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]
See also
- List of notable asteroids § Retrograde and highly inclined
- 2006 BZ8 – retrograde centaur, damocloid, and potential co-orbital with Saturn
- 2006 RJ2 – another retrograde centaur, damocloid, and potential co-orbital with Saturn
References
- ^ a b c d e "2017 SV13". Minor Planet Center. International Astronomical Union. Retrieved 8 August 2021.
- ^ a b c "JPL Small-Body Database Browser: (2017 SV13)" (2017-10-28 last obs.). Jet Propulsion Laboratory. Retrieved 8 August 2021.
- ^ a b c d 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.
External links
- 2017 SV13 at the JPL Small-Body Database
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