LEW 85332 Comparison Table

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Next Antarctic meteorite: LEW 88516 Up: Antarctic meteorite, ungrouped carbonaceous chondrite Previous Antarctic meteorite: Isna

LEW 85332 comparison table

Subject has sediment mechanism has weather resistance has metal abundance has part mean Ni content of sulfide has age has refractory inclusion abundance is an instance of has distinguishing feature has part feldspar has part metal maximum bulk has fragmentation probability has fall location has name has homogeneity of olivine and low Ca pyroxene has chondrule abundance has relative abundance has part chondrule has abundance has total mass of find has structural state of low Ca pyroxene has peak temperature has parent body has part matrix has matrix abundance has petrologic type range has part carbon is a kind of has find date has part water has number of find has ablative mass loss has chondrule mean diameter

Antarctic meteorite which depends on its composition during meteor phase which depends on composition indicated by letters in the beginning of name 3 or 4 letter contracted from find location then last two digits of year then id number 485755 kg meteorite recovery year is first 2 numbers in name 1691 directly proportional to initial velocity

ungrouped carbonaceous chondrite agglomeration of particles, many of which record individual, diverse histories low in volume % in weight % oldest and most primitive rock in solar system in volume % elemental carbon usually plagioclase tectosilicate in weight % high because it is more friable than iron meteorite strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity based on the locale, region, or nearby town in which the fall occurred definition goes here in volume % 8 % of meteorite falls small sphere of about 1 mm diameter of formerly melted minerals rare relative to other chondrite types 2577 kg definition goes here less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents in volume % which depends on degree of aqueous alteration and thermal metamorphism in weight % carbonaceous chondrite in weight % 36 high because it is more friable than iron meteorite millimeters

LEW 85332 agglomeration of particles, many of which record individual, diverse histories which depends on its composition in volume % in weight % oldest and most primitive rock in solar system in volume % Antarctic meteorite elemental carbon usually plagioclase tectosilicate in weight % during meteor phase which depends on composition indicated by letters in the beginning of name LEW 85332 definition goes here in volume % small sphere of about 1 mm diameter of formerly melted minerals rare relative to other chondrite types 485755 kg definition goes here less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents in volume % which depends on degree of aqueous alteration and thermal metamorphism in weight % 1985 in weight % 1691 directly proportional to initial velocity millimeters

Next Antarctic meteorite: LEW 88516 Up: Antarctic meteorite, ungrouped carbonaceous chondrite Previous Antarctic meteorite: Isna

Subject	has sediment mechanism	has weather resistance	has metal abundance	has part mean Ni content of sulfide	has age	has refractory inclusion abundance	is an instance of	has distinguishing feature	has part feldspar	has part metal maximum bulk	has fragmentation probability	has fall location	has name	has homogeneity of olivine and low Ca pyroxene	has chondrule abundance	has relative abundance	has part chondrule	has abundance	has total mass of find	has structural state of low Ca pyroxene	has peak temperature	has parent body	has part matrix	has matrix abundance	has petrologic type range	has part carbon	is a kind of	has find date	has part water	has number of find	has ablative mass loss	has chondrule mean diameter
Antarctic meteorite		which depends on its composition									during meteor phase which depends on composition	indicated by letters in the beginning of name	3 or 4 letter contracted from find location then last two digits of year then id number						485755 kg								meteorite	recovery year is first 2 numbers in name		1691	directly proportional to initial velocity
ungrouped carbonaceous chondrite	agglomeration of particles, many of which record individual, diverse histories	low	in volume %	in weight %	oldest and most primitive rock in solar system	in volume %		elemental carbon	usually plagioclase tectosilicate	in weight %	high because it is more friable than iron meteorite	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	based on the locale, region, or nearby town in which the fall occurred	definition goes here	in volume %	8 % of meteorite falls	small sphere of about 1 mm diameter of formerly melted minerals	rare relative to other chondrite types	2577 kg	definition goes here	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents	in volume %	which depends on degree of aqueous alteration and thermal metamorphism	in weight %	carbonaceous chondrite		in weight %	36	high because it is more friable than iron meteorite	millimeters
LEW 85332	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	in volume %	in weight %	oldest and most primitive rock in solar system	in volume %	Antarctic meteorite	elemental carbon	usually plagioclase tectosilicate	in weight %	during meteor phase which depends on composition	indicated by letters in the beginning of name	LEW 85332	definition goes here	in volume %		small sphere of about 1 mm diameter of formerly melted minerals	rare relative to other chondrite types	485755 kg	definition goes here	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents	in volume %	which depends on degree of aqueous alteration and thermal metamorphism	in weight %		1985	in weight %	1691	directly proportional to initial velocity	millimeters