HaH 046 Comparison Table

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rock > metamorphic rock > altered chondrite > thermally altered chondrite > type 6 chondrite > LL6 chondrite > HaH 046

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HaH 046 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 alteration temperature range 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 metal iron content has fragmentation probability has fall location has metamorphism mechanism has degree of secondary process has chondrule glass type has weather has homogeneity of olivine and low Ca pyroxene has acronym has chondrule abundance has relative abundance has abundance has part chondrule 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 petrologic type range has matrix abundance 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 number of find has ablative mass loss has synonym has chondrule mean diameter has part sulfide Ni content

Hammadah al Hamra meteorite which depends on its composition during meteor phase which depends on composition Hammadah al Hamra can be severe due to long exposure time to environmental corrosion agents HaH lower because the fall was not witnessed 485755 kg often minerals not found on Earth Sahara meteorite when the meteorite was found 1691 directly proportional to initial velocity

LL6 chondrite 20 % of total iron agglomeration of particles, many of which record individual, diverse histories low 2 % by volume in weight % the range over at which the alteration took place oldest and most primitive rock in solar system 0.1 to 1 % by volume low homogeneous secondary, grains greater than 50 microns in weight % about 2 % high because it is more friable than iron meteorite strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity thermal metamorphism providing insight into geological evolution of parent asteroid devitrified, absent definition goes here 60 to 80 % by volume 85.7 % of meteorite falls most common chondrite observed from falls chondrules poorly defined 715 kg orthorhombic less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter transparent, recrystallized, coarse crystals strong which depends on degree of aqueous alteration and thermal metamorphism 10 to 15 % by volume less than 0.2 % by weight 6 greater than 20 % by weight, kamacite and taenite in exsolution relationship bronzite, olivine and minor oligoclase type 6 chondrite less than 1.5 % by weight 20 high because it is more friable than iron meteorite amphoterite 0.9 millimeters less than 0.5 % by weight

HaH 046 20 % of total iron agglomeration of particles, many of which record individual, diverse histories which depends on its composition 2 % by volume in weight % the range over at which the alteration took place oldest and most primitive rock in solar system 0.1 to 1 % by volume Hammadah al Hamra meteorite low homogeneous secondary, grains greater than 50 microns in weight % about 2 % during meteor phase which depends on composition Hammadah al Hamra thermal metamorphism providing insight into geological evolution of parent asteroid devitrified, absent can be severe due to long exposure time to environmental corrosion agents definition goes here HaH 60 to 80 % by volume most common chondrite observed from falls chondrules poorly defined lower because the fall was not witnessed 715 kg orthorhombic less than 950 degree Celsius during its entire history since solidification asteroid smaller than 100 km in diameter transparent, recrystallized, coarse crystals strong which depends on degree of aqueous alteration and thermal metamorphism 10 to 15 % by volume less than 0.2 % by weight 6 greater than 20 % by weight, kamacite and taenite in exsolution relationship bronzite, olivine and minor oligoclase when the meteorite was found less than 1.5 % by weight 20 directly proportional to initial velocity amphoterite 0.9 millimeters less than 0.5 % by weight

Next Hammadah al Hamra meteorite: HaH 064 Up: Hammadah al Hamra meteorite, LL6 chondrite Previous Hammadah al Hamra meteorite: HaH 260

Subject	has iron metal and iron sulfide	has sediment mechanism	has weather resistance	has metal abundance	has part mean Ni content of sulfide	has alteration temperature range	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 metal iron content	has fragmentation probability	has fall location	has metamorphism mechanism	has degree of secondary process	has chondrule glass type	has weather	has homogeneity of olivine and low Ca pyroxene	has acronym	has chondrule abundance	has relative abundance	has abundance	has part chondrule	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 petrologic type range	has matrix abundance	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 number of find	has ablative mass loss	has synonym	has chondrule mean diameter	has part sulfide Ni content
Hammadah al Hamra meteorite			which depends on its composition												during meteor phase which depends on composition	Hammadah al Hamra				can be severe due to long exposure time to environmental corrosion agents		HaH					lower because the fall was not witnessed	485755 kg											often minerals not found on Earth	Sahara meteorite	when the meteorite was found		1691	directly proportional to initial velocity
LL6 chondrite	20 % of total iron	agglomeration of particles, many of which record individual, diverse histories	low	2 % by volume	in weight %	the range over at which the alteration took place	oldest and most primitive rock in solar system	0.1 to 1 % by volume		low	homogeneous	secondary, grains greater than 50 microns	in weight %	about 2 %	high because it is more friable than iron meteorite	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	thermal metamorphism	providing insight into geological evolution of parent asteroid	devitrified, absent		definition goes here		60 to 80 % by volume	85.7 % of meteorite falls	most common chondrite observed from falls	chondrules poorly defined		715 kg	orthorhombic	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	transparent, recrystallized, coarse crystals	strong	which depends on degree of aqueous alteration and thermal metamorphism	10 to 15 % by volume	less than 0.2 % by weight	6	greater than 20 % by weight, kamacite and taenite in exsolution relationship	bronzite, olivine and minor oligoclase	type 6 chondrite		less than 1.5 % by weight	20	high because it is more friable than iron meteorite	amphoterite	0.9 millimeters	less than 0.5 % by weight
HaH 046	20 % of total iron	agglomeration of particles, many of which record individual, diverse histories	which depends on its composition	2 % by volume	in weight %	the range over at which the alteration took place	oldest and most primitive rock in solar system	0.1 to 1 % by volume	Hammadah al Hamra meteorite	low	homogeneous	secondary, grains greater than 50 microns	in weight %	about 2 %	during meteor phase which depends on composition	Hammadah al Hamra	thermal metamorphism	providing insight into geological evolution of parent asteroid	devitrified, absent	can be severe due to long exposure time to environmental corrosion agents	definition goes here	HaH	60 to 80 % by volume		most common chondrite observed from falls	chondrules poorly defined	lower because the fall was not witnessed	715 kg	orthorhombic	less than 950 degree Celsius during its entire history since solidification	asteroid smaller than 100 km in diameter	transparent, recrystallized, coarse crystals	strong	which depends on degree of aqueous alteration and thermal metamorphism	10 to 15 % by volume	less than 0.2 % by weight	6	greater than 20 % by weight, kamacite and taenite in exsolution relationship	bronzite, olivine and minor oligoclase		when the meteorite was found	less than 1.5 % by weight	20	directly proportional to initial velocity	amphoterite	0.9 millimeters	less than 0.5 % by weight