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rock > meteorite > highly reduced meteorite > enstatite chondrite > E3 chondrite > EH3 chondrite > Sahara 97096

Sahara 97096 comparison table

Subject	has sediment mechanism	has oxidized iron content	has metal abundance	has part mean Ni content of sulfide	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 part metal maximum bulk	has fall location	has name	has chondrule glass type	has weather	has homogeneity of olivine and low Ca pyroxene	has chondrule abundance	has part chondrule	has degree of aqueous alteration	has oxidation state	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 matrix abundance	has petrologic type range	has fall coordinate	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 synonym	has definition	has chondrule mean diameter	has part sulfide Ni content
EH3 chondrite	agglomeration of particles, many of which record individual, diverse histories	zero	8 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 to 1 % by volume		high	greater than 5 % deviations	minor primary grains only	in weight %	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	clear, isotropic, variable abundance		definition goes here	60 to 80 % by volume	chondrules very sharply defined	none	highly reduced with very little FeO		1 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	clastic and minor opaque	none	less than 2 to 15 % by volume	which depends on degree of aqueous alteration and thermal metamorphism	in degrees, minutes and seconds of lattitude and longitude	0.2 to 1 % by weight	3 to 5	greater than 20 % by weight, kamacite and taenite in exsolution relationship	E3 chondrite		0.3 to 3 % by weight			1	E chondrite		0.2 millimeters	less than 0.5 % by weight
meteorite find												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 witnessed	485755 kg								in degrees, minutes and seconds of lattitude and longitude				meteorite	when the meteorite was found				1691		a meteorite whose fall was not witnessed
Sahara 97096	agglomeration of particles, many of which record individual, diverse histories	zero	8 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 to 1 % by volume	meteorite find	high	greater than 5 % deviations	minor primary grains only	in weight %	Sahara	Sahara 97096	clear, isotropic, variable abundance	can be severe due to long exposure time to environmental corrosion agents	definition goes here	60 to 80 % by volume	chondrules very sharply defined	none	highly reduced with very little FeO	lower because the fall was not witnessed	485755 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	clastic and minor opaque	none	less than 2 to 15 % by volume	which depends on degree of aqueous alteration and thermal metamorphism	y° 01' 43" N., x° 32' 21" W.	0.2 to 1 % by weight	3 to 5	greater than 20 % by weight, kamacite and taenite in exsolution relationship		1997	0.3 to 3 % by weight	28 kg		1691	E chondrite		0.2 millimeters	less than 0.5 % by weight

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