| ALH 84001 | is an instance of ALH 84001 meteorite |  |
| is an instance of Antarctic meteorite |  |
| has name ALH 84001 |  |
| has fall location Allan Hills, Antarctica |  |
| has find date 1994 |  |
| has identification date 1993 |  |
| has mass 1.90 kg |  |
| has curatorial location MWG (JSC), SI |  |
| has SiO2 content 52.8 % by mass |  |
| has TiO2 content 0.20 % by mass |  |
| has Al2O3 content 1.23 % by mass |  |
| has Cr2O3 content 1.22 % by mass |  |
| has FeO content 17.4 % by mass |  |
| has MnO content 0.45 % by mass |  |
| has MgO content 24.6 % by mass |  |
| has CaO content 1.78 % by mass |  |
| has Na2O content 0.14 % by mass |  |
| has K2O content 0.02 % by mass |  |
| has P2O5 content 0.01 % by mass |  |
| has sulfur content 0.01 % by mass |  |
| ALH 84001 meteorite | has prototype ALH 84001 meteorite |  |
| martian meteorite | has origin Mars |  |
| orthopyroxenite | has composition orthopyroxene |  |
| meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
| has fall coordinates in degrees, minutes and seconds of lattitude and longitude |  |
| 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 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 |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| achondrite | has distinguishing feature no chondrules |  |
| plutonic rock | has solidification mechanism cooling in deep underground chambers |  |
| has solidification timescale very slow |  |
| gravitationally separated rock | has property formed by separation of molten rock in a gravity field |  |