| type IID iron meteorite | is a kind of magmatic iron meteorite |  |
| is a kind of Om octahedrite |  |
| has composition kamacite, taenite |  |
has formation cooling rate 5 degrees C per million years  |  |
parent body radius 70 kilometers  |  |
| has total mass of finds 1166 kg |  |
| has number of finds 11 |  |
has nickel content 11.2 % by weight  |  |
has gallium content 76.2 microgram/gram  |  |
has germanium content 87 microgram/gram  |  |
has iridium content 9.9 microgram/gram  |  |
has phosphor content 9.8 milligram/gram  |  |
has chromium content 31 microgram/gram  |  |
has cobalt content 4.7 milligram/gram  |  |
has copper content 280 microgram/gram  |  |
has molydbenum content 9.4 microgram/gram  |  |
has tungsten content 2.4 microgram/gram  |  |
has palladium content 5.3 microgram/gram  |  |
has gold content 1.1 microgram/gram  |  |
has arsenic content 10 microgram/gram  |  |
has antimony content 220 nanogram/gram  |  |
| Om octahedrite | has structural class Om |  |
| has crystal size 0.5 to 1.3 mm (medium) |  |
| iron meteorite | has relative abundance 5.7 % of meteorite falls |  |
| has weather resistance high |  |
| has fragmentation probability low because it is tougher than stony meteorite |  |
| has ablative mass loss low because it has higher tensile strength than stony meteorite |  |
| metal-rich meteorite | has metal content higher than that of average solar system material |  |
| structural iron meteorite | has distinguishing feature crystalline iron-nickel alloy |  |
| differentiated meteorite | has origin planet or asteroid much larger than 100 km in diameter |  |
| meteorite | has fall date recorded by eyewitness or inferred from dating methods |  |
| has fall location strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity |  |
| 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 monetary value large if the fall was witnessed |  |
| has name based on the locale, region, or nearby town in which the fall occurred |  |
| 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 |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| igneous rock | has solidification mechanism |  |
| has solidification timescale |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |