| Discovery | |
|---|---|
| Discovered by | Gary M. Bernstein |
| Discovery date | 29 May 1998 |
| Designations | |
| (85633) 1998 KR65 | |
| 1998 KR65 | |
| TNO · cubewano[1][2][3] cold[4] | |
| Orbital characteristics[5] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter3 | |
| Observation arc | 3289 days (9.00 yr) |
| Aphelion | 44.719 AU (6.6899 Tm) |
| Perihelion | 41.986 AU (6.2810 Tm) |
| 43.352 AU (6.4854 Tm) | |
| Eccentricity | 0.031514 |
| 285.45 yr (104260 d)[6] | |
| 247.48° | |
| 0° 0m 12.43s / day | |
| Inclination | 1.1903° |
| 101.95° | |
| 338.56° | |
| Physical characteristics | |
Mean diameter | 192 km[1] |
| 0.09 (assumed) | |
| 6.7 | |
(85633) 1998 KR65 (provisional designation 1998 KR65) is a trans-Neptunian object from the classical Kuiper belt, located in the outermost region of the Solar System. The cubewano belongs to the cold population. It has a perihelion (closest approach to the Sun) at 42.385 AU and an aphelion (farthest approach from the Sun) at 44.859 AU. It is about 192 km in diameter. It was discovered on 29 May 1998, by Gary M. Bernstein.
2007-05-22 using 55 observations
|
| |
|---|---|
| TNO classes |
|
| Dwarf planets (moons) |
|
| Sednoids |
|
 | This article about a centaur (minor planet)ortrans-Neptunian object is a stub. You can help Wikipedia by expanding it. |
