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anhydrous chondrite comparison table
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 low0.01 % by volume 4 % by volume elemental carbonusually plagioclase tectosilicatehigh because it is more friable than iron meteorite   15 % by volume8 % of meteorite falls small sphere of about 1 mm diameter of formerly melted mineralsrare relative to other chondrite types??? meteorite 2577 kgdefinition goes here fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents75 % by volumein weight %3 to 6 often minerals not found on Earthanhydrous chondrite0 % by weight (approximately)36high because it is more friable than iron meteorite 0.7 millimeters 
enstatite chondritezerowhich depends on its compositionin volume % in volume %  usually plagioclase tectosilicateduring meteor phase which depends on composition   in volume %  small sphere of about 1 mm diameter of formerly melted minerals  highly reduced with very little FeO234 kgdefinition goes here fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituentsin volume %in weight %  often minerals not found on Earthhighly reduced meteorite0 % by weight (approximately)16directly proportional to initial velocityE chondritemillimeters 
ordinary chondrite lowin volume % in volume %  usually plagioclase tectosilicatehigh 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 mineralsmost common chondrite observed from falls  20461 kgdefinition goes here fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituentsin volume %in weight %3 to 6 often minerals not found on Earthanhydrous chondrite0 % by weight (approximately)1030high because it is more friable than iron meteoriteO chondritemillimeters 
R chondrite low0.1 % by volume 0 % by volume  usually plagioclase tectosilicatehigh because it is more friable than iron meteorite   greater than 40 % by volume85.7 % of meteorite falls small sphere of about 1 mm diameter of formerly melted minerals Rumuruti meteoritehighly oxidized20461 kgdefinition goes here fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents36 % by volumein weight %3 to 6 enriched in 17O isotopeanhydrous chondrite0 % by weight (approximately)1030high because it is more friable than iron meteoriterumurutiite0.4 millimeters 
type 3 chondrite lowin volume % in volume %greater than 5 % deviations minor primary grains onlyhigh because it is more friable than iron meteorite  clear, isotropic, variable abundancein volume %85.7 % of meteorite fallsnonechondrules very sharply defined   20461 kgpredominantly monoclinicnoneclastic and minor opaquein volume %0.2 to 1 % by weight3greater than 20 % by weight, kamacite and taenite in exsolution relationshipoften minerals not found on Earthanhydrous chondrite0.3 to 3 % by weight1030high because it is more friable than iron meteorite millimetersless than 0.5 % by weight
type 4 chondrite lowin volume %the range over at which the alteration took placein volume %less than 5 % mean deviations secondary, grains than 2 micronshigh because it is more friable than iron meteoritethermal metamorphismproviding insight into geological evolution of parent asteroiddevitrified, absentin volume %85.7 % of meteorite falls chondrules well defined   20461 kggreater than 20 % monoclinicweaktransparent, recrystallized, small crystalsin volume %less than 0.2 % by weight4greater than 20 % by weight, kamacite and taenite in exsolution relationshipoften minerals not found on Earthanhydrous chondriteless than 1.5 % by weight1030high because it is more friable than iron meteorite millimetersless than 0.5 % by weight
type 5 chondrite lowin volume %the range over at which the alteration took placein volume %homogeneous secondary, 2 to 50 micron grainshigh because it is more friable than iron meteoritethermal metamorphismproviding insight into geological evolution of parent asteroiddevitrified, absentin volume %85.7 % of meteorite falls chondrules readily delineated   20461 kgless than 20 % monoclinicmoderatetransparent, recrystallized, moderate size crystalsin volume %less than 0.2 % by weight5greater than 20 % by weight, kamacite and taenite in exsolution relationshipoften minerals not found on Earthanhydrous chondriteless than 1.5 % by weight1030high because it is more friable than iron meteorite millimetersless than 0.5 % by weight
type 6 chondrite lowin volume %the range over at which the alteration took placein volume %homogeneous secondary, grains greater than 50 micronshigh because it is more friable than iron meteoritethermal metamorphismproviding insight into geological evolution of parent asteroiddevitrified, absentin volume %85.7 % of meteorite falls chondrules poorly defined   20461 kgorthorhombicstrongtransparent, recrystallized, coarse crystalsin volume %less than 0.2 % by weight6greater than 20 % by weight, kamacite and taenite in exsolution relationshipoften minerals not found on Earthanhydrous chondriteless than 1.5 % by weight1030high because it is more friable than iron meteorite millimetersless than 0.5 % by weight

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