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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > ureilite > medium shock ureilite > euhedral ureilite

euhedral ureilite comparison table

Subject	has weather resistance	has shock texture	has reference	has minerology	has degree of shock metamorphism	fragment	has shock stage	survive fall if	is an instance of	has distinguishing feature	vaporize completely if	has fragmentation probability	be associated with	has fall location	has olivine grain characteristic	has fall date	has metamorphism mechanism	has impact angle	has pyroxene shock metamorphism	has likely origin	has solidification mechanism	has name	has shock diagnostic mineral	has olivine composition	has olivine shock metamorphism	has genesi	has weather	has letter designation	has relative abundance	shatter	has texture	has value	has total mass of find	has impact velocity	has matrix composition	has fall coordinate	has characteristic mineral	has composition	has monetary value	has original mass	has part mineral	has find date	has origin	has number of find	has ablative mass loss	produce	has shock pressure	has solidification timescale	has pigeonite composition	has intergranular boundary	have crater image	has pyroxene content	has fall map	has petrology
Dingo Pup Donga	which depends on its composition	greater extent of fracturing, undulatory extinction, and kink banding	Berkley et. al (1980)	olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite)	medium	during meteor phase	S4-S6	it fragments because smaller pieces with less mass are more easily slowed by the atmosphere	meteorite find	no chondrules	size is between 3 micrometers and 3 millimeters	during meteor phase which depends on composition	crater	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal	recorded by eyewitness or inferred from dating methods	shock metamorphism		may be cloudy due to glassy inclusions	partial melting residue	cooling in deep underground chambers	based on the locale, region, or nearby town in which the fall occurred	diamonds and/or lonsdaleite	Fo% 84	sub-grain boundaries may be prominent		can be severe due to long exposure time to environmental corrosion agents	AURE		during impact phase	size-sorted layers	lower because the fall was not witnessed	485755 kg	when it hits the ground which is smaller than its velocity before it enters the atmosphere	carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	in degrees, minutes and seconds of lattitude and longitude	olivine-pigeonite about 90% by volume	often minerals not found on Earth	large if the fall was witnessed	which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site		when the meteorite was found	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691	directly proportional to initial velocity	power outages and failures in electrical equipment due to EMP (electromagnetic pulse)	from 20 GPa to 100 GPa	very slow	Wo% 5.0 En% 81	euhedral, non-interlocking grains		0.5 in modal pyroxene/(pryroxene+olivine)	which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity	coarse-grained granular

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