Tieschitz Comparison Table

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Tieschitz 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 fall date has name has chondrule glass type has weather has fall description 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 is a kind of 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

L3 chondrite 50 % of total iron agglomeration of particles, many of which record individual, diverse histories low 5 % 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 5 to 10 % in weight % strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity recorded by eyewitness or inferred from dating methods 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 131 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 10 high because it is more friable than iron meteorite hypersthene chondrite 0.7 millimeters less than 0.5 % by weight

meteorite fall 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 recorded by eyewitness or instruments based on the locale, region, or nearby town in which the fall occurred negligible due to quick recovery of meteorite before corrosion begins what witnesses saw or what was recorded by instruments higher because the fall was witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude meteorite 1691 directly proportional to initial velocity a meteorite whose fall was witnessed by human or electronic means

Tieschitz 50 % of total iron agglomeration of particles, many of which record individual, diverse histories which depends on its composition 5 % by volume in weight % oldest and most primitive rock in solar system 0.1 to 1 % by volume meteorite fall low greater than 5 % deviations minor primary grains only during meteor phase which depends on composition 5 to 10 % in weight % Prostejov, Jihomoravsky, Czechoslovakia 1:45 pm July 15, 1878 Tieschitz clear, isotropic, variable abundance negligible due to quick recovery of meteorite before corrosion begins what witnesses saw or what was recorded by instruments definition goes here 60 to 80 % by volume chondrules very sharply defined most common chondrite observed from falls none 3.6 higher because the fall was witnessed 131 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 49° 36' N., 17° 7' E. 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 0.3 to 3 % by weight 27.4 kg
10 directly proportional to initial velocity hypersthene chondrite 0.7 millimeters less than 0.5 % by weight

Next L3 chondrite: Moorabie Up: L3 chondrite, meteorite fall Previous L3 chondrite: Tagounite 019

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 fall date	has name	has chondrule glass type	has weather	has fall description	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	is a kind of	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
L3 chondrite	50 % of total iron	agglomeration of particles, many of which record individual, diverse histories	low	5 % 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	5 to 10 %	in weight %	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	recorded by eyewitness or inferred from dating methods	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			131 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			10	high because it is more friable than iron meteorite	hypersthene chondrite		0.7 millimeters	less than 0.5 % by weight
meteorite fall			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	recorded by eyewitness or instruments	based on the locale, region, or nearby town in which the fall occurred		negligible due to quick recovery of meteorite before corrosion begins	what witnesses saw or what was recorded by instruments								higher because the fall was witnessed	485755 kg						in degrees, minutes and seconds of lattitude and longitude						meteorite				1691	directly proportional to initial velocity		a meteorite whose fall was witnessed by human or electronic means
Tieschitz	50 % of total iron	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	5 % by volume	in weight %	oldest and most primitive rock in solar system	0.1 to 1 % by volume	meteorite fall	low	greater than 5 % deviations	minor primary grains only	during meteor phase which depends on composition	5 to 10 %	in weight %	Prostejov, Jihomoravsky, Czechoslovakia	1:45 pm July 15, 1878	Tieschitz	clear, isotropic, variable abundance	negligible due to quick recovery of meteorite before corrosion begins	what witnesses saw or what was recorded by instruments	definition goes here	60 to 80 % by volume		chondrules very sharply defined	most common chondrite observed from falls	none	3.6	higher because the fall was witnessed	131 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	49° 36' N., 17° 7' E.	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		0.3 to 3 % by weight	27.4 kg		10	directly proportional to initial velocity	hypersthene chondrite		0.7 millimeters	less than 0.5 % by weight