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|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=445473
|url=http://www.minorplanetcenter.net/db_search/show_object?object_id=445473
|accessdate=2015-11-11}}</ref>
|accessdate=2015-11-11}}</ref>
| epoch = January 13, 2016 ([[Julian day|JD]] 2457400.5)<br>([[Uncertainty Parameter U|Uncertainty]]=3)
| epoch = January 13, 2016 ([[Julian day|JD]] 2457400.5)
| uncertainty = 3
| aphelion = 271.482 [[Astronomical unit|AU]] (Q)
| aphelion = 271.482 [[Astronomical unit|AU]] (Q)
| perihelion = 34.3218 ± 0.0014 AU (q)
| perihelion = 34.3218 ± 0.0014 AU (q)

Revision as of 16:01, 11 November 2015

2010 VZ98
Discovery[1]
Discovery dateNovember 2010
Designations
Designation
2010 VZ98
TNO (SDO)[2]
Orbital characteristics[3]
Epoch January 13, 2016 (JD 2457400.5)
Uncertainty parameter 3
Aphelion271.482 AU (Q)
Perihelion34.3218 ± 0.0014 AU (q)
152.9019 AU (a)
Eccentricity0.77553 ± 0.00016
1891 yr
357.73300
Inclination4.50967°±0.00001°
117.4391°±0.0045° (Ω)
313.9021°±0.0045° (ω)
Physical characteristics
Dimensions461 km (assumed)[4]
9.72 h?[5]
Albedo0.07 (assumed)[4]
5.1[3]

(445473) 2010 VZ98 is a trans-Neptunian object (TNO) orbiting the Sun in the scattered disc. It was discovered in November 2010 when it was 38 AU from the Sun. With an absolute magnitude of 5.0,[5] it is likely a dwarf planet and might be around 500 kilometres (310 mi) in diameter.[4]

Small number statistics suggest (445473) 2010 VZ98 may be trapped in a 3:2 orbital resonance with an unseen planet beyond Neptune with a semi-major axis of 195–215 AU.[6]

References

  1. ^ "MPEC 2011-Q57 : 2010 VZ98". IAU Minor Planet Center. 2011-08-31. Retrieved 2012-08-31.
  2. ^ "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2012-08-31.
  3. ^ a b "IAU Minor Planet Center: (445473) 2010 VZ98" (last observation: 2015-10-12; arc: 17 years years). Retrieved 2015-11-11.
  4. ^ a b c Michael E. Brown. "How many dwarf planets are there in the outer solar system? (updates daily)". California Institute of Technology. Retrieved 2012-08-31.
  5. ^ a b "JPL Small-Body Database Browser: (2010 VZ98)" (last observation: 2013-11-04; arc: 2.98 years). Retrieved 2014-06-12.
  6. ^ de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (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.