| Discovery [1] | |
|---|---|
| Discovered by | D. C. Jewitt C. Trujillo J. X. Luu J. Chen |
| Discovery site | Mauna Kea Obs. |
| Discovery date | 8 October 1996 |
| Designations | |
| (20161) 1996 TR66 | |
| 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 |
| 47.621 AU | |
| Eccentricity | 0.3988 |
| 328.63 yr (120,032 d) | |
| 55.593° | |
| 0° 0m 10.8s / day | |
| Inclination | 12.436° |
| 343.11° | |
| 308.70° | |
| Physical characteristics | |
| Dimensions | 139 km [5] |
| 7.5 [1] | |
(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.
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 2025, it has not been named. [4]
using 22 observations