diogenite | low | orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica | during meteor phase | it fragments because smaller pieces with less mass are more easily slowed by the atmosphere | no chondrules | size is between 3 micrometers and 3 millimeters | high because it is more friable than iron meteorite | crater | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | cumulates, crystallized melts, impact mixing | based on the locale, region, or nearby town in which the fall occurred | ADIO | 7.1 % of meteorite falls | during impact phase | | 68 kg | when it hits the ground which is smaller than its velocity before it enters the atmosphere | in degrees, minutes and seconds of lattitude and longitude | hyperstene | silicates (with very few exceptions) | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | large if the fall was witnessed | plutonic cumulate | 8 | 4 Vesta | high because it is more friable than iron meteorite | power outages and failures in electrical equipment due to EMP (electromagnetic pulse) | Howardite, Eucrite, Diogenite | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity | coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated |
nakhilite | low | | during meteor phase | it fragments because smaller pieces with less mass are more easily slowed by the atmosphere | no chondrules | size is between 3 micrometers and 3 millimeters | high because it is more friable than iron meteorite | crater | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | | based on the locale, region, or nearby town in which the fall occurred | ACANOM | 7.1 % of meteorite falls | during impact phase | Nakhla meteorite | 1606 kg | when it hits the ground which is smaller than its velocity before it enters the atmosphere | in degrees, minutes and seconds of lattitude and longitude | diopside-olivine | cumulus-augite-bearing proxenite | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | large if the fall was witnessed | clinopyroxenite | 70 | Mars | high because it is more friable than iron meteorite | power outages and failures in electrical equipment due to EMP (electromagnetic pulse) | Shergottite, Nakhilite, Chassignite | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity | |