(40314) 1999 KR16
Discovery [1] | |
---|---|
Discovered by | A. Dalsanti O. R. Hainaut |
Discovery site | ESO–La Silla Obs. |
Discovery date | 16 May 1999 |
Designations | |
MPC designation | (40314) 1999 KR16 |
1999 KR16 | |
TNO | |
Orbital characteristics [1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 3 | |
Observation arc | 5877 days (16.09 yr) |
Aphelion | 64.024 AU (9.5779 Tm) |
Perihelion | 33.987 AU (5.0844 Tm) |
49.005 AU (7.3310 Tm) | |
Eccentricity | 0.30647 |
343.06 yr (125304 d) | |
345.41° | |
Inclination | 24.778° |
205.58° | |
58.261° | |
Earth MOID | 33.0383 AU (4.94246 Tm) |
Jupiter MOID | 29.0377 AU (4.34398 Tm) |
Physical characteristics | |
Dimensions | 254±37 km[2] 235.25 km (derived)[3] |
11.7 h (0.49 d)[4] 5.8 h[5] |
|
0.204±0.070[2] 0.10 (assumed)[3] |
|
C [3] | |
5.9[1] | |
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(40314) 1999 KR16, also written as (40314) 1999 KR16, is a carbonaceous and eccentric minor planet, classified as trans-Neptunian object (TNO), about 250 kilometers in diameter. It was discovered by French female astronomer Audrey Delsanti and Oliver Hainaut at ESO's La Silla Observatory, Chile, on 16 May 1999.[6]
The C-type minor planet orbits the Sun at a distance of 34–64 AU once every 342 years and 1 month (124,953 days). Its orbit shows a high eccentricity of 0.31 and is notably tilted by 25 degrees to the plane of the ecliptic. It has a rotation period of 6 to 12 hours[4][5] and an albedo of 0.20.[2]
References
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External links
- “TNOs are Cool”: A Survey of the Transneptunian Region IV - Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS
- TNO listing – at Minor Planet Center
- TNO listing – at johnstonsarchive.net
- Asteroid Lightcurve Database (LCDB), query form (info)
- (40314) 1999 KR16 at the JPL Small-Body Database
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