| Discovery[1][2][3] | |
|---|---|
| Discovered by |
|
| Discovery site | Las Campañas Obs. (first observed) |
| Discovery date | 21 May 2010 (first observed) |
| Designations | |
| 2010 KZ39 | |
| Orbital characteristics[4][5] | |
| Epoch 2024 October 17 (JD 2460600.5) | |
| Uncertainty parameter 4 | |
| Observation arc | 11.94 yr (4,361 days) |
| Aphelion | 47.55 AU |
| Perihelion | 42.48 AU |
| 45.01 AU | |
| Eccentricity | 0.0563 |
| 302.0 yr (110,300 days) | |
| 256.5° | |
| 0° 0m 11.736s / day | |
| Inclination | 26.156° |
| 53.277° | |
| ≈ 6 May 2110[6] ±5 months | |
| 322.6° | |
| Knownsatellites | 0 |
| Physical characteristics | |
| 743 km?[11] 660 km (estimated albedo)[12] | |
| 0.10(assumed)[7] | |
| 20.7[13] | |
| |
2010 KZ39 is atrans-Neptunian object orbiting the Sun as adetached object in the outer reaches of theSolar System. The object was first observed on 21 May 2010 by astronomersAndrzej Udalski,Scott Sheppard, M. Szymanski andChad Trujillo at theLas Campañas Observatory in Chile.[1][3]

2010 KZ39 orbits the Sun at a distance of 42.5–47.6 AU once every 302 years, similar toMakemake,19521 Chaos and other bodies that circle the Sun in 6:11resonance toNeptune. Its orbit has aneccentricity of 0.056 and aninclination of 26° with respect to theecliptic.
Using the best-fit values for its orbit, it is expected to come toperihelion in 2109.[4] It has been observed 50 times over 12 years and has anuncertainty parameter of 4.[1] As of 2016, it is 46.1 AU from the Sun.[13] The body's spectral type as well as its rotation period remain unknown.
This article about acentaur (minor planet) ortrans-Neptunian object is astub. You can help Wikipedia byexpanding it. |