Abbott Comparison Table

Meteorites View all facts Glossary Help

rock > meteorite > meteorite find > Abbott

Next H3 chondrite: Clovis no.1 Up: H3 chondrite, meteorite find Previous H3 chondrite: Grady (1937)

Abbott 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 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 is a kind of has comment 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

H3 chondrite 75 % of total iron agglomeration of particles, many of which record individual, diverse histories low 10 % 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 high because it is more friable than iron meteorite 12 to 21 % 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 349 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 type 3 chondrite 0.3 to 3 % by weight 9 high because it is more friable than iron meteorite bronzite chondrite 0.3 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

Abbott 75 % of total iron agglomeration of particles, many of which record individual, diverse histories which depends on its composition 10 % 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 during meteor phase which depends on composition 12 to 21 % in weight % Colfax County, New Mexico Abbott 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 lower because the fall was not witnessed 349 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 36° 18' N., 104° 17' 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 polymict regolith breccia 1951 0.3 to 3 % by weight 9.5 kg
9 directly proportional to initial velocity bronzite chondrite 0.3 millimeters less than 0.5 % by weight

Next H3 chondrite: Clovis no.1 Up: H3 chondrite, meteorite find Previous H3 chondrite: Grady (1937)

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 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	is a kind of	has comment	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
H3 chondrite	75 % of total iron	agglomeration of particles, many of which record individual, diverse histories	low	10 % 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	high because it is more friable than iron meteorite	12 to 21 %	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		349 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	type 3 chondrite			0.3 to 3 % by weight			9	high because it is more friable than iron meteorite	bronzite chondrite		0.3 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
Abbott	75 % of total iron	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	10 % 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	during meteor phase which depends on composition	12 to 21 %	in weight %	Colfax County, New Mexico	Abbott	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	lower because the fall was not witnessed	349 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	36° 18' N., 104° 17' 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		polymict regolith breccia	1951	0.3 to 3 % by weight	9.5 kg		9	directly proportional to initial velocity	bronzite chondrite		0.3 millimeters	less than 0.5 % by weight