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rock > gravitationally separated rock > fractional crystallized rock > plutonic cumulate > dunitic wehrlite
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dunitic wehrlite comparison table
Subject has weather resistance has minerology fragment survive fall if has distinguishing feature vaporize completely if has fragmentation probability be associated with has fall location has fall date has impact angle has likely origin has solidification mechanism has name has genesi has relative abundance shatter has texture has prototype has total mass of find has impact velocity has fall coordinate has composition has original mass has monetary value is a kind of has part mineral has property has number of find has origin has ablative mass loss produce has solidification timescale have crater image has fall map has petrology
brachinitelowolivine, augite, Fe-sulfide, some orthopyroxene and some sodic plagioclaseduring meteor phaseit fragments because smaller pieces with less mass are more easily slowed by the atmosphereno chondrulessize is between 3 micrometers and 3 millimetershigh because it is more friable than iron meteoritecraterstrewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocityrecorded by eyewitness or inferred from dating methods metamorphosed chondrite, partial melting residuecooling in deep underground chambersbased on the locale, region, or nearby town in which the fall occurredfractional crystallization7.1 % of meteorite fallsduring impact phase Brachina meteorite1606 kgwhen it hits the ground which is smaller than its velocity before it enters the atmospherein degrees, minutes and seconds of lattitude and longitudeolivine and some clinopyroxenewhich can over an order of magnitude greater than total mass of fragment(s) collected at the impact sitelarge if the fall was witnesseddunitic wehrlite formed by separation of molten rock in a gravity field70asteroidhigh because it is more friable than iron meteoritepower outages and failures in electrical equipment due to EMP (electromagnetic pulse)very slow which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocitymedium- to coarse-grained equigranular

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