Subject |
has oxidized iron content |
has weather resistance |
has metal abundance |
has alteration temperature range |
has refractory inclusion abundance |
has olivine and low Ca pyroxene homogeneity |
has distinguishing feature |
has part feldspar |
has fragmentation probability |
has metamorphism mechanism |
has degree of secondary process |
has chondrule glass type |
has chondrule abundance |
has relative abundance |
has degree of aqueous alteration |
has part chondrule |
has abundance |
has prototype |
has oxidation state |
has total mass of find |
has structural state of low Ca pyroxene |
has degree of thermal metamorphism |
has part matrix |
has matrix abundance |
has part carbon |
has petrologic type |
has part maximum bulk Ni in metal |
has composition |
is a kind of |
has part water |
has number of find |
has ablative mass loss |
has synonym |
has chondrule mean diameter |
has part sulfide Ni content |
CK chondrite | | low | 0.01 % by volume | | 4 % by volume | | elemental carbon | usually plagioclase tectosilicate | high because it is more friable than iron meteorite | | | | 15 % by volume | 8 % of meteorite falls | | small sphere of about 1 mm diameter of formerly melted minerals | rare relative to other chondrite types | ??? meteorite | | 2577 kg | definition goes here | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | 75 % by volume | in weight % | 3 to 6 | | often minerals not found on Earth | anhydrous chondrite | 0 % by weight (approximately) | 36 | high because it is more friable than iron meteorite | | 0.7 millimeters | |
enstatite chondrite | zero | which depends on its composition | in volume % | | in volume % | | | usually plagioclase tectosilicate | during meteor phase which depends on composition | | | | in volume % | | | small sphere of about 1 mm diameter of formerly melted minerals | | | highly reduced with very little FeO | 234 kg | definition goes here | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | in volume % | in weight % | | | often minerals not found on Earth | highly reduced meteorite | 0 % by weight (approximately) | 16 | directly proportional to initial velocity | E chondrite | millimeters | |
ordinary chondrite | | low | in volume % | | in volume % | | | usually plagioclase tectosilicate | high because it is more friable than iron meteorite | | | | in volume % | 85.7 % of meteorite falls | | small sphere of about 1 mm diameter of formerly melted minerals | most common chondrite observed from falls | | | 20461 kg | definition goes here | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | in volume % | in weight % | 3 to 6 | | often minerals not found on Earth | anhydrous chondrite | 0 % by weight (approximately) | 1030 | high because it is more friable than iron meteorite | O chondrite | millimeters | |
R chondrite | | low | 0.1 % by volume | | 0 % by volume | | | usually plagioclase tectosilicate | high because it is more friable than iron meteorite | | | | greater than 40 % by volume | 85.7 % of meteorite falls | | small sphere of about 1 mm diameter of formerly melted minerals | | Rumuruti meteorite | highly oxidized | 20461 kg | definition goes here | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | 36 % by volume | in weight % | 3 to 6 | | enriched in 17O isotope | anhydrous chondrite | 0 % by weight (approximately) | 1030 | high because it is more friable than iron meteorite | rumurutiite | 0.4 millimeters | |
type 3 chondrite | | low | in volume % | | in volume % | greater than 5 % deviations | | minor primary grains only | high because it is more friable than iron meteorite | | | clear, isotropic, variable abundance | in volume % | 85.7 % of meteorite falls | none | chondrules very sharply defined | | | | 20461 kg | predominantly monoclinic | none | clastic and minor opaque | in volume % | 0.2 to 1 % by weight | 3 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | often minerals not found on Earth | anhydrous chondrite | 0.3 to 3 % by weight | 1030 | high because it is more friable than iron meteorite | | millimeters | less than 0.5 % by weight |
type 4 chondrite | | low | in volume % | the range over at which the alteration took place | in volume % | less than 5 % mean deviations | | secondary, grains than 2 microns | high because it is more friable than iron meteorite | thermal metamorphism | providing insight into geological evolution of parent asteroid | devitrified, absent | in volume % | 85.7 % of meteorite falls | | chondrules well defined | | | | 20461 kg | greater than 20 % monoclinic | weak | transparent, recrystallized, small crystals | in volume % | less than 0.2 % by weight | 4 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | often minerals not found on Earth | anhydrous chondrite | less than 1.5 % by weight | 1030 | high because it is more friable than iron meteorite | | millimeters | less than 0.5 % by weight |
type 5 chondrite | | low | in volume % | the range over at which the alteration took place | in volume % | homogeneous | | secondary, 2 to 50 micron grains | high because it is more friable than iron meteorite | thermal metamorphism | providing insight into geological evolution of parent asteroid | devitrified, absent | in volume % | 85.7 % of meteorite falls | | chondrules readily delineated | | | | 20461 kg | less than 20 % monoclinic | moderate | transparent, recrystallized, moderate size crystals | in volume % | less than 0.2 % by weight | 5 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | often minerals not found on Earth | anhydrous chondrite | less than 1.5 % by weight | 1030 | high because it is more friable than iron meteorite | | millimeters | less than 0.5 % by weight |
type 6 chondrite | | low | in volume % | the range over at which the alteration took place | in volume % | homogeneous | | secondary, grains greater than 50 microns | high because it is more friable than iron meteorite | thermal metamorphism | providing insight into geological evolution of parent asteroid | devitrified, absent | in volume % | 85.7 % of meteorite falls | | chondrules poorly defined | | | | 20461 kg | orthorhombic | strong | transparent, recrystallized, coarse crystals | in volume % | less than 0.2 % by weight | 6 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | often minerals not found on Earth | anhydrous chondrite | less than 1.5 % by weight | 1030 | high because it is more friable than iron meteorite | | millimeters | less than 0.5 % by weight |