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 |  |