2015 FJ345
| Discovery | |
|---|---|
| Discovered by | Mauna Kea Obs. |
| Discovery site | Mauna Kea Obs. (first observed only) |
| Discovery date | 17 March 2015 |
| Designations | |
| 2015 FJ345 | |
| Orbital characteristics | |
| Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter
| |
| Observation arc | 1.13 yr (413 d) |
| Aphelion | 74.837 AU |
| Perihelion | 50.785 AU |
| 62.811 AU | |
| Eccentricity | 0.1915 |
| 497.81 yr (181,824 d) | |
| 58.879° | |
| 0° 0m 7.2s / day | |
| Inclination | 34.973° |
| 37.881° | |
| 77.511° | |
| Physical characteristics | |
| |
| |
| 25.74 | |
| 7.9 | |
2015 FJ345 is a trans-Neptunian object and detached object, located in the scattered disc, the outermost region of the Solar System. It was first observed on 17 March 2015, by a team led by American astronomer Scott Sheppard at the Mauna Kea Observatories, in Hawaii, United States. With its perihelion of almost 51 AU, it belongs to a small and poorly understood group of very distant objects with moderate eccentricities. The object is not a dwarf planet candidate as it only measures approximately 120 kilometers (75 miles) in diameter.