2017 SV₁₃

2017 SV₁₃
Discovery
Discovered by	Pan-STARRS 1
Discovery site	Haleakala Obs.
Discovery date	17 September 2017; (first observed only)
Designations
Minor planet category	centaur · damocloid; unusual · distant
Orbital characteristics
	Epoch 1 July 2021 (JD 2459396.5)
	Uncertainty parameter 6
Observation arc	42 days
Aphelion	17.302 AU
Perihelion	2.010 AU
Semi-major axis	9.656 AU
Eccentricity	0.7919
Orbital period (sidereal)	30.09 yr (10,990 d)
Mean anomaly	46.490°
Mean motion	0° 1m 58.253s / day
Inclination	113.283°
Longitude of ascending node	11.633°
Argument of perihelion	343.213°
Earth MOID	1.0349 AU
Jupiter MOID	2.8967 AU
Saturn MOID	3.1974 AU
TJupiter	–1.119
Physical characteristics
Mean diameter	1 km (est.)
Geometric albedo	0.09 (assumed)
Absolute magnitude (H)	18.2

2017 SV₁₃ is a centaur and damocloid on a retrograde and highly eccentric orbit from the outer region of the Solar System. It was first observed on 17 September 2017 by the Pan-STARRS survey at Haleakala Observatory in Hawaii, United States.^[1] This unusual object measures approximately 1 kilometer (0.6 miles) in diameter.^[3]

References

1 2 3 4 5 "2017 SV13". Minor Planet Center. International Astronomical Union. Retrieved 8 August 2021.
1 2 3 "JPL Small-Body Database Browser: (2017 SV13)" (2017-10-28 last obs.). Jet Propulsion Laboratory. Retrieved 8 August 2021.
1 2 3 4 Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 8 August 2021.
↑ "List Of Other Unusual Objects". Minor Planet Center. International Astronomical Union. 8 August 2021. Retrieved 8 August 2021.