Discovery[1] | |
---|---|
Discovered by | Pan-STARRS 1 |
Discovery site | Haleakala Obs. |
Discovery date | 1 November 2010 |
Designations | |
(523645) 2010 VK201 | |
2010 VK201 | |
TNO[2][3] · KBO (hot)[4] · distant[1] | |
Orbital characteristics[2] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 3 | |
Observation arc | 7.13 yr (2,606 d) |
Aphelion | 48.065 AU |
Perihelion | 37.973 AU |
43.019 AU | |
Eccentricity | 0.1173 |
282.16 yr (103,060 d) | |
170.71° | |
0° 0m 12.6s / day | |
Inclination | 28.845° |
156.40° | |
88.906° | |
Physical characteristics | |
443 km (est.)[4] 501 km (est.)[5] 505 km (calc.)[6] | |
7.59±0.05 h[7][8] | |
0.10 (assumed)[6] | |
C (assumed)[6] | |
4.40±0.07 (SR)[7] 4.6[6] 5.0[1][2][5] | |
(523645) 2010 VK201 (provisional designation 2010 VK201) is a trans-Neptunian object and member of the classical Kuiper belt, approximately 500 kilometers (310 miles) in diameter. It was discovered on 1 November 2010, by the Pan-STARRS 1 survey at Haleakala Observatory, Hawaii, United States.[1] It has a rotation period of 7.6 hours.[6] It was numbered in September 2018 and remains unnamed.
MPC-object
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).MPC-TNO-list
was invoked but never defined (see the help page).johnstonsarchive-TNO-list
was invoked but never defined (see the help page).Brown-dplist
was invoked but never defined (see the help page).lcdb
was invoked but never defined (see the help page).Benecchi-2013
was invoked but never defined (see the help page).Ferret
was invoked but never defined (see the help page).