Orbital diagrams of 2012 VP113 with Pluto and the outer planets as of 2017
Discovery[1][2]
Discovered by
S. S. Sheppard
C. Trujillo
Discovery site
Cerro Tololo Obs.
Discovery date
5 November 2012 (announced: 26 March 2014)
Designations
MPC designation
2012 VP113
Alternative designations
"Biden" (nickname)
Minor planet category
TNO[3]
sednoid[4]
Orbital characteristics[3]
Epoch 2022 Aug 09 (JD 2459800.5)
Uncertainty parameter 4
Observation arc
8.29 yr (3,028 d)
Aphelion
462±1 AU
Perihelion
80.522 AU[5]
80.47±0.03 AU
Semi-major axis
271.5±0.6 AU
Eccentricity
0.7036±0.0007
Orbital period (sidereal)
4473±14 yr
4240 yr (barycentric)[6]
Mean anomaly
3.50°±0.01°
Mean motion
0° 0m 0.792s / day
Inclination
24.0563°±0.006°
Longitude of ascending node
90.787°
Time of perihelion
≈ 28 September 1979[5]
Argument of perihelion
293.8°
Physical characteristics
Mean diameter
574 km?[7] 300–1000 km[8]
Geometric albedo
0.09 (assumed)[4][9]
0.15[10]
Spectral type
moderately red
V−R = 0.52[10]
B−V = 0.92
Apparent magnitude
23.34[11]
Absolute magnitude (H)
4.1[3]
2012 VP113, also known by its nickname "Biden", is a trans-Neptunian object of the sednoid population, located in the outermost reaches of the Solar System. It was first observed on 5 November 2012 by American astronomers Scott Sheppard and Chad Trujillo at the Cerro Tololo Inter-American Observatory in Chile.[1][2] The discovery was announced on 26 March 2014.[10][12] The object probably measures somewhere between 300 and 1000 km in diameter, possibly large enough to be a dwarf planet.
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2012VP113, also known by its nickname "Biden", is a trans-Neptunian object of the sednoid population, located in the outermost reaches of the Solar System...
"younger" than the Oort cloud. However, only Sedna and two other sednoids (2012VP113 and 541132 Leleākūhonua) bear those irregularities; for 2000 OO67 and...
orbital class of objects named after itself, the sednoids, which include 2012VP113, Leleākūhonua, and 2021 RR205, all celestial bodies with extremely elongated...
orbits like Sedna's. In 2014, astronomers announced the discovery of 2012VP113, a large object with a Sedna-like 4,200-year orbit and a perihelion of...
only three objects that are known from this population: 90377 Sedna, 2012VP113, and 541132 Leleākūhonua (2015 TG387). All three have perihelia greater...
the Sun as of 2022 The orbits of the three known sednoids: 90377 Sedna, 2012VP113, and Leleākūhonua Eris and its moon Dysnomia as viewed with the Hubble...
of exoplanets discovered in 2011 (178) List of exoplanets discovered in 2012 (149) List of exoplanets discovered in 2013 (151) List of exoplanets discovered...
"The Dwarf Planets". Retrieved 20 January 2008. Stern, Alan (24 August 2012). "The Kuiper Belt at 20: Paradigm Changes in Our Knowledge of the Solar...
Mons ("Mount Sharp"), Mars (as viewed by the rover Curiosity on 6 August 2012). Maat Mons, Venus (radar imaging plus altimetry, 10x vertical exaggeration)...
Central Scranton Expressway in 2021 The discovery of the minor planet 2012VP113 was announced in 2014. Because its name includes "VP", which often stands...
are termed sednoids. As of 2023, there are four known sednoids: Sedna, 2012VP113, Leleākūhonua, and 2021 RR205. These objects exhibit a highly statistically...
Retrieved January 12, 2012. Hughes, David W. (2007). "Finding Asteroids In Space". BBC. Archived from the original on March 10, 2012. Retrieved April 20...
Retrieved 10 May 2012. "Tours of Model Solar Systems". University of Illinois. Archived from the original on 12 April 2011. Retrieved 10 May 2012. "Luleå är...
Sednoids, detached objects with a perihelion greater than 75 AU (Sedna, 2012VP113, and Leleākūhonua). The Oort cloud, a hypothetical population thought...
(December 2012). "Density of asteroids". Planetary and Space Science. 73 (1): 98–118. arXiv:1203.4336. Bibcode:2012P&SS...73...98C. doi:10.1016/j.pss.2012.03...
with the other known extreme trans-Neptunian objects such as Sedna and 2012VP113, i.e. its longitude of perihelion differs by 180° from other objects....