| Mayo Belwa | has image
 |  |
| is an instance of aubrite |  |
| is an instance of meteorite fall |  |
| has name Mayo Belwa |  |
| has fall date August 3, 1974 |  |
| has fall coordinates 8° 58' N., 12° 5' E. |  |
| has fall location Adamawa district of north-eastern Nigeria |  |
| has mass 4.85 kg |  |
| aubrite | has letter designation AUB |  |
| has characteristic mineral enstatite |  |
| has total mass of finds 1205 kg |  |
| has number of finds 9 |  |
| has minerology enstatite, forsterite, sodic plagioclase, metal, numerous sulfides |  |
| has petrology breccias of igneous lithologies |  |
| has likely origin melted and crystallized residues from partial melting |  |
| meteorite fall | has value higher because the fall was witnessed |  |
| has fall description what witnesses saw or what was recorded by instruments |  |
| has weathering negligible due to quick recovery of meteorite before corrosion begins |  |
| asteroidal achondrite | has origin asteroid |  |
| highly reduced meteorite | has oxidation state highly reduced with very little FeO |  |
| meteorite | has fall map which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |  |
| can have crater image |  |
| has original mass which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site |  |
| has composition often minerals not found on Earth |  |
| has relative abundance |  |
| has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
| has impact angle |  |
| has weather resistance which depends on its composition |  |
| has monetary value large if the fall was witnessed |  |
| often produce power outages and failures in electrical equipment due to EMP (electromagnetic pulse) |  |
| can be associated with crater |  |
| has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal |  |
| vaporizes completely if size is between 3 micrometers and 3 millimeters |  |
| can survive fall if size is larger than 3 mm and velocity is less than 24 km per second |  |
| can survive fall if it fragments because smaller pieces with less mass are more easily slowed by the atmosphere |  |
| has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid |  |
| has ablative mass loss directly proportional to initial velocity |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| has fragmentation probability during meteor phase which depends on composition |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| achondrite | has distinguishing feature no chondrules |  |
| igneous rock | has solidification mechanism |  |
| has solidification timescale |  |