External links
- 2017 SV13 at the JPL Small-Body Database
 | This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by adding missing information. |
| Discovery | |
|---|---|
| Discovered by | Pan-STARRS 1 |
| Discovery site | Haleakala Obs. |
| Discovery date | 17 September 2017 (first observed only) |
| Designations | |
| 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 |
| 9.656 AU | |
| Eccentricity | 0.7919 |
| 30.09 yr (10,990 d) | |
| 46.490° | |
| 0° 1m 58.253s / day | |
| Inclination | 113.283° |
| 11.633° | |
| 343.213° | |
| Earth MOID | 1.0349 AU |
| Jupiter MOID | 2.8967 AU |
| Saturn MOID | 3.1974 AU |
| TJupiter | –1.119 |
| Physical characteristics | |
| 1 km (est.) | |
| 0.09 (assumed) | |
| 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. This unusual object measures approximately 1 kilometer (0.6 miles) in diameter.
| This article about a centaur (minor planet) or trans-Neptunian object is a stub. You can help Wikipedia by adding missing information. |