low shock ureilite Comparison Table

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

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low shock ureilite comparison table

Subject is paired with has olivine inclusion has sediment mechanism has reference has degree of shock metamorphism has shock stage is an instance of has orthopyroxene composition has fall location has name has olivine composition has weather has weathering stage has acronym has texture has value has total mass of find has pronunciation has matrix composition has fall coordinate is a kind of has find date has mass has image has augite composition has origin has number of find has shock pressure has lithic clast composition has plagioclase has pigeonite composition has intergranular boundary has gain size has pyroxene content has pyroxene inclusion

ALHA 77257 Goodrich et al. (1987b), Goodrich and Berkley (1986), Berkley and Jones (1982) low S2-S3 meteorite find 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 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 6.8 En% 80 curved meeting in triple junctions 1 mm 0.16 in modal pyroxene/(pryroxene+olivine)

ALHA 78262 Goodrich et al. (1987b), Goodrich and Berkley (1986), Berkley and Jones (1982) low S2-S3 meteorite find 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 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 8.4 En% 72 curved meeting in triple junctions 1 mm

Asuka 881931 Yanai and Kojima (1995b) low S2-S3 meteorite find 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 Fo% 76 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 8.8 En% 73 curved meeting in triple junctions 1 mm

DaG 319 unshocked S1 S1 shock stage meteorite Dar al Gani plateau, Libyan Sahara Desert DaG 319 can be severe due to long exposure time to environmental corrosion agents W2 DaG lower because the fall was not witnessed 9 kg (out of date) bre - chia smaller mineral fragments, carbon, suessite (Fe3Si), sulfides, minor chromite and minor apatite 27° 01.68' N., 16° 21.52' E. 1997 0.740 kg
meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 6 (out of date) less than 5 GPa typical monomict ureilite material plus a variety of other lithic clasts common in clasts

EET 87511 EET 87717 meteorite Berkley (1990), AMN 11-2 low S2-S3 meteorite find Wo% 4.5 En% 82 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 Fo% 85 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume in degrees, minutes and seconds of lattitude and longitude when the meteorite was found Wo% 36 En% 55 meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal 1691 less than 20 GPa

EET 87517 AMN 11-2 low S2-S3 meteorite find 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 Fo% 92 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 5.0 En% 87 curved meeting in triple junctions 1 mm 0.5 in modal pyroxene/(pryroxene+olivine)

LEW 85328 AMN 10-1 low S2-S3 meteorite find 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 Fo% 80 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 9.0 En% 74 curved meeting in triple junctions 1 mm 0.33 in modal pyroxene/(pryroxene+olivine)

LEW 88006 AMN 13-2 low S2-S3 meteorite find 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 Fo% 82 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 8.0 En% 76 curved meeting in triple junctions 1 mm

monomict-poikilitic ureilite small rounded pyroxene grains (poikilitic) low S2-S3 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 large, anhedral olivine and pyroxene grains 9 kg (out of date) carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume in degrees, minutes and seconds of lattitude and longitude low shock ureilite asteroid 6 (out of date) less than 20 GPa 0 % curved meeting in triple junctions 1 mm small rounded olivine grains (poikilitic)

Roosevelt County 027 Goodrich et al. (1987a) low S2-S3 meteorite find 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 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 8.0 En% 75 curved meeting in triple junctions 1 mm 0.25 in modal pyroxene/(pryroxene+olivine)

Y-74659 Takeda et al. (1979a), Takeda (1987), Takeda and Yanai (1978) low S2-S3 meteorite find Wo% 4.5 En% 88 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 Fo% 91 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 7.3 En% 86 curved meeting in triple junctions 1 mm 0.52 in modal pyroxene/(pryroxene+olivine)

Y-791538 Yanai and Kojima (1995b), Takeda et al. (1992), Takeda (1989) low S2-S3 meteorite find Wo% 4.9 En% 88 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 Fo% 91 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 9.0 En% 84 curved meeting in triple junctions 1 mm 0.45 in modal pyroxene/(pryroxene+olivine)

Y-82100 Yanai and Kojima (1995b) low S2-S3 meteorite find 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 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % Wo% 8.6 En% 77 curved meeting in triple junctions 1 mm 0.2 in modal pyroxene/(pryroxene+olivine)

Y-8448 Yanai and Kojima (1995b) low S2-S3 meteorite find 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 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 carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume 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 less than 20 GPa 0 % variable curved meeting in triple junctions 1 mm

Next S2 shock stage meteorite: S2 shock stage chondrite Up: S2 shock stage meteorite, S3 shock stage meteorite, ureilite

Subject	is paired with	has olivine inclusion	has sediment mechanism	has reference	has degree of shock metamorphism	has shock stage	is an instance of	has orthopyroxene composition	has fall location	has name	has olivine composition	has weather	has weathering stage	has acronym	has texture	has value	has total mass of find	has pronunciation	has matrix composition	has fall coordinate	is a kind of	has find date	has mass	has image	has augite composition	has origin	has number of find	has shock pressure	has lithic clast composition	has plagioclase	has pigeonite composition	has intergranular boundary	has gain size	has pyroxene content	has pyroxene inclusion
ALHA 77257				Goodrich et al. (1987b), Goodrich and Berkley (1986), Berkley and Jones (1982)	low	S2-S3	meteorite find		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	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 6.8 En% 80	curved meeting in triple junctions	1 mm	0.16 in modal pyroxene/(pryroxene+olivine)
ALHA 78262				Goodrich et al. (1987b), Goodrich and Berkley (1986), Berkley and Jones (1982)	low	S2-S3	meteorite find		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	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 8.4 En% 72	curved meeting in triple junctions	1 mm
Asuka 881931				Yanai and Kojima (1995b)	low	S2-S3	meteorite find		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	Fo% 76	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 8.8 En% 73	curved meeting in triple junctions	1 mm
DaG 319					unshocked	S1	S1 shock stage meteorite		Dar al Gani plateau, Libyan Sahara Desert	DaG 319		can be severe due to long exposure time to environmental corrosion agents	W2	DaG		lower because the fall was not witnessed	9 kg (out of date)	bre - chia	smaller mineral fragments, carbon, suessite (Fe3Si), sulfides, minor chromite and minor apatite	27° 01.68' N., 16° 21.52' E.		1997	0.740 kg			meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	6 (out of date)	less than 5 GPa	typical monomict ureilite material plus a variety of other lithic clasts	common in clasts
EET 87511	EET 87717 meteorite			Berkley (1990), AMN 11-2	low	S2-S3	meteorite find	Wo% 4.5 En% 82	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	Fo% 85	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	in degrees, minutes and seconds of lattitude and longitude		when the meteorite was found			Wo% 36 En% 55	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	1691	less than 20 GPa
EET 87517				AMN 11-2	low	S2-S3	meteorite find		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	Fo% 92	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 5.0 En% 87	curved meeting in triple junctions	1 mm	0.5 in modal pyroxene/(pryroxene+olivine)
LEW 85328				AMN 10-1	low	S2-S3	meteorite find		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	Fo% 80	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 9.0 En% 74	curved meeting in triple junctions	1 mm	0.33 in modal pyroxene/(pryroxene+olivine)
LEW 88006				AMN 13-2	low	S2-S3	meteorite find		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	Fo% 82	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 8.0 En% 76	curved meeting in triple junctions	1 mm
monomict-poikilitic ureilite		small rounded pyroxene grains (poikilitic)			low	S2-S3			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					large, anhedral olivine and pyroxene grains		9 kg (out of date)		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	in degrees, minutes and seconds of lattitude and longitude	low shock ureilite					asteroid	6 (out of date)	less than 20 GPa		0 %		curved meeting in triple junctions	1 mm		small rounded olivine grains (poikilitic)
Roosevelt County 027				Goodrich et al. (1987a)	low	S2-S3	meteorite find		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	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 8.0 En% 75	curved meeting in triple junctions	1 mm	0.25 in modal pyroxene/(pryroxene+olivine)
Y-74659				Takeda et al. (1979a), Takeda (1987), Takeda and Yanai (1978)	low	S2-S3	meteorite find	Wo% 4.5 En% 88	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	Fo% 91	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 7.3 En% 86	curved meeting in triple junctions	1 mm	0.52 in modal pyroxene/(pryroxene+olivine)
Y-791538				Yanai and Kojima (1995b), Takeda et al. (1992), Takeda (1989)	low	S2-S3	meteorite find	Wo% 4.9 En% 88	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	Fo% 91	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 9.0 En% 84	curved meeting in triple junctions	1 mm	0.45 in modal pyroxene/(pryroxene+olivine)
Y-82100				Yanai and Kojima (1995b)	low	S2-S3	meteorite find		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	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	Wo% 8.6 En% 77	curved meeting in triple junctions	1 mm	0.2 in modal pyroxene/(pryroxene+olivine)
Y-8448				Yanai and Kojima (1995b)	low	S2-S3	meteorite find		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	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		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume	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	less than 20 GPa		0 %	variable	curved meeting in triple junctions	1 mm