2017 FO161 is a large trans-Neptunian object from the scattered disc located in the outermost region of the Solar System. It is estimated to measure approximately 600 kilometers (370 mi) in diameter and currently orbits at a distance of about 78.5 AU from the Sun.[1][3][4] The object was first observed by American astronomers Chad Trujillo and Scott Sheppard using the 4-meter Víctor M. Blanco Telescope at the Cerro Tololo Inter-American Observatory in Chile on 23 March 2017.[2] Precovery observations were made by the Pan-STARRS-1 survey at Haleakalā Observatory and by the Dark Energy Survey with DECam, dating back as far as March 2012 and January 2016, respectively.[1]
![]() Orbital diagram of 2017 FO161 | |
Discovery[1][2] | |
---|---|
Discovered by | CTIO |
Discovery site | CTIO |
Discovery date | 23 March 2017 (first observed only) |
Designations | |
MPC designation | 2017 FO161 |
Minor planet category | TNO[3] · SDO[4] distant[1] |
Orbital characteristics[3] | |
Epoch 31 May 2020 (JD 2459000.5) | |
Uncertainty parameter 4 | |
Observation arc | 7.04 yr (2,571 d) |
Aphelion | 85.459 AU |
Perihelion | 34.069 AU |
Semi-major axis | 59.764 AU |
Eccentricity | 0.42994 |
Orbital period (sidereal) | 462.03 yr (168,756 d) |
Mean anomaly | 240.958° |
Mean motion | 0° 0m 7.68s / day |
Inclination | 54.350° |
Longitude of ascending node | 164.985° |
Argument of perihelion | 151.017° |
Physical characteristics | |
Mean diameter | 612 km (est. at 0.09)[4] |
Geometric albedo | 0.09 (est.)[4] |
Absolute magnitude (H) | 4.3[3] |
Trans-Neptunian objects | |
---|---|
TNO classes |
|
Dwarf planets (moons) | |
Sednoids |
Small Solar System bodies | |||||||
---|---|---|---|---|---|---|---|
Minor planets |
| ||||||
Comets |
| ||||||
Other |
|
![]() | This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by expanding it. |