| metal-rich meteorite | is a kind of differentiated meteorite  |  |
| has definition meteorite with metal content higher than that of average solar system material |  |
| has metal content higher than that of average solar system material |  |
| has nickel content always greater than 4 % |  |
| 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 composition often minerals not found on Earth |  |
| has relative abundance |  |
| has total mass of finds 485755 kg |  |
| has number of finds 1691 |  |
| has impact velocity when it hits the ground which is smaller than its velocity before it enters the atmosphere |  |
| has impact angle |  |
| has weather resistance which depends on its composition |  |
| 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 |  |
| has ablative mass loss depending on composition, more friable stony meteoroids loses more mass than iron meteoroid |  |
| has ablative mass loss directly proportional to initial velocity |  |
| can shatter during impact phase |  |
| can fragment during meteor phase |  |
| has fragmentation probability during meteor phase which depends on composition |  |
| igneous rock | has composition silicates (with very few exceptions) |  |
| has solidification mechanism |  |
| has solidification timescale |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |