Chinga | high | 1.5 nanogram/gram | during meteor phase | 22 microgram/gram | it fragments because smaller pieces with less mass are more easily slowed by the atmosphere | type IVB iron meteorite | D | crystalline iron-nickel alloy | size is between 3 micrometers and 3 millimeters | 1.1 microgram/gram | 40 microgram/gram | low because it is tougher than stony meteorite | crater | Tanna Tuva, Tuvinskaya, Russia | recorded by eyewitness or inferred from dating methods | | higher than that of average solar system material | 30 to 260 degrees C per million years | | Chinga | 11 to 30 kilometers | also called Widmanstatten bandwidth | 0.03 % by weight | 0.15 microgram/gram | | 12 microgram/gram | 5.7 % of meteorite falls | 27 microgram/gram | during impact phase | | 60487 kg | when it hits the ground which is smaller than its velocity before it enters the atmosphere | Latitude 51 degrees 3 minutes 30 seconds North, Longitude 94 degrees 0 degrees 24 seconds East | 12 microgram/gram | 3 microgram/gram | kamacite, taenite | large if the fall was witnessed | greater than 80 kg | | 1913 | 7.1 % by weight | 87.7 microgram/gram |
 | planet or asteroid much larger than 100 km in diameter | 11 | low because it has higher tensile strength than stony meteorite | 16.38% Ni, 0.181 ppm Ga, 0.082 ppm Ge, 3.6 ppm Ir | power outages and failures in electrical equipment due to EMP (electromagnetic pulse) | 7.4 milligram/gram | | 0.221 microgram/gram | 0.0526 microgram/gram | 1 milligram/gram | | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |