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| rock > meteorite > highly reduced meteorite > enstatite chondrite |
| enstatite chondrite (E chondrite) | ||||
| subject | fact | |||
| enstatite chondrite | is a kind of anhydrous chondrite | ![]() |
| is a kind of highly reduced meteorite | ![]() | |
| has synonym E chondrite | ![]() | |
| has total mass of finds 234 kg | ![]() | |
| has number of finds 16 | ![]() | |
| has oxidized iron content zero | ![]() | |
| anhydrous chondrite | has part water 0 % by weight (approximately) | ![]() |
| highly reduced meteorite | has oxidation state highly reduced with very little FeO | ![]() |
| chondrite | has petrologic type range which depends on degree of aqueous alteration and thermal metamorphism | ![]() |
| has relative abundance 85.7 % of meteorite falls | ![]() | |
| 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 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 | ![]() | |
| 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 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 | ![]() | |
| 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 | ![]() | |
| 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 | ![]() | |
| rock | has part mineral | ![]() |
| has texture | ![]() | |
| has genesis | ![]() | |
| conglomerate | has sediment mechanism agglomeration of particles, many of which record individual, diverse histories | ![]() |
Kinds of enstatite chondrite :
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