(82158) 2001 FP185
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(Redirected from 2001 FP185)
| Discovery[1] | |
|---|---|
| Discovered by | Marc Buie at Kitt Peak |
| Discovery date | 26 March 2001 |
| Designations | |
| MPC designation | 2001 FP185 |
| TNO[1] | |
| Orbital characteristics[1][2] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 3197 days (8.75 yr) |
| Aphelion | 418.44 AU (62.598 Tm) |
| Perihelion | 34.253 AU (5.1242 Tm) |
| 226.34 AU (33.860 Tm) | |
| Eccentricity | 0.84867 |
| 3405.37 yr (1243810 d) | |
| 1.2717° | |
| Inclination | 30.7572° |
| 179.3004° | |
| 6.9787° | |
| Earth MOID | 33.2572 AU (4.97521 Tm) |
| Jupiter MOID | 28.8042 AU (4.30905 Tm) |
| Physical characteristics | |
| Dimensions | 332+31 −24 km[3] |
| 0.046±0.007 [3] | |
| 21.86 [2] | |
| 6.38 [4] 6.2[1] 6.1 [2] HR: 5.80 [4] |
|
(82158) 2001 FP185 is a scattered disc object. If a massive trans-Neptunian object exists, 2001 FP185 may be co-orbital with it.[5][6]
See also
References
- ↑ 1.0 1.1 1.2 1.3 Lua error in package.lua at line 80: module 'strict' not found.
- ↑ 2.0 2.1 2.2 AstDys-2 Retrieved 2011-09-05
- ↑ 3.0 3.1 Santos-Sanz, P., Lellouch, E., Fornasier, S., Kiss, C., Pal, A., Müller, T. G., Vilenius, E., Stansberry, J., Mommert, M., Delsanti, A., Mueller, M., Peixinho, N., Henry, F., Ortiz, J. L., Thirouin, A., Protopapa, S., Duffard, R., Szalai, N., Lim, T., Ejeta, C., Hartogh, P., Harris, A. W., & Rengel, M. (2012). “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
- ↑ 4.0 4.1 Accurate absolute magnitudes for Kuiper belt objects and centaurs
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
- ↑ Lua error in package.lua at line 80: module 'strict' not found.
External links
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