Ragland Comparison Table

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Ragland comparison table

Subject has iron metal and iron sulfide 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 total iron content has olivine and low Ca pyroxene homogeneity has part feldspar has fragmentation probability has metal iron content 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 degree of aqueous alteration has petrologic subtype 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 fall coordinate has matrix abundance has petrologic type range has part carbon has petrologic type has part maximum bulk Ni in metal has composition is a kind of has find date has part water has mass has image has number of find has ablative mass loss has synonym has definition has chondrule mean diameter has part sulfide Ni content

LL3 chondrite 20 % of total iron agglomeration of particles, many of which record individual, diverse histories low 2 % by volume in weight % oldest and most primitive rock in solar system 0.1 to 1 % by volume low greater than 5 % deviations minor primary grains only high because it is more friable than iron meteorite about 2 % 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 85.7 % of meteorite falls chondrules very sharply defined most common chondrite observed from falls none 90 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 in degrees, minutes and seconds of lattitude and longitude 10 to 15 % 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 bronzite, olivine and minor oligoclase type 3 chondrite 0.3 to 3 % by weight 5 high because it is more friable than iron meteorite amphoterite 0.9 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 often minerals not found on Earth meteorite when the meteorite was found 1691 directly proportional to initial velocity a meteorite whose fall was not witnessed

Ragland 20 % of total iron agglomeration of particles, many of which record individual, diverse histories which depends on its composition 2 % by volume in weight % oldest and most primitive rock in solar system 0.1 to 1 % by volume meteorite find low greater than 5 % deviations minor primary grains only during meteor phase which depends on composition about 2 % in weight % wheat field in New Mexico Ragland 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 most common chondrite observed from falls none 3.4 lower because the fall was not witnessed 90 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 34° 46' 4" N., 103° 33' 33" W. 10 to 15 % 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 often minerals not found on Earth 1982 0.3 to 3 % by weight 12.1 kg
5 directly proportional to initial velocity amphoterite 0.9 millimeters less than 0.5 % by weight

Next LL3 chondrite: Semarkona Up: LL3 chondrite, meteorite find Previous LL3 chondrite: Parnallee

Subject	has iron metal and iron sulfide	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 total iron content	has olivine and low Ca pyroxene homogeneity	has part feldspar	has fragmentation probability	has metal iron content	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 degree of aqueous alteration	has petrologic subtype	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 fall coordinate	has matrix abundance	has petrologic type range	has part carbon	has petrologic type	has part maximum bulk Ni in metal	has composition	is a kind of	has find date	has part water	has mass	has image	has number of find	has ablative mass loss	has synonym	has definition	has chondrule mean diameter	has part sulfide Ni content
LL3 chondrite	20 % of total iron	agglomeration of particles, many of which record individual, diverse histories	low	2 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 to 1 % by volume		low	greater than 5 % deviations	minor primary grains only	high because it is more friable than iron meteorite	about 2 %	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	85.7 % of meteorite falls	chondrules very sharply defined	most common chondrite observed from falls	none			90 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	in degrees, minutes and seconds of lattitude and longitude	10 to 15 % 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	bronzite, olivine and minor oligoclase	type 3 chondrite		0.3 to 3 % by weight			5	high because it is more friable than iron meteorite	amphoterite		0.9 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						often minerals not found on Earth	meteorite	when the meteorite was found				1691	directly proportional to initial velocity		a meteorite whose fall was not witnessed
Ragland	20 % of total iron	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	2 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 to 1 % by volume	meteorite find	low	greater than 5 % deviations	minor primary grains only	during meteor phase which depends on composition	about 2 %	in weight %	wheat field in New Mexico	Ragland	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	most common chondrite observed from falls	none	3.4	lower because the fall was not witnessed	90 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	34° 46' 4" N., 103° 33' 33" W.	10 to 15 % 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	often minerals not found on Earth		1982	0.3 to 3 % by weight	12.1 kg		5	directly proportional to initial velocity	amphoterite		0.9 millimeters	less than 0.5 % by weight