| ungrouped carbonaceous chondrite | is a kind of carbonaceous chondrite |  |
| carbonaceous chondrite | has relative abundance 8 % of meteorite falls |  |
| has total mass of finds 2577 kg |  |
| has number of finds 36 |  |
| has distinguishing feature elemental carbon |  |
| has abundance rare relative to other chondrite types |  |
| chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism |  |
| has part chondrule as a distinguishing feature -has URL: http://www.arachnaut.org/meteor/chondrules.html |  |
| has homogeneity of olivine and low Ca pyroxene definition goes here |  |
| has structural state of low Ca pyroxene definition goes here |  |
| has part feldspar usually plagioclase tectosilicate |  |
| has chondrule glass type |  |
| has part metal maximum bulk in weight % |  |
| has part mean Ni content of sulfides in weight % |  |
| has part matrix fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents |  |
| has part chondrule small sphere of about 1 mm diameter of formerly melted minerals |  |
| has part carbon in weight % |  |
| has part water in weight % |  |
| has chondrule abundance in volume % |  |
| has matrix abundance in volume % |  |
| has refractory inclusion abundance in volume % |  |
| has metal abundance in volume % |  |
| has chondrule mean diameter millimeters |  |
| stony meteorite | has weather resistance low |  |
| has fragmentation probability high because it is more friable than iron meteorite |  |
| has ablative mass loss high because it is more friable than iron meteorite |  |
| undifferentiated meteorite | has peak temperature less than 950 degree Celsius during its entire history since solidification |  |
| has parent body asteroid smaller than 100 km in diameter |  |
| has age oldest and most primitive rock in solar system |  |
| 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 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 |  |
| has origin meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal |  |
| 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 |  |
| conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |