clinopyroxenite Comparison Table

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clinopyroxenite comparison table

Subject has weather resistance 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 solidification mechanism has name has genesi has letter designation has relative abundance shatter has texture has prototype has total mass of find has impact velocity has fall coordinate has characteristic mineral 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 be an acronym for has fall map

nakhilite low during meteor phase it fragments because smaller pieces with less mass are more easily slowed by the atmosphere no chondrules size is between 3 micrometers and 3 millimeters high because it is more friable than iron meteorite crater strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity recorded by eyewitness or inferred from dating methods cooling in deep underground chambers based on the locale, region, or nearby town in which the fall occurred fractional crystallization ACANOM 7.1 % of meteorite falls during impact phase Nakhla meteorite 1606 kg when it hits the ground which is smaller than its velocity before it enters the atmosphere in degrees, minutes and seconds of lattitude and longitude diopside-olivine cumulus-augite-bearing proxenite which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site large if the fall was witnessed clinopyroxenite formed by separation of molten rock in a gravity field 70 Mars high because it is more friable than iron meteorite power outages and failures in electrical equipment due to EMP (electromagnetic pulse) very slow Shergottite, Nakhilite, Chassignite which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity

Next plutonic cumulate: diogenite Up: plutonic cumulate Previous plutonic cumulate: orthopyroxenite

Subject	has weather resistance	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 solidification mechanism	has name	has genesi	has letter designation	has relative abundance	shatter	has texture	has prototype	has total mass of find	has impact velocity	has fall coordinate	has characteristic mineral	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	be an acronym for	has fall map
nakhilite	low	during meteor phase	it fragments because smaller pieces with less mass are more easily slowed by the atmosphere	no chondrules	size is between 3 micrometers and 3 millimeters	high because it is more friable than iron meteorite	crater	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	recorded by eyewitness or inferred from dating methods		cooling in deep underground chambers	based on the locale, region, or nearby town in which the fall occurred	fractional crystallization	ACANOM	7.1 % of meteorite falls	during impact phase		Nakhla meteorite	1606 kg	when it hits the ground which is smaller than its velocity before it enters the atmosphere	in degrees, minutes and seconds of lattitude and longitude	diopside-olivine	cumulus-augite-bearing proxenite	which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site	large if the fall was witnessed	clinopyroxenite		formed by separation of molten rock in a gravity field	70	Mars	high because it is more friable than iron meteorite	power outages and failures in electrical equipment due to EMP (electromagnetic pulse)	very slow		Shergottite, Nakhilite, Chassignite	which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity