![]() 2002 GB32 is seen lower right in blue with hypothetical Planet Nine in green | |
Discovery [1] | |
---|---|
Discovered by | M. W. Buie [2] |
Discovery site | Cerro Tololo Obs. |
Discovery date | 7 April 2002 |
Designations | |
2002 GB32 | |
TNO [3] · SDO [2] [4] distant [1] · detached | |
Orbital characteristics [3] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 3 | |
Observation arc | 12.96 yr (4,733 days) |
Aphelion | 402.66 AU |
Perihelion | 35.347 AU |
219.01 AU | |
Eccentricity | 0.8386 |
3241.10 yr (1,183,810 days) | |
0.3780° | |
0° 0m 1.08s / day | |
Inclination | 14.176° |
176.99° | |
37.158° | |
Physical characteristics | |
Dimensions | 122 km (calculated) [4] |
0.09 (assumed) [4] | |
7.8 [3] | |
2002 GB32 is a trans-Neptunian object from the scattered disc in the outermost region of the Solar System, approximately 122 kilometers in diameter. [3] [4] It was first observed on 7 April 2002, by American astronomer Marc Buie at Cerro Tololo Observatory in Chile. [1] [2]
2002 GB32 belongs to a small number of detached objects with perihelion distances of 30 AU or more, and semi-major axis of 200 AU or more. [5] Such objects can not reach such orbits without some perturbing object, which leads to the speculation of Planet Nine.
This minor planet orbits the Sun at a distance of 35.3–402.7 AU once every 3,241 years and 1 month (1,183,810 days). Its orbit has an eccentricity of 0.84 and an inclination of 14° with respect to the ecliptic. [3]
Based on an absolute magnitude of 7.8 and an assumed albedo of 0.09, Johnston's Archive calculated a mean-diameter of 122 kilometers. [4]