Discovery[1][2] | |
---|---|
Discovered by | Mount Lemmon Srvy. |
Discovery site | Mount Lemmon Obs. (first observed only) |
Discovery date | 1 November 2005 |
Designations | |
2005 VX3 | |
TNO[3] · damocloid[4] unusual[5] · distant[1] | |
Orbital characteristics[3] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 4 | |
Observation arc | 81 days |
Aphelion | 1825.61 AU |
Perihelion | 4.1058 AU |
914.86 AU | |
Eccentricity | 0.9955 |
27,672 yr | |
0.1730° | |
0° 0m 0s / day | |
Inclination | 112.22° |
255.35° | |
196.37° | |
Jupiter MOID | 0.8884 AU |
TJupiter | −0.9430 |
Physical characteristics | |
7 km (est.)[4] | |
0.09 (assumed)[4] | |
14.1[1][3] | |
2005 VX3 is trans-Neptunian object and retrograde damocloid on a highly eccentric, cometary-like orbit. It was first observed on 1 November 2005, by astronomers with the Mount Lemmon Survey at the Mount Lemmon Observatory in Arizona, United States. The unusual object measures approximately 7 kilometers (4 miles) in diameter.[4] It has the 3rd largest known heliocentric semi-major axis and aphelion.[6] Additionally its perihelion lies within the orbit of Jupiter, which means it also has the largest orbital eccentricity of any known minor planet.
MPC-object
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