Acfer 182 Comparison Table

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Acfer 182 comparison table

Subject has sediment mechanism has weather resistance has metal abundance has part mean Ni content of sulfide has age has refractory inclusion abundance is an instance of has distinguishing feature has olivine and low Ca pyroxene homogeneity has part feldspar has fragmentation probability 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 relative abundance has part chondrule has abundance has prototype has degree of aqueous alteration has value has total mass of find has structural state of low Ca pyroxene has peak temperature has part matrix has volatile content has parent body 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 image has number of find has ablative mass loss has definition has chondrule mean diameter has part sulfide Ni content

CH chondrite agglomeration of particles, many of which record individual, diverse histories low 20 % by volume in weight % oldest and most primitive rock in solar system 0.1 % by volume elemental carbon greater than 5 % deviations minor primary grains only high because it is more friable than iron meteorite 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 about 70 % by volume 8 % of meteorite falls chondrules very sharply defined rare relative to other chondrite types ALH 85085 meteorite none 2577 kg predominantly monoclinic less than 950 degree Celsius during its entire history since solidification clastic and minor opaque low asteroid smaller than 100 km in diameter none in degrees, minutes and seconds of lattitude and longitude 5 % by volume which depends on degree of aqueous alteration and thermal metamorphism 0.2 to 1 % by weight 3 greater than 20 % by weight, kamacite and taenite in exsolution relationship type 3 chondrite 0.3 to 3 % by weight 36 high because it is more friable than iron meteorite 0.02 millimeters less 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 witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude meteorite when the meteorite was found 1691 directly proportional to initial velocity a meteorite whose fall was not witnessed

Acfer 182 agglomeration of particles, many of which record individual, diverse histories which depends on its composition 20 % by volume in weight % oldest and most primitive rock in solar system 0.1 % by volume meteorite find elemental carbon greater than 5 % deviations minor primary grains only during meteor phase which depends on composition in weight % Algerian Sahara Desert Acfer 182 clear, isotropic, variable abundance can be severe due to long exposure time to environmental corrosion agents definition goes here about 70 % by volume chondrules very sharply defined rare relative to other chondrite types ALH 85085 meteorite none lower because the fall was not witnessed 485755 kg predominantly monoclinic less than 950 degree Celsius during its entire history since solidification clastic and minor opaque low asteroid smaller than 100 km in diameter none 27° 41.40' N., 4° 22.72' E. 5 % by volume which depends on degree of aqueous alteration and thermal metamorphism 0.2 to 1 % by weight 3 greater than 20 % by weight, kamacite and taenite in exsolution relationship 1991 0.3 to 3 % by weight
1691 directly proportional to initial velocity 0.02 millimeters less than 0.5 % by weight

Next CH chondrite: ALH 85085 Up: CH chondrite, meteorite find Previous CH chondrite: RKP 92435

Subject	has sediment mechanism	has weather resistance	has metal abundance	has part mean Ni content of sulfide	has age	has refractory inclusion abundance	is an instance of	has distinguishing feature	has olivine and low Ca pyroxene homogeneity	has part feldspar	has fragmentation probability	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 relative abundance	has part chondrule	has abundance	has prototype	has degree of aqueous alteration	has value	has total mass of find	has structural state of low Ca pyroxene	has peak temperature	has part matrix	has volatile content	has parent body	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 image	has number of find	has ablative mass loss	has definition	has chondrule mean diameter	has part sulfide Ni content
CH chondrite	agglomeration of particles, many of which record individual, diverse histories	low	20 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 % by volume		elemental carbon	greater than 5 % deviations	minor primary grains only	high because it is more friable than iron meteorite	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	about 70 % by volume	8 % of meteorite falls	chondrules very sharply defined	rare relative to other chondrite types	ALH 85085 meteorite	none		2577 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	clastic and minor opaque	low	asteroid smaller than 100 km in diameter	none	in degrees, minutes and seconds of lattitude and longitude	5 % by volume	which depends on degree of aqueous alteration and thermal metamorphism	0.2 to 1 % by weight	3	greater than 20 % by weight, kamacite and taenite in exsolution relationship	type 3 chondrite		0.3 to 3 % by weight		36	high because it is more friable than iron meteorite		0.02 millimeters	less 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 witnessed	485755 kg							in degrees, minutes and seconds of lattitude and longitude						meteorite	when the meteorite was found			1691	directly proportional to initial velocity	a meteorite whose fall was not witnessed
Acfer 182	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	20 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 % by volume	meteorite find	elemental carbon	greater than 5 % deviations	minor primary grains only	during meteor phase which depends on composition	in weight %	Algerian Sahara Desert	Acfer 182	clear, isotropic, variable abundance	can be severe due to long exposure time to environmental corrosion agents	definition goes here	about 70 % by volume		chondrules very sharply defined	rare relative to other chondrite types	ALH 85085 meteorite	none	lower because the fall was not witnessed	485755 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	clastic and minor opaque	low	asteroid smaller than 100 km in diameter	none	27° 41.40' N., 4° 22.72' E.	5 % by volume	which depends on degree of aqueous alteration and thermal metamorphism	0.2 to 1 % by weight	3	greater than 20 % by weight, kamacite and taenite in exsolution relationship		1991	0.3 to 3 % by weight		1691	directly proportional to initial velocity		0.02 millimeters	less than 0.5 % by weight