| Orgueil | has image
 |  |
| is an instance of meteorite fall |  |
| is an instance of CI chondrite |  |
| has name Orgueil |  |
| has fall coordinates 43° 53' N., 1° 23' E. |  |
| has fall date May 14, 1864 few minutes after 8:00 pm |  |
| has mass 11 kg |  |
| meteorite fall | has value higher because the fall was witnessed |  |
| has fall description what witnesses saw or what was recorded by instruments |  |
| has weathering negligible due to quick recovery of meteorite before corrosion begins |  |
| CI chondrite | has prototype Ivuna meteorite |  |
| has chondrule abundance less than 1 % by volume |  |
| has matrix abundance greater than 99 % by volume |  |
| has refractory inclusion abundance less than 1 % by volume |  |
| has metal abundance 0 % by volume |  |
| has chondrule mean diameter no chondrules |  |
| has tenacity friable |  |
| has volatile content high |  |
| meteorite | has fall location strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity |  |
| 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 |  |
| 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 |  |
| 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 |  |
| 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 |  |
| type 1 chondrite | has petrologic type 1 |  |
| has degree of aqueous alteration strong |  |
| has part matrix all fine-grained, opaque |  |
| has part chondrule no chondrules |  |
| has part carbon 3 to 5 % by weight |  |
| has part water 18 to 22 % by weight |  |
| rock | has part mineral |  |
| has texture |  |
| has genesis |  |
| chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism |  |
| 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 % |  |
| water altered chondrite | has metamorphism mechanism aqueous altermation |  |
| 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 |  |
| altered chondrite | has degree of secondary processing providing insight into geological evolution of parent asteroid |  |
| conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories |  |