The asteroid was discovered by ATLAS–MLO on 22 June 2019 and was observed four times with an observation arc of just 30 minutes, typical for ATLAS discoveries before they are followed up by other resources. With such a short observation arc, how far away the object is very uncertain until more data are available. Using these four observations, JPL's Scout listed the impact risk as modest, and calculated that the asteroid was about 160 meters in diameter and would pass about 36 LD from Earth. A fireball was however reported. When the Caribbean bolide report came in from the GOES-16weather satellite it was possible to link the ATLAS astrometry to it. Three additional precovery observations by Pan-STARRS 2 were then located and extended the observation arc to 2.3 hours. Using all seven observations, Scout then obtained a significantly better orbit determination with an impact rating of "elevated". The updated orbit shows that the asteroid was about 1.3 LD from Earth when ATLAS-MLO observed it, 12 hours before impact.
Visibility
The asteroid came to opposition 175 degrees from the Sun on 17 May 2019 when it had an apparent magnitude of 27. Such a faint apparent magnitude would require a 10 hour image to detect with the largest 8-meter class telescopes in the world. Pan-STARRS is a 1.8-meter class telescope and with 30 second images has a limiting apparent magnitude of around 22. ATLAS has a limiting apparent magnitude closer to 19. The asteroid did not become brighter than apparent magnitude 23 until 19 June when it was about 4 million km from Earth. The asteroid was detected by ATLAS when it was apparent magnitude 18.1.
Meteorites
This bolide was a probable meteorite fall into waters 4.8 km deep. NEXRADweather radar detected falling meteorites at 21:26:15 UT at 10.6 kmabove sea level. Signatures consistent with falling meteorites appear in a total of four radar sweeps. Meteorite falls with enough mass to generate green pixels on weather radar are very rare.
Origin
It could be an Alinda asteroid originating from the 3:1 mean-motion resonance with Jupiter. Even though 2019 MO has a geometric similarity to the June epsilon Ophiuchids and four other minor meteor showers, it could just as easily be a sporadic meteor that just looks similar by chance. 2019 MO is about 12° away from the concentration of June epsilon Ophiuchids orbits. The few other asteroids discovered before impacting are 2008 TC3, 2014 AA, and 2018 LA.
