Chassigny | low | 1.37 % by mass | 0.53 % by mass | during meteor phase | it fragments because smaller pieces with less mass are more easily slowed by the atmosphere | chassignite | no chondrules | size is between 3 micrometers and 3 millimeters | 0.11 % by mass | 27.2 % by mass | high because it is more friable than iron meteorite | crater | Haute-Marne, France | 1815 | | 0.04 % by mass | cooling in deep underground chambers | Chassigny | 0.04 % by mass | 0.49 % by mass | fractional crystallization | ACANOM | 7.1 % of meteorite falls | during impact phase | | Paris, Vienna, London | Chassigny 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 | 37.2 % by mass | olivine | 31.9 % by mass | olivine | large if the fall was witnessed | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | | 0.12 % by mass | 0.04 % by mass | formed by separation of molten rock in a gravity field | 4.00 kg | 70 | Mars | high because it is more friable than iron meteorite | power outages and failures in electrical equipment due to EMP (electromagnetic pulse) | very slow | | Shergottite, Nakhilite, Chassignite | 0.69 % by mass | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |