° 0m 12.533s / day | |
Inclination | 25.87838° |
324.6984° | |
338.958° | |
Physical characteristics | |
Mass | ~1.2×1019 kg (assumed)[6] |
8.12 h (0.338 d) | |
0.504 d (12.101 h)[1] | |
Temperature | < 41 K |
19.4[9] | |
3.4[1] | |
(55636) 2002 TX300 is a bright Kuiper belt object in the outer Solar System estimated to be about 286 kilometres (178 mi) in diameter.[4] It is a large member of the Haumea family that was discovered on 15 October 2002 by the Near-Earth Asteroid Tracking (NEAT) program.[1]
2002 TX300 is a classical Kuiper belt object with an absolute magnitude between that of 50000 Quaoar and 20000 Varuna. 2002 TX300 has the most eccentric and inclined orbit of the three.
A variability of the visual brightness was also detected which could fit to 7.9 h or 15.8 h rotational period (the distinction between single or double-peaked curved could not be made with confidence). The changes in brightness are quite close to the error margin and could also be due to an irregular shape.[10]
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