medium shock ureilite Comparison Table

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rock > igneous rock > differentiated meteorite > differentiated achondrite > asteroidal achondrite > ureilite > medium shock ureilite

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medium shock ureilite comparison table

Subject is paired with has reference is an instance of has orthopyroxene composition has fall location has fall date has name has olivine composition has fall description has weather has acronym has texture has value has total mass of find has fall coordinate is a kind of has find date has mass has image has augite composition has origin has number of find has minor mineral has plagioclase has pigeonite composition has intergranular boundary has gain size has pyroxene content

Acfer 277 Baba et al (1993), Bland et al. (1992) meteorite find 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 Fo% 79 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 9.6 En% 73 curved meeting in triple junctions 1 mm 0.55, 0.33 in modal pyroxene/(pryroxene+olivine)

Asuka 87031 Yanai and Kojima (1995b) meteorite find 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 Fo% 79 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 7.5 En% 75 curved meeting in triple junctions 1 mm 0 in modal pyroxene/(pryroxene+olivine)

Dingo Pup Donga Berkley et. al (1980) meteorite find 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 Fo% 84 can be severe due to long exposure time to environmental corrosion agents size-sorted layers lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 Wo% 5.0 En% 81 euhedral, non-interlocking grains 0.5 in modal pyroxene/(pryroxene+olivine)

EET 83225 AMN 8-1 meteorite find 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 Fo% 87 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 10 En% 78 curved meeting in triple junctions 1 mm

euhedral ureilite 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 size-sorted layers 9 kg (out of date) in degrees, minutes and seconds of lattitude and longitude medium shock ureilite asteroid 6 (out of date) euhedral, non-interlocking grains

HaH 064 Weber and Bischoff (1996), Weber and Bischoff (1998) meteorite find Wo% 4.6 En% 77 Hammadah al Hamra recorded by eyewitness or inferred from dating methods based on the locale, region, or nearby town in which the fall occurred Fo% 78 can be severe due to long exposure time to environmental corrosion agents HaH bi-modal with extremely large 15mm crystals of low-Ca pyroxene poikilitically enclosing domains with ureilite texture lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found Wo% 32 En% 55 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0.65 in modal pyroxene/(pryroxene+olivine)

HaH 126 Weber and Bischoff (1996), Sexton et al. (1996), Chikami et al. (1997b) Hammadah al Hamra meteorite Hammadah al Hamra recorded by eyewitness or inferred from dating methods based on the locale, region, or nearby town in which the fall occurred Fo% 79 can be severe due to long exposure time to environmental corrosion agents HaH large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 9 kg (out of date) in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 6 (out of date) 0 % Wo% 8.4 En% 74 curved meeting in triple junctions 1 mm 0.3 in modal pyroxene/(pryroxene+olivine)

Hajma Hutchison (1977) meteorite find Hajmah, Oman recorded by eyewitness or inferred from dating methods Hajmah Fo% 85 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg 19° 55' N., 56° 15' E. 1958 0.596 kg
Wo% En% meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 9.0 En% 78 curved meeting in triple junctions 1 mm

Hughes 009 Wlotzka (1994), Goodrich (1998) meteorite find Wo% 4.9 En% 84 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 Fo% 87 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found Wo% 37 En% 56 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % curved meeting in triple junctions 1 mm 0.7 in modal pyroxene/(pryroxene+olivine)

Jalanash Weber and Bischoff (1998) meteorite find 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 Fo% 81 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 7.8 En% 75 curved meeting in triple junctions 1 mm 0.15 in modal pyroxene/(pryroxene+olivine)

Kenna Berkley et. al (1980) meteorite find Roosevelt County, New Mexico recorded by eyewitness or inferred from dating methods Kenna Fo% 79 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg 33° 54' N., 103° 33.2' W. February 1972 10.9 kg
meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 9.8 En% 72 curved meeting in triple junctions 1 mm 0.25 in modal pyroxene/(pryroxene+olivine)

Lahrauli Malhotra (1962), Bhandari et al. (1981) meteorite fall 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 Fo% 79 what witnesses saw or what was recorded by instruments negligible due to quick recovery of meteorite before corrosion begins large, anhedral olivine and pyroxene grains higher because the fall was witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 7.7 En% 74 curved meeting in triple junctions 1 mm

LEW 88774 Warren and Kallemeyn (1994), Prinz et. al (1994) meteorite find Wo% 4.2 En% 75 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 Fo% 75 can be severe due to long exposure time to environmental corrosion agents bi-modal with extremely large 15mm crystals of low-Ca pyroxene poikilitically enclosing domains with ureilite texture lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found Wo% 33 En% 53 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 6% chromite 0.83-0.87 in modal pyroxene/(pryroxene+olivine)

META 78008 Takeda et al. (1989) meteorite find Wo% 4.5 En% 76 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 Fo% 77 can be severe due to long exposure time to environmental corrosion agents bi-modal with extremely large 15mm crystals of low-Ca pyroxene poikilitically enclosing domains with ureilite texture lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found Wo% 32 En% 55 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 Wo% 16 En% 66 0.05, 0.37 in modal pyroxene/(pryroxene+olivine)

Novo Urei Berkley et. al (1980) meteorite fall 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 Fo% 79 what witnesses saw or what was recorded by instruments negligible due to quick recovery of meteorite before corrosion begins large, anhedral olivine and pyroxene grains higher because the fall was witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 10 En% 72 curved meeting in triple junctions 1 mm 0.31 in modal pyroxene/(pryroxene+olivine)

QUE 93336 QUE 93341 meteorite AMN 18-1 meteorite find 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 Fo% 77 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 10 En% 72 curved meeting in triple junctions 1 mm

Y-790981 Goodrich et al. (1987b), Berkley (1986), Takeda (1987) meteorite find 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 Fo% 78 can be severe due to long exposure time to environmental corrosion agents large, anhedral olivine and pyroxene grains lower because the fall was not witnessed 485755 kg in degrees, minutes and seconds of lattitude and longitude when the meteorite was found meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 0 % Wo% 8.9 En% 73 curved meeting in triple junctions 1 mm 0.11 in modal pyroxene/(pryroxene+olivine)

Next S4 shock stage meteorite: S4 shock stage chondrite Up: S4 shock stage meteorite, S5 shock stage meteorite, S6 shock stage meteorite, ureilite

Subject	is paired with	has reference	is an instance of	has orthopyroxene composition	has fall location	has fall date	has name	has olivine composition	has fall description	has weather	has acronym	has texture	has value	has total mass of find	has fall coordinate	is a kind of	has find date	has mass	has image	has augite composition	has origin	has number of find	has minor mineral	has plagioclase	has pigeonite composition	has intergranular boundary	has gain size	has pyroxene content
Acfer 277		Baba et al (1993), Bland et al. (1992)	meteorite find		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	Fo% 79		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 9.6 En% 73	curved meeting in triple junctions	1 mm	0.55, 0.33 in modal pyroxene/(pryroxene+olivine)
Asuka 87031		Yanai and Kojima (1995b)	meteorite find		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	Fo% 79		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 7.5 En% 75	curved meeting in triple junctions	1 mm	0 in modal pyroxene/(pryroxene+olivine)
Dingo Pup Donga		Berkley et. al (1980)	meteorite find		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	Fo% 84		can be severe due to long exposure time to environmental corrosion agents		size-sorted layers	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691			Wo% 5.0 En% 81	euhedral, non-interlocking grains		0.5 in modal pyroxene/(pryroxene+olivine)
EET 83225		AMN 8-1	meteorite find		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	Fo% 87		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 10 En% 78	curved meeting in triple junctions	1 mm
euhedral ureilite					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					size-sorted layers		9 kg (out of date)	in degrees, minutes and seconds of lattitude and longitude	medium shock ureilite					asteroid	6 (out of date)				euhedral, non-interlocking grains
HaH 064		Weber and Bischoff (1996), Weber and Bischoff (1998)	meteorite find	Wo% 4.6 En% 77	Hammadah al Hamra	recorded by eyewitness or inferred from dating methods	based on the locale, region, or nearby town in which the fall occurred	Fo% 78		can be severe due to long exposure time to environmental corrosion agents	HaH	bi-modal with extremely large 15mm crystals of low-Ca pyroxene poikilitically enclosing domains with ureilite texture	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found			Wo% 32 En% 55	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691						0.65 in modal pyroxene/(pryroxene+olivine)
HaH 126		Weber and Bischoff (1996), Sexton et al. (1996), Chikami et al. (1997b)	Hammadah al Hamra meteorite		Hammadah al Hamra	recorded by eyewitness or inferred from dating methods	based on the locale, region, or nearby town in which the fall occurred	Fo% 79		can be severe due to long exposure time to environmental corrosion agents	HaH	large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	9 kg (out of date)	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	6 (out of date)		0 %	Wo% 8.4 En% 74	curved meeting in triple junctions	1 mm	0.3 in modal pyroxene/(pryroxene+olivine)
Hajma		Hutchison (1977)	meteorite find		Hajmah, Oman	recorded by eyewitness or inferred from dating methods	Hajmah	Fo% 85		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	19° 55' N., 56° 15' E.		1958	0.596 kg		Wo% En%	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 9.0 En% 78	curved meeting in triple junctions	1 mm
Hughes 009		Wlotzka (1994), Goodrich (1998)	meteorite find	Wo% 4.9 En% 84	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	Fo% 87		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found			Wo% 37 En% 56	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %		curved meeting in triple junctions	1 mm	0.7 in modal pyroxene/(pryroxene+olivine)
Jalanash		Weber and Bischoff (1998)	meteorite find		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	Fo% 81		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 7.8 En% 75	curved meeting in triple junctions	1 mm	0.15 in modal pyroxene/(pryroxene+olivine)
Kenna		Berkley et. al (1980)	meteorite find		Roosevelt County, New Mexico	recorded by eyewitness or inferred from dating methods	Kenna	Fo% 79		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	33° 54' N., 103° 33.2' W.		February 1972	10.9 kg			meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 9.8 En% 72	curved meeting in triple junctions	1 mm	0.25 in modal pyroxene/(pryroxene+olivine)
Lahrauli		Malhotra (1962), Bhandari et al. (1981)	meteorite fall		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	Fo% 79	what witnesses saw or what was recorded by instruments	negligible due to quick recovery of meteorite before corrosion begins		large, anhedral olivine and pyroxene grains	higher because the fall was witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude						meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 7.7 En% 74	curved meeting in triple junctions	1 mm
LEW 88774		Warren and Kallemeyn (1994), Prinz et. al (1994)	meteorite find	Wo% 4.2 En% 75	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	Fo% 75		can be severe due to long exposure time to environmental corrosion agents		bi-modal with extremely large 15mm crystals of low-Ca pyroxene poikilitically enclosing domains with ureilite texture	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found			Wo% 33 En% 53	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691	6% chromite					0.83-0.87 in modal pyroxene/(pryroxene+olivine)
META 78008		Takeda et al. (1989)	meteorite find	Wo% 4.5 En% 76	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	Fo% 77		can be severe due to long exposure time to environmental corrosion agents		bi-modal with extremely large 15mm crystals of low-Ca pyroxene poikilitically enclosing domains with ureilite texture	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found			Wo% 32 En% 55	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691			Wo% 16 En% 66			0.05, 0.37 in modal pyroxene/(pryroxene+olivine)
Novo Urei		Berkley et. al (1980)	meteorite fall		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	Fo% 79	what witnesses saw or what was recorded by instruments	negligible due to quick recovery of meteorite before corrosion begins		large, anhedral olivine and pyroxene grains	higher because the fall was witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude						meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 10 En% 72	curved meeting in triple junctions	1 mm	0.31 in modal pyroxene/(pryroxene+olivine)
QUE 93336	QUE 93341 meteorite	AMN 18-1	meteorite find		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	Fo% 77		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 10 En% 72	curved meeting in triple junctions	1 mm
Y-790981		Goodrich et al. (1987b), Berkley (1986), Takeda (1987)	meteorite find		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	Fo% 78		can be severe due to long exposure time to environmental corrosion agents		large, anhedral olivine and pyroxene grains	lower because the fall was not witnessed	485755 kg	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found				meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691		0 %	Wo% 8.9 En% 73	curved meeting in triple junctions	1 mm	0.11 in modal pyroxene/(pryroxene+olivine)