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rock > metamorphic rock > altered chondrite > thermally altered chondrite > type 6 chondrite > H6 chondrite > Mulga North
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Mulga North comparison table
Subject has iron metal and iron sulfide has sediment mechanism has weather resistance has metal abundance has part mean Ni content of sulfide has alteration temperature range has age has refractory inclusion abundance is an instance of has total iron content has olivine and low Ca pyroxene homogeneity has part feldspar has fragmentation probability has metal iron content has part metal maximum bulk has fall location has metamorphism mechanism has degree of secondary process has name has chondrule glass type has weather has homogeneity of olivine and low Ca pyroxene has chondrule abundance has relative abundance has part chondrule has abundance has value has total mass of find has structural state of low Ca pyroxene has peak temperature has parent body has part matrix has degree of thermal metamorphism has fall coordinate has matrix abundance has petrologic type range has part carbon has petrologic type has part maximum bulk Ni in metal is a kind of has find date has part water has mass has image has number of find has ablative mass loss has synonym has definition has chondrule mean diameter has part sulfide Ni content
H6 chondrite75 % of total ironagglomeration of particles, many of which record individual, diverse historieslow10 % by volumein weight %the range over at which the alteration took placeoldest and most primitive rock in solar system0.1 to 1 % by volume highhomogeneoussecondary, grains greater than 50 micronshigh because it is more friable than iron meteorite12 to 21 %in weight %strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocitythermal metamorphismproviding insight into geological evolution of parent asteroidbased on the locale, region, or nearby town in which the fall occurreddevitrified, absent definition goes here60 to 80 % by volume85.7 % of meteorite fallschondrules poorly definedmost common chondrite observed from falls 11357 kgorthorhombicless than 950 degree Celsius during its entire history since solidificationasteroid smaller than 100 km in diametertransparent, recrystallized, coarse crystalsstrongin degrees, minutes and seconds of lattitude and longitude10 to 15 % by volumewhich depends on degree of aqueous alteration and thermal metamorphismless than 0.2 % by weight6greater than 20 % by weight, kamacite and taenite in exsolution relationshiptype 6 chondrite less than 1.5 % by weight  44high because it is more friable than iron meteoritebronzite chondrite 0.3 millimetersless than 0.5 % by weight
meteorite find  which depends on its composition         during meteor phase which depends on composition  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 can be severe due to long exposure time to environmental corrosion agents     lower because the fall was not witnessed485755 kg     in degrees, minutes and seconds of lattitude and longitude     meteoritewhen the meteorite was found   1691directly proportional to initial velocity a meteorite whose fall was not witnessed  
Mulga North75 % of total ironagglomeration of particles, many of which record individual, diverse historieswhich depends on its composition10 % by volumein weight %the range over at which the alteration took placeoldest and most primitive rock in solar system0.1 to 1 % by volumemeteorite findhighhomogeneoussecondary, grains greater than 50 micronsduring meteor phase which depends on composition12 to 21 %in weight %Western Australiathermal metamorphismproviding insight into geological evolution of parent asteroidMulga Northdevitrified, absentcan be severe due to long exposure time to environmental corrosion agentsdefinition goes here60 to 80 % by volume chondrules poorly definedmost common chondrite observed from fallslower because the fall was not witnessed11357 kgorthorhombicless than 950 degree Celsius during its entire history since solidificationasteroid smaller than 100 km in diametertransparent, recrystallized, coarse crystalsstrong30° 11' S., 126° 22' E.10 to 15 % by volumewhich depends on degree of aqueous alteration and thermal metamorphismless than 0.2 % by weight6greater than 20 % by weight, kamacite and taenite in exsolution relationship 1964less than 1.5 % by weight2.42 kg
44directly proportional to initial velocitybronzite chondrite 0.3 millimetersless than 0.5 % by weight

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