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(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]

82158 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°
0° 0m 1.042s / day
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]

See alsoEdit

ReferencesEdit

  1. ^ a b c d "JPL Small-Body Database Browser: 82158 (2001 FP185)" (last observation: 2014-12-21; arc: 6.74 years). Retrieved 7 April 2016. 
  2. ^ a b c AstDys-2 Retrieved 2011-09-05
  3. ^ a b 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. ^ a b Accurate absolute magnitudes for Kuiper belt objects and centaurs
  5. ^ de la Fuente Marcos, C.; de la Fuente Marcos, R. (1 September 2014). "Extreme trans-Neptunian objects and the Kozai mechanism: signalling the presence of trans-Plutonian planets". Monthly Notices of the Royal Astronomical Society: Letters. 443 (1): L59–L63. arXiv:1406.0715 . Bibcode:2014MNRAS.443L..59D. doi:10.1093/mnrasl/slu084. 
  6. ^ de la Fuente Marcos, C.; de la Fuente Marcos, R.; Aarseth, S. J. (11 January 2015). "Flipping minor bodies: what comet 96P/Machholz 1 can tell us about the orbital evolution of extreme trans-Neptunian objects and the production of near-Earth objects on retrograde orbits". Monthly Notices of the Royal Astronomical Society. 446 (2): 1867–1873. arXiv:1410.6307 . Bibcode:2015MNRAS.446.1867D. doi:10.1093/mnras/stu2230. 

External linksEdit