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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]

2017 FO161
Orbital diagram of 2017 FO161
Discovery[1][2]
Discovered byCTIO
Discovery siteCTIO
Discovery date23 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 arc7.04 yr (2,571 d)
Aphelion85.459 AU
Perihelion34.069 AU
Semi-major axis
59.764 AU
Eccentricity0.42994
Orbital period (sidereal)
462.03 yr (168,756 d)
Mean anomaly
240.958°
Mean motion
0° 0m 7.68s / day
Inclination54.350°
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]

    See also



    References


    1. "2017 FO161". Minor Planet Center. Retrieved 6 March 2019.
    2. Trujillo, C.; Sheppard, S. S. (April 2018). "2017 FO161". Minor Planet Electronic Circulars. 2018-G10. Bibcode:2018MPEC....G...10T. ISSN 1523-6714.
    3. "JPL Small-Body Database Browser: (2017 FO161)" (2018-03-12 last obs.). Jet Propulsion Laboratory. Retrieved 6 March 2019.
    4. Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 3 March 2021.




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