| Nakhla | is an instance of nakhilite |  |
| has name Nakhla |  |
| has fall location Alexandria, Egypt |  |
| has fall date 1911 |  |
| has mass 10.00 kg |  |
| has curatorial location Cairo, London, SI, Berlin, Vienna, Paris, dealers |  |
| has SiO2 content 48.6 % by mass |  |
| has TiO2 content 0.33 % by mass |  |
| has Al2O3 content 1.60 % by mass |  |
| has Cr2O3 content 0.28 % by mass |  |
| has FeO content 21.3 % by mass |  |
| has MnO content 0.50 % by mass |  |
| has MgO content 12.0 % by mass |  |
| has CaO content 15.3 % by mass |  |
| has Na2O content 0.45 % by mass |  |
| has K2O content 0.13 % by mass |  |
| has P2O5 content 0.11 % by mass |  |
| has sulfur content 0.04 % by mass |  |
| nakhilite | has prototype Nakhla meteorite |  |
| has letter designation ACANOM |  |
| has characteristic mineral diopside-olivine |  |
| has composition cumulus-augite-bearing proxenite |  |
| SNC meteorite | is an acronym for Shergottite, Nakhilite, Chassignite |  |
| martian meteorite | has origin Mars |  |
| plutonic rock | has solidification mechanism cooling in deep underground chambers |  |
| has solidification timescale very slow |  |
| fractional crystallized rock | has genesis fractional crystallization |  |
| gravitationally separated rock | has property formed by separation of molten rock in a gravity field |  |
| achondrite | has relative abundance 7.1 % of meteorite falls |  |
| has distinguishing feature no chondrules |  |
| has number of finds 70 |  |
| has total mass of finds 1606 kg |  |
| rock | has part mineral |  |
| has texture |  |
| meteorite | 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 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 |  |
| 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 |  |
| stony meteorite | has weather resistance low |  |
| has fragmentation probability high because it is more friable than iron meteorite |  |
| has ablative mass loss high because it is more friable than iron meteorite |  |