| Zagami | is an instance of basalt shergottite |  |
| has name Zagami |  |
| has fall location Katsina, Nigeria, Africa |  |
| has fall date 1962 |  |
| has mass 18.00 kg |  |
| has curatorial location dealers, New Mexico, Berlin, London, Paris |  |
| has SiO2 content 51.1 % by mass |  |
| has TiO2 content 0.78 % by mass |  |
| has Al2O3 content 6.10 % by mass |  |
| has Cr2O3 content 0.32 % by mass |  |
| has FeO content 18.4 % by mass |  |
| has MnO content 0.52 % by mass |  |
| has MgO content 11.0 % by mass |  |
| has CaO content 11.0 % by mass |  |
| has Na2O content 1.17 % by mass |  |
| has K2O content 0.14 % by mass |  |
| has P2O5 content 0.53 % by mass |  |
| has sulfur content 0.19 % by mass |  |
| basalt shergottite | has prototype Shergotty meteorite |  |
| shergottite | has letter designation AEUC |  |
| SNC meteorite | is an acronym for Shergottite, Nakhilite, Chassignite |  |
| volcanic rock | has solidification mechanism extrusion onto the surface of the planet or asteroid via a volcanic eruption |  |
| has solidification timescale very rapid |  |
| martian meteorite | has origin Mars |  |
| igneous rock | has composition silicates (with very few exceptions) |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| 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 |  |
| 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 |  |