2015 ME131
| Discovery[1][2] | |
|---|---|
| Discovery site | Pan-STARRS at the Haleakala Observatory, Hawaii |
| Discovery date | June 23, 2015 |
| Designations | |
MPC designation | 2015 ME131 |
| 2020 RX8 | |
Minor planet category | [1][2][3] |
| Orbital characteristics[3] | |
| Epoch 2020-Dec-17 (JD 2459200.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 5.3 years[4] |
| Aphelion | 0.98964 AU (Q) |
| Perihelion | 0.64282 AU (q) |
| 0.81623 AU (a) | |
| Eccentricity | 0.21245 (e) |
| 0.74 years | |
| 358.69° (M) | |
| Inclination | 33.645° (i) |
| 317.78° (Ω) | |
| 156.86° (ω) | |
| Earth MOID | 0.0458 AU (6,850,000 km) |
| Jupiter MOID | 4.01 AU (600,000,000 km) |
| Physical characteristics | |
Mean diameter | 400 m[2] 500 m[4] |
Absolute magnitude (H) | 19.5[3] |
2015 ME131 (also written 2015 ME131) was a lost asteroid[5] and a Near-Earth object (NEO). It is an Atira asteroid, which is by far the smallest group of near-Earth objects. This makes it an interior-Earth object (IEO),[2] meaning that it has an orbit entirely confined within Earth's orbit. It was recovered on September 15, 2020 as 2020 RX8 which has extended the observation arc from 1.8 days to 5 years.[3] It was removed from the Sentry Risk Table on February 15, 2021 after the two orbits were linked together. It was first observed on June 23, 2015, when the asteroid was more than 1 AU from Earth[1] and had a solar elongation of 68 degrees.[6]
This asteroid was in both the Risk list[2] and the Priority List of the European Space Agency (ESA) - Space Situational Awareness (SSA). This asteroid was also in the Sentry list[7] of the Jet Propulsion Laboratory (JPL) - Center for Near Earth Object Studies (CNEOS). According to the Sentry List, of the possible close encounters with Earth in the foreseeable future, an encounter on August 18, 2020 had the highest Palermo Technical Impact Hazard Scale value.[4]
According to the Near Earth Objects Dynamic Site (NEODyS), of the possible close encounters with Earth in the foreseeable future, an encounter on August 10, 2025 is the most likely.[8] This encounter has a minimum possible distance of zero, meaning that an impact onto Earth is possible.
See also[]
References[]
- ^ a b c "IAU Minor Planet Center 2015 ME131". International Astronomical Union. Retrieved 3 August 2020.
- ^ a b c d e "ESA space situational awareness 2015ME131". European Space Agency. Retrieved 3 August 2020.
- ^ a b c d "JPL Small-Body Database Browser (2015 ME131)". Jet Propulsion Laboratory. Retrieved 3 August 2020.
- ^ a b c "Sentry: Earth Impact Monitoring - Object Details 2015 ME131". Jet Propulsion Laboratory. Retrieved 3 August 2020.
- ^ "NEODyS-2 - Near Earth Objects - Dynamic Site - Risk List". SpaceDys. Retrieved 3 August 2020.
- ^ "JPL HORIZONS Web-Interface (2015 ME131)". Jet Propulsion Laboratory. Retrieved 3 August 2020.
- ^ "Sentry: Earth Impact Monitoring - Impact Risk Data". Jet Propulsion Laboratory. Retrieved 3 August 2020.
- ^ "NEODyS-2 - Near Earth Objects - Dynamic Site - 2015ME131 - Close Approaches". SpaceDys. Retrieved 4 August 2020.
External links[]
- 2015 ME131 at NeoDyS-2, Near Earth Objects—Dynamic Site
- Ephemeris · Obs prediction · Orbital info · MOID · Proper elements · Obs info · Close · Physical info · NEOCC
- 2015 ME131 at ESA–space situational awareness
- 2015 ME131 at the JPL Small-Body Database
 | This near-Earth asteroid-related article is a stub. You can help Wikipedia by . |
- Atira asteroids
- Minor planet object articles (unnumbered)
- Discoveries by Pan-STARRS
- Near-Earth objects removed from the Sentry Risk Table
- Astronomical objects discovered in 2015
- Near-Earth asteroid stubs