2017 VR12
| Discovery | |
|---|---|
| Discovered by | Pan-STARRS 1 | 
| Discovery site | Haleakala Obs. | 
| Discovery date | 10 November 2017 (first observed only) | 
| Designations | |
| 2017 VR12 | |
| NEO · PHA Apollo · Amor | |
| Orbital characteristics | |
| Epoch 23 March 2018 (JD 2458200.5) | |
| Uncertainty parameter 3 | |
| Observation arc | 118 days | 
| Aphelion | 1.7389 AU | 
| Perihelion | 1.0004 AU | 
| 1.3697 AU | |
| Eccentricity | 0.2696 | 
| 1.60 yr (585.50 d) | |
| 8.8927° | |
| 0° 36m 53.64s / day | |
| Inclination | 9.2247° | 
| 347.32° | |
| 180.74° | |
| Earth MOID | 0.0077 AU (3.0 LD) | 
| Physical characteristics | |
| Dimensions | 160 m × 100 m | 
| 160 m | |
| 1.4 h 1.5 h | |
| V | |
| 20.6 | |
2017 VR12 is a sub-kilometer asteroid with a somewhat elongated and angular shape, approximately 160 meters (500 feet) in diameter. It is classified as near-Earth object and potentially hazardous asteroid of the Apollo or Amor group. The V-type asteroid has a rotation period of approximately 1.5 hours. It was first observed on 10 November 2017 by the 60-inch Pan-STARRS 1 telescope at Haleakala Observatory in Hawaii.