type IIAB iron meteorite | high | 201 nanogram/gram | during meteor phase | 10 microgram/gram | it fragments because smaller pieces with less mass are more easily slowed by the atmosphere | H | crystalline iron-nickel alloy | size is between 3 micrometers and 3 millimeters | 9.9 microgram/gram | 2000 microgram/gram | low because it is tougher than stony meteorite | crater | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | | higher than that of average solar system material | 0.8 to 3 degrees C per million years | | based on the locale, region, or nearby town in which the fall occurred | 90 to 165 kilometers | greater than 50 mm | 0.20 % by weight | 1.1 microgram/gram | | 2.6 microgram/gram | 5.7 % of meteorite falls | 6.9 microgram/gram | during impact phase | | 3563 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 | 129 microgram/gram | 2.1 microgram/gram | kamacite, daubreelite | 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 | hexahedrite | | 6.15 % by weight | 28 microgram/gram | 43 | planet or asteroid much larger than 100 km in diameter | low because it has higher tensile strength than stony meteorite | power outages and failures in electrical equipment due to EMP (electromagnetic pulse) | 5.3 milligram/gram | | 58.3 microgram/gram | 173 microgram/gram | 6 milligram/gram | | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |