2015 ME131

2015 ME131 (also written 2015 ME131) is 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. Because it has a short observation arc of 1.8 days, and has not been seen since 2015, it has an orbit that is only roughly calculated. 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]

2015 ME131
Discovery[1][2]
Discovery sitePan-STARRS at the Haleakala Observatory, Hawaii
Discovery dateJune 23, 2015
Designations
2015 ME131
[1][2][3]
Orbital characteristics[3]
Epoch 2015-Jun-24.0 (JD 2457197.5)
Uncertainty parameter 9
Observation arc1.8 days[4]
Aphelion0.97±0.16 AU (Q)
Perihelion0.64±0.24 AU (q)
0.81±0.13 AU (a)
Eccentricity0.2 ? (e)
0.72±0.18 years
193°±34° (M)
Inclination30°±15° (i)
315°±12° (Ω)
162°±23° (ω)
Earth MOID0.05 AU (7,500,000 km) ?
Jupiter MOID4.1 AU (610,000,000 km) ?
Physical characteristics
Mean diameter
400 m[2]
500 m[4]
19.5[3]

    This asteroid is in both the Risk list[2] and the Priority List of the European Space Agency (ESA) - Space Situational Awareness (SSA). This asteroid is 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 has 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


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