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S1 shock stage meteorite comparison table

Subject	has part mean Ni content of sulfide	has pronunciation	has solidification timescale	has part carbon	has olivine shock metamorphism	has part matrix	has prototype	is independent of	has acronym	has matrix abundance	has shock texture	has letter designation	has sediment mechanism	has origin	has likely origin	has inclusion minerology	has image	has weather	has distinguishing feature	has part feldspar	has degree of secondary process	has metal abundance	has refractory inclusion abundance	has solidification mechanism	has chondrule mean diameter	has petrology	has weathering stage	is a kind of	has chondrule glass type	has age	has number of find	has find date	has part water	has plagioclase	has orthopyroxene shock metamorphism	has plagioclase shock metamorphism	has characteristic mineral	has mass	has peak temperature	has shock diagnostic mineral	has name	be shock	has fall location	is an instance of	has part metal maximum bulk	has homogeneity of olivine and low Ca pyroxene	has lithic clast composition	has composition	has structural state of low Ca pyroxene	has matrix composition	has value	has fall coordinate	has minerology	has total mass of find	has chondrule abundance	has parent body	has part chondrule	has olivine grain characteristic	has petrologic type range
DaG 319		bre - chia	very slow		fracturing, undulatory extinction and kink bands				DaG		silicates show minor fracturing, undulatory extinction and kink bands primarily in olivine	AURE		meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	partial melting residue			can be severe due to long exposure time to environmental corrosion agents	no chondrules					cooling in deep underground chambers		coarse-grained granular	W2				6 (out of date)	1997		common in clasts			olivine-pigeonite about 90% by volume	0.740 kg		small euhedral graphite crystals can sometimes be distinguished	DaG 319		Dar al Gani plateau, Libyan Sahara Desert	S1 shock stage meteorite			typical monomict ureilite material plus a variety of other lithic clasts	often minerals not found on Earth		smaller mineral fragments, carbon, suessite (Fe3Si), sulfides, minor chromite and minor apatite	lower because the fall was not witnessed	27° 01.68' N., 16° 21.52' E.	olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite)	9 kg (out of date)				reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal
HaH 193							Winona meteorite		HaH				agglomeration of particles, many of which record individual, diverse histories	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal	ultrametamorphism, partial melting with some melt migration	troilite, metal, daubreilite, schreibersite, graphite		can be severe due to long exposure time to environmental corrosion agents	no chondrules							fine- to coarse-grained equigranular	W3			oldest and most primitive rock in solar system	1691	October 1996						0.259 kg	less than 950 degree Celsius during its entire history since solidification		HaH 193		Hammadah al Hamra	S1 shock stage meteorite				IAB-silica related			lower because the fall was not witnessed	28° 39.28' N., 13° 27.52' E.	olivine, orthopyroxene, clinopyroxene, metal with some troilite and some sodic plagioclase	485755 kg		asteroid smaller than 100 km in diameter
S1 shock stage chondrite	in weight %			in weight %	sharp optical extinction, irregular fractures	fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents		the nature and degree of thermal metamorphism or aqueous alteration		in volume %			agglomeration of particles, many of which record individual, diverse histories	meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal						usually plagioclase tectosilicate	providing insight into geological evolution of parent asteroid	in volume %	in volume %		millimeters			S1 shock stage meteorite		oldest and most primitive rock in solar system	1691		in weight %		sharp optical extinction, irregular fractures	sharp optical extinction, irregular fractures			less than 950 degree Celsius during its entire history since solidification	orthopyroxene for enstatite chondrite	based on the locale, region, or nearby town in which the fall occurred	before, during or after other types of metamorphism	strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity		in weight %	definition goes here		often minerals not found on Earth	definition goes here			in degrees, minutes and seconds of lattitude and longitude		485755 kg	in volume %	asteroid smaller than 100 km in diameter	small sphere of about 1 mm diameter of formerly melted minerals		which depends on degree of aqueous alteration and thermal metamorphism
very low shock ureilite			very slow									AURE		asteroid	partial melting residue				no chondrules					cooling in deep underground chambers		coarse-grained granular		S1 shock stage meteorite			6 (out of date)						olivine-pigeonite about 90% by volume			no diamonds or lonsdaleite	based on the locale, region, or nearby town in which the fall occurred		strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity					often minerals not found on Earth		carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume		in degrees, minutes and seconds of lattitude and longitude	olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite)	9 kg (out of date)				reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal

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