2019 EU5 is an extreme trans-Neptunian object from the scattered disc on a highly eccentric orbit in the outermost region of the Solar System. It was discovered on 5 March 2019, by American astronomers Scott Sheppard, David Tholen, and Chad Trujillo at Mauna Kea Observatories in Hawaii, and announced on 17 December 2021.[1] It was 83.4 astronomical units from the Sun when it was discovered, making it one of the most distant known Solar System objects from the Sun as of December 2021[update].[1] It has been identified in precovery images from 6 January 2016.[2]
Discovery[1] | |
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Discovered by | S. S. Sheppard D. J. Tholen C. Trujillo |
Discovery site | Mauna Kea Obs. |
Discovery date | 5 March 2019 |
Designations | |
MPC designation | 2019 EU5 |
Minor planet category | TNO[2] · ESDO (detached)[3] · ETNO · distant[4] |
Orbital characteristics (barycentric)[5] | |
Epoch 21 January 2022 (JD 2459600.5) | |
Uncertainty parameter 4[2] | |
Observation arc | 5.03 yr (1,837 days) |
Earliest precovery date | 6 January 2016 |
Aphelion | 2,395 AU |
Perihelion | 46.759 AU |
Semi-major axis | 1,221 AU |
Eccentricity | 0.9617 |
Orbital period (sidereal) | 42,630 yr |
Mean anomaly | 359.331° |
Mean motion | 0° 0m 0.083s / day |
Inclination | 18.207° |
Longitude of ascending node | 109.227° |
Argument of perihelion | 109.204° |
Physical characteristics | |
Mean diameter | 220–160 km (est. 0.1–0.2)[6] |
Apparent magnitude | 25.6[1] |
Absolute magnitude (H) | 6.35±0.14[2][4] |
Trans-Neptunian objects | |
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TNO classes |
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Dwarf planets (moons) | |
Sednoids |
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