Discovery[1][2] | |
---|---|
Discovered by | Dark Energy Survey |
Discovery site | Cerro Tololo Obs. |
Discovery date | 17 January 2015 (first observed only) |
Designations | |
2015 BP519 | |
Caju (nickname)[a] | |
TNO[3] · ESDO[4] · ETNO distant[2] | |
Orbital characteristics[3] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 5 | |
Observation arc | 3.22 yr (1,176 d) |
Aphelion | 820 AU |
Perihelion | 35.2 AU |
428.03 AU | |
Eccentricity | 0.9178 |
8856 yr (3,234,488 d) | |
358.39° | |
0° 0m 0.36s / day | |
Inclination | 54.125° |
135.11° | |
≈ 7 September 2058[5] ±1 month | |
348.37° | |
Physical characteristics | |
524 km (est.)[6] 584 km (est.)[4] | |
0.08 (assumed)[6] 0.09 (assumed)[4] | |
21.5 | |
4.4[2][3] | |
2015 BP519, nicknamed Caju,[a] is an extreme trans-Neptunian object from the scattered disc on a highly eccentric and inclined orbit in the outermost region of the Solar System.[7] It was first observed on 17 January 2015, by astronomers with the Dark Energy Survey at Cerro Tololo Observatory (W84) in Chile.[1][2] It has been described as an extended scattered disc object (ESDO),[4] and fits into the group of extreme objects that led to the prediction of Planet Nine, and has the highest orbital inclination of any of these objects.[a]
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