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== External links ==
== External links ==
* [http://neo.jpl.nasa.gov/cgi-bin/db?sstr=2002+VR128 Orbit simulation from NASA JPL site]
* [http://neo.jpl.nasa.gov/cgi-bin/db?sstr=2002+VR128 Orbit simulation from NASA JPL site]
* [http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=d&o=84719 Orbital details from the IAU Minor Planets Center]
* [https://web.archive.org/web/20160303180011/http://scully.cfa.harvard.edu/cgi-bin/returnprepeph.cgi?d=d&o=84719 Orbital details from the IAU Minor Planets Center]
* {{JPL small body|id=84719}}
* {{JPL small body|id=84719}}



Revision as of 05:25, 8 January 2018

(84719) 2002 VR128
Discovery[1]
Discovered byMichael E. Brown
Chadwick A. Trujillo
Discovery sitePalomar Observatory
Discovery date3 November 2002
Designations
(84719) 2002 VR128
TNO, plutino[2]
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 3
Observation arc9153 days (25.06 yr)
Aphelion49.650 AU (7.4275 Tm)
Perihelion28.999 AU (4.3382 Tm)
39.325 AU (5.8829 Tm)
Eccentricity0.26257
246.61 yr (90072.7 d)
73.453°
0° 0m 14.388s / day
Inclination14.040°
23.152°
287.87°
Earth MOID28.0112 AU (4.19042 Tm)
Jupiter MOID24.0604 AU (3.59938 Tm)
Physical characteristics
Dimensions448.5+42.1
−43.2
 km
[3]
0.052+0.027
−0.018
[3]
Temperature≈ 44 K
B−V = 0.94±0.03
V−R = 0.60±0.02[3]
5.58±0.37[3]
5.4[1]

(84719) 2002 VR128, also written (84719) 2002 VR128, is a trans-Neptunian object (TNO). It was discovered in 2002 by Michael Brown and Chad Trujillo. The object is a plutino, an object in 2:3 orbital resonance with Neptune.

Physical properties

The size of (84719) 2002 VR128 was measured by the Herschel Space Telescope to be 448.5+42.1
−43.2
 km
.[3] The surface of (84719) 2002 VR128 is red in the visible spectral range.[3]

References

  1. ^ a b c "JPL Small-Body Database Browser: 84719 (2002 VR128)" (2008-10-22 last obs). Retrieved 7 April 2016.
  2. ^ Marsden, Brian G. (2002-11-21). "MPEC 2002-W27 : 2002 MS4, 2002 QX47, 2002 VR128". IAU Minor Planet Center. Harvard-Smithsonian Center for Astrophysics. Retrieved 2012-05-14.
  3. ^ a b c d e f Mommert, Michael; Harris, A. W.; Kiss, C.; Pál, A.; Santos-Sanz, P.; Stansberry, J.; Delsanti, A.; Vilenius, E.; Müller, T. G.; Peixinho, N.; Lellouch, E.; Szalai, N.; Henry, F.; Duffard, R.; Fornasier, S.; Hartogh, P.; Mueller, M.; Ortiz, J. L.; Protopapa, S.; Rengel, M.; Thirouin, A. (May 2012). "TNOs are cool: A survey of the trans-Neptunian region—V. Physical characterization of 18 Plutinos using Herschel-PACS observations". Astronomy & Astrophysics. 541: A93. arXiv:1202.3657. Bibcode:2012A&A...541A..93M. doi:10.1051/0004-6361/201118562.