Subject |
has metal abundance |
has refractory inclusion abundance |
has olivine and low Ca pyroxene homogeneity |
has part feldspar |
has metamorphism mechanism |
has degree of secondary process |
has chondrule glass type |
has chondrule abundance |
has part chondrule |
has prototype |
has degree of aqueous alteration |
has structural state of low Ca pyroxene |
has part matrix |
has volatile content |
has degree of thermal metamorphism |
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 tenacity |
has chondrule mean diameter |
has part sulfide Ni content |
CH chondrite | 20 % by volume | 0.1 % by volume | greater than 5 % deviations | minor primary grains only | | | clear, isotropic, variable abundance | about 70 % by volume | chondrules very sharply defined | ALH 85085 meteorite | none | predominantly monoclinic | clastic and minor opaque | low | none | 5 % by 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 | type 3 chondrite | 0.3 to 3 % by weight | | 0.02 millimeters | less than 0.5 % by weight |
CI chondrite | 0 % by volume | less than 1 % by volume | | usually plagioclase tectosilicate | aqueous altermation | providing insight into geological evolution of parent asteroid | | less than 1 % by volume | no chondrules | Ivuna meteorite | strong | definition goes here | all fine-grained, opaque | high | | greater than 99 % by volume | 3 to 5 % by weight | 1 | | often minerals not found on Earth | type 1 chondrite | 18 to 22 % by weight | friable | no chondrules | |
CK chondrite | 0.01 % by volume | 4 % by volume | | usually plagioclase tectosilicate | | | | 15 % by volume | small sphere of about 1 mm diameter of formerly melted minerals | ??? meteorite | | 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) | | 0.7 millimeters | |
CM chondrite | 0.1 % by volume | 5 % by volume | greater than 5 % deviations | minor primary grains only | aqueous altermation | providing insight into geological evolution of parent asteroid | rare | 20 % by volume | chondrules very sharply defined | Mighei meteorite | moderate | predominantly monoclinic | mostly fine, opaque | | | 70 % by volume | 0.8 to 2.6 % by weight | 2 | less than 20 % by weight; taenite minor or absent | often minerals not found on Earth | type 2 chondrite | 2 to 16 % by weight | friable | 0.3 millimeters | greater than 0.5 % by weight |
CO chondrite | 1 to 5 % by volume | 13 % by volume | greater than 5 % deviations | minor primary grains only | | | clear, isotropic, variable abundance | 48 % by volume | chondrules very sharply defined | Ornans meteorite | none | predominantly monoclinic | clastic and minor opaque | | none | 34 % by 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 | type 3 chondrite | 0.3 to 3 % by weight | | 0.15 millimeters | less than 0.5 % by weight |
CR chondrite | 5 to 8 % by volume | 0.5 % by volume | greater than 5 % deviations | minor primary grains only | aqueous altermation | providing insight into geological evolution of parent asteroid | preserved | 50 to 60 % by volume | chondrules very sharply defined | ??? meteorite | moderate | predominantly monoclinic | mostly fine, opaque | | | 30 to 50 % by volume | 0.8 to 2.6 % by weight | 2 | less than 20 % by weight; taenite minor or absent | often minerals not found on Earth | type 2 chondrite | 2 to 16 % by weight | | 0.7 millimeters | greater than 0.5 % by weight |
CV chondrite | 0 to 5 % by volume | 10 % by volume | greater than 5 % deviations | minor primary grains only | | | clear, isotropic, variable abundance | 45 % by volume | chondrules very sharply defined | Vigarano meteorite | weak | predominantly monoclinic | clastic and minor opaque | | none | 40 % by volume | 0.2 to 1 % by weight | 3 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | iron-rich olivine, calcium aluminum inclusions | type 3 chondrite | 0.3 to 3 % by weight | | 1.0 millimeters | less than 0.5 % by weight |
ungrouped carbonaceous chondrite | in volume % | in volume % | | usually plagioclase tectosilicate | | | | in volume % | small sphere of about 1 mm diameter of formerly melted minerals | | | 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 | carbonaceous chondrite | in weight % | | millimeters | |