2010 VK201
| Discovery[1] | |
|---|---|
| Discovered by | S. D. Benecchi, Las Campanas Observatory |
| Discovery date | 2011 |
| Designations | |
| MPC designation | 2010 VK201 |
| TNO | |
| Orbital characteristics[2] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 5 | |
| Observation arc | 736 days (2.02 yr) |
| Aphelion | 47.943 AU (7.1722 Tm) (Q) |
| Perihelion | 38.282 AU (5.7269 Tm) (q) |
| 43.113 AU (6.4496 Tm) (a) | |
| Eccentricity | 0.11204 (e) |
| 283.08 yr (103397 d) | |
| 173.94° (M) | |
| 0° 0m 12.534s /day (n) | |
| Inclination | 28.861° (i) |
| 156.60° (Ω) | |
| 82.855° (ω) | |
| Earth MOID | 37.3962 AU (5.59439 Tm) |
| Jupiter MOID | 33.5753 AU (5.02279 Tm) |
| Physical characteristics | |
| Dimensions | 520 km (from assumed albedo)[3] |
| 7.59 h (0.316 d) | |
Sidereal rotation period | 7.6 h[2] |
| 0.08 (assumed)[3] | |
|
4.6,[2] 4.9,[3] 4.5[1] | |
|
| |
2010 VK201, also written as 2010 VK201, is a trans-Neptunian object and likely a dwarf planet.[3]
References
- 1 2 MPEC 2011-U10 : 2010 VK201
- 1 2 3 "JPL Small-Body Database Browser: (2010 VK201)" (last observation: 2012-11-08 (arc=736 days (2.02 years))). Jet Propulsion Laboratory. Retrieved 31 March 2016.
- 1 2 3 4 "How many dwarf planets are there in the outer solar system?". Gps.caltech.edu. 2013-11-01. Archived from the original on 2011-10-18. Retrieved 2014-06-13.
External links
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