(65407) 2002 RP120
| Discovery | |
|---|---|
| Discovered by |
Brian A. Skiff (LONEOS) |
| Discovery date | 4 September 2002 |
| Designations | |
|
Damocloid Scattered disk object | |
| Orbital characteristics [1] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 1225 days (3.35 yr) |
| Aphelion | 107.08 AU (16.019 Tm) |
| Perihelion | 2.4759 AU (370.39 Gm) |
| 54.780 AU (8.1950 Tm) | |
| Eccentricity | 0.95480 |
| 405.45 yr (148092 d) | |
Average orbital speed | 3.98 km/s |
| 11.779° | |
| 0° 0m 8.751s / day | |
| Inclination | 119.00° |
| 39.238° | |
| 357.99° | |
| Earth MOID | 1.48322 AU (221.887 Gm) |
| Jupiter MOID | 2.50008 AU (374.007 Gm) |
| Physical characteristics | |
| Dimensions | 14.6 km[1] |
Mean radius | 7.3 ± 1.4 km |
| Mass | 3.1×1015 kg |
| 200 h (8.3 d)[1] | |
| 0.098 ± 0.036[1] | |
| Temperature | ~ 37 K |
| 12.3[1] | |
|
| |
(65407) 2002 RP120 (also written (65407) 2002 RP120) is a damocloid, which means it is also a member of a small group of retrograde minor planets. Aside from being a damocloid, it is also a scattered-disc object – a trans-Neptunian object with a very eccentric orbit, probably ejected from the ecliptic by Neptune.
References
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