| Monument Draw | has image
 |  |
| is an instance of acapulcoite |  |
| is an instance of meteorite find |  |
| is an instance of Antarctic meteorite |  |
| has name Monument Draw |  |
| has find date 1985 |  |
| has fall coordinates 32° 30.2' N., 102° 44.6' W. |  |
| has fall location 18 miles NW of Andrews, Texas |  |
| has mass 0.5245 kg |  |
| acapulcoite | has composition chondritic abundances of plagioclase and troilite; |  |
| has texture medium grained |  |
| has prototype Acapulco meteorite |  |
| meteorite find | has value lower because the fall was not witnessed |  |
| has weathering can be severe due to long exposure time to environmental corrosion agents |  |
| Antarctic meteorite | has identification date |  |
| primitive achondrite | has minerology olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase |  |
| has petrology fine- to coarse-grained equigranular |  |
| has likely origin ultrametamorphism, partial melting with some melt migration |  |
| meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
| 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 relative abundance |  |
| has total mass of finds 485755 kg |  |
| has number of finds 1691 |  |
| 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 |  |
| achondrite | has distinguishing feature no chondrules |  |
| undifferentiated meteorite | has peak temperature less than 950 degree Celsius during its entire history since solidification |  |
| has parent body asteroid smaller than 100 km in diameter |  |
| has age oldest and most primitive rock in solar system |  |
| rock | has part mineral |  |
| has genesis |  |
| conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |