(20161) 1996 TR66 is a trans-Neptunian object orbiting beyond Pluto in the Kuiper belt of the outermost Solar System, approximately 139 kilometers (86 miles) in diameter. It was discovered on 8 October 1996, by astronomers David Jewitt, Chad Trujillo, Jane Luu, and Jun Chen at the Mauna Kea Observatory, Hawaii, in the United States.[4] It was the first discovery of a twotino.
Discovery[1] | |
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Discovered by | D. C. Jewitt C. Trujillo J. X. Luu J. Chen |
Discovery site | Mauna Kea Obs. |
Discovery date | 8 October 1996 |
Designations | |
MPC designation | (20161) 1996 TR66 |
Minor planet category | TNO[1] · twotino[2][3] distant[4] |
Orbital characteristics[1] | |
Epoch 4 September 2017 (JD 2458000.5) | |
Uncertainty parameter 4 | |
Observation arc | 12.04 yr (4,398 days) |
Aphelion | 66.612 AU |
Perihelion | 28.630 AU |
Semi-major axis | 47.621 AU |
Eccentricity | 0.3988 |
Orbital period (sidereal) | 328.63 yr (120,032 d) |
Mean anomaly | 55.593° |
Mean motion | 0° 0m 10.8s / day |
Inclination | 12.436° |
Longitude of ascending node | 343.11° |
Argument of perihelion | 308.70° |
Physical characteristics | |
Dimensions | 139 km[5] |
Absolute magnitude (H) | 7.5[1] |
It orbits the Sun at a distance of 28.6–66.6 AU once every 328 years and 8 months (120,032 days). Its orbit has an eccentricity of 0.40 and an inclination of 12° with respect to the ecliptic.[1] Near perihelion, it comes closer to the Sun than Neptune does (29.7 AU). It has a semi-major axis (average distance from the Sun) near the edge of the classical belt.
1996 TR66 was the first twotino discovered. Twotinos stay in a 1:2 orbital resonance with Neptune, which means that for every one orbit a twotino makes, Neptune orbits two times. Both the Minor Planet Center and the Deep Ecliptic Survey list this trans-Neptunian object as a twotino.[2][3]
This minor planet was numbered by the Minor Planet Center on 9 January 2001.[6] As of 2018, it has not been named.[4]
using 22 observations
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