Camel Donga 003 Comparison Table

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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > HED meteorite > eucrite > Camel Donga 003

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Camel Donga 003 comparison table

Subject has sediment mechanism has metal abundance has part mean Ni content of sulfide has minerology has age has refractory inclusion abundance is an instance of has distinguishing feature has olivine and low Ca pyroxene homogeneity has part feldspar has part metal maximum bulk has fall location has likely origin has solidification mechanism has name has chondrule glass type has letter designation 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 total mass of find has structural state of low Ca pyroxene has peak temperature has part matrix has parent body has degree of thermal metamorphism has matrix abundance has petrologic type range has part carbon has characteristic mineral has petrologic type has part maximum bulk Ni in metal has composition is a kind of has find date has part water has image has origin has number of find has solidification timescale has chondrule mean diameter has part sulfide Ni content be an acronym for has petrology

CK3 chondrite agglomeration of particles, many of which record individual, diverse histories 0.01 % by volume in weight % oldest and most primitive rock in solar system 4 % by volume elemental carbon greater than 5 % deviations minor primary grains only 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 15 % by volume 8 % of meteorite falls chondrules very sharply defined rare relative to other chondrite types ??? meteorite none 2577 kg predominantly monoclinic less than 950 degree Celsius during its entire history since solidification clastic and minor opaque asteroid smaller than 100 km in diameter none 75 % 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 type 3 chondrite 0.3 to 3 % by weight meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 36 0.7 millimeters less than 0.5 % by weight

eucrite orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica no chondrules strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity cumulates, crystallized melts, impact mixing extrusion onto the surface of the planet or asteroid via a volcanic eruption based on the locale, region, or nearby town in which the fall occurred AUEC 7.1 % of meteorite falls 231 kg anorthite-pigeonite Ca-rich silicates (with very few exceptions) basalt 4 Vesta 23 very rapid Howardite, Eucrite, Diogenite coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated

Camel Donga 003 agglomeration of particles, many of which record individual, diverse histories 0.01 % by volume in weight % orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica oldest and most primitive rock in solar system 4 % by volume eucrite elemental carbon greater than 5 % deviations minor primary grains only in weight % Camel Donga, West Australia, Australia cumulates, crystallized melts, impact mixing extrusion onto the surface of the planet or asteroid via a volcanic eruption Camel Donga clear, isotropic, variable abundance AUEC definition goes here 15 % by volume 8 % of meteorite falls chondrules very sharply defined rare relative to other chondrite types ??? meteorite none 231 kg predominantly monoclinic less than 950 degree Celsius during its entire history since solidification clastic and minor opaque asteroid smaller than 100 km in diameter none 75 % by volume which depends on degree of aqueous alteration and thermal metamorphism 0.2 to 1 % by weight anorthite-pigeonite Ca-rich 3 greater than 20 % by weight, kamacite and taenite in exsolution relationship silicates (with very few exceptions) 1984 0.3 to 3 % by weight
4 Vesta 23 very rapid 0.7 millimeters less than 0.5 % by weight Howardite, Eucrite, Diogenite coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated

Next CK3 chondrite: Watson 002 Up: CK3 chondrite, eucrite

Subject	has sediment mechanism	has metal abundance	has part mean Ni content of sulfide	has minerology	has age	has refractory inclusion abundance	is an instance of	has distinguishing feature	has olivine and low Ca pyroxene homogeneity	has part feldspar	has part metal maximum bulk	has fall location	has likely origin	has solidification mechanism	has name	has chondrule glass type	has letter designation	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 total mass of find	has structural state of low Ca pyroxene	has peak temperature	has part matrix	has parent body	has degree of thermal metamorphism	has matrix abundance	has petrologic type range	has part carbon	has characteristic mineral	has petrologic type	has part maximum bulk Ni in metal	has composition	is a kind of	has find date	has part water	has image	has origin	has number of find	has solidification timescale	has chondrule mean diameter	has part sulfide Ni content	be an acronym for	has petrology
CK3 chondrite	agglomeration of particles, many of which record individual, diverse histories	0.01 % by volume	in weight %		oldest and most primitive rock in solar system	4 % by volume		elemental carbon	greater than 5 % deviations	minor primary grains only	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	15 % by volume	8 % of meteorite falls	chondrules very sharply defined	rare relative to other chondrite types	??? meteorite	none	2577 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	clastic and minor opaque	asteroid smaller than 100 km in diameter	none	75 % 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	type 3 chondrite		0.3 to 3 % by weight		meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	36		0.7 millimeters	less than 0.5 % by weight
eucrite				orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica				no chondrules				strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity	cumulates, crystallized melts, impact mixing	extrusion onto the surface of the planet or asteroid via a volcanic eruption	based on the locale, region, or nearby town in which the fall occurred		AUEC			7.1 % of meteorite falls					231 kg									anorthite-pigeonite Ca-rich			silicates (with very few exceptions)	basalt				4 Vesta	23	very rapid			Howardite, Eucrite, Diogenite	coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated
Camel Donga 003	agglomeration of particles, many of which record individual, diverse histories	0.01 % by volume	in weight %	orthopyroxene, olivine, chromite; pigeonite, calcic plagioclase, silica	oldest and most primitive rock in solar system	4 % by volume	eucrite	elemental carbon	greater than 5 % deviations	minor primary grains only	in weight %	Camel Donga, West Australia, Australia	cumulates, crystallized melts, impact mixing	extrusion onto the surface of the planet or asteroid via a volcanic eruption	Camel Donga	clear, isotropic, variable abundance	AUEC	definition goes here	15 % by volume	8 % of meteorite falls	chondrules very sharply defined	rare relative to other chondrite types	??? meteorite	none	231 kg	predominantly monoclinic	less than 950 degree Celsius during its entire history since solidification	clastic and minor opaque	asteroid smaller than 100 km in diameter	none	75 % by volume	which depends on degree of aqueous alteration and thermal metamorphism	0.2 to 1 % by weight	anorthite-pigeonite Ca-rich	3	greater than 20 % by weight, kamacite and taenite in exsolution relationship	silicates (with very few exceptions)		1984	0.3 to 3 % by weight		4 Vesta	23	very rapid	0.7 millimeters	less than 0.5 % by weight	Howardite, Eucrite, Diogenite	coarse-grained orthopyroxenites, gabbros, fine- to coarse-grained basalts, brecciated