2005 RH52
 | The topic of this article may not meet Wikipedia's notability guideline for astronomical objects. (August 2017) |
| Designations | |
|---|---|
| 2005 RH52 | |
| Detached object | |
| Orbital characteristics | |
| Epoch 2016-07-31.0, JD=2457600.5 | |
| Aphelion | 263.434 au |
| Perihelion | 38.9788709 au |
| 151.2066497 au | |
| 1859 years | |
| 2.55993° | |
| 0.00053010°/day | |
| Inclination | 20.45750° |
| 306.14871° | |
| 32.34277° | |
2005 RH52, is a trans-Neptunian object discovered at Mauna Kea on September 3, 2005.
It is one a small number of detached objects with perihelion distances of 30 AUs or more, and semi-major axes of 150 AU or more.[1] Such objects can not reach such orbits without some perturbing object, which lead to the speculation of planet nine.
Notes
References
External links
- 2005 RH52 at the JPL Small-Body Database
 | This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it. |