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rock > metamorphic rock > altered chondrite > shocked chondrite > S2 shock stage chondrite
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S2 shock stage chondrite comparison table
Subject has part carbon has synonym has alteration temperature range has chodrule size has part matrix has prototype has acronym has degree of aqueous alteration has matrix abundance has petrologic subtype has olivine composition has image has weather has distinguishing feature has part feldspar has metal abundance has refractory inclusion abundance has relative abundance has oxidized iron content has chondrule mean diameter has metamorphism mechanism has fall date has weathering stage has fall description has chondrule glass type has oxidation state has number of fragment has part sulfide Ni content has part maximum bulk Ni in metal has total iron content has number of find has petrologic type has find date has comment has part water has iron metal and iron sulfide has degree of thermal metamorphism has mass has abundance has name has fall location is an instance of has pyroxene composition has composition has structural state of low Ca pyroxene has value has fall coordinate has olivine and low Ca pyroxene homogeneity has total mass of find has chondrule abundance has part chondrule has metal iron content classified by
DaG 0050.2 to 1 % by weight   clastic and minor opaqueOrnans meteoriteDaGnone34 % by volume  
can be severe due to long exposure time to environmental corrosion agentselemental carbonminor primary grains only1 to 5 % by volume13 % by volume8 % of meteorite falls 0.15 millimetersshock metamorphismrecorded by eyewitness or inferred from dating methodsW2 clear, isotropic, variable abundance  less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationship 3631995 0.3 to 3 % by weight none rare relative to other chondrite typesDaG 005Dar al Gani plateau, Libyan Sahara DesertS2 shock stage chondrite often minerals not found on Earthpredominantly monocliniclower because the fall was not witnessed27° 09.39' N., 15° 57.15' E.greater than 5 % deviations2577 kg48 % by volumechondrules very sharply defined  
DaG 055in weight %   fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents DaG in volume %3 
can be severe due to long exposure time to environmental corrosion agentselemental carbonusually plagioclase tectosilicatein volume %in volume %8 % of meteorite falls millimetersshock metamorphismrecorded by eyewitness or inferred from dating methodsW1       36 June 1995 in weight %  0.451 kgrare relative to other chondrite typesDaG 055Dar al Gani plateau, Libyan Sahara DesertS2 shock stage chondrite often minerals not found on Earthdefinition goes herelower because the fall was not witnessed27° 16.03' N., 16° 25.22' E. 2577 kgin volume %small sphere of about 1 mm diameter of formerly melted minerals  
DaG 275less than 0.2 % by weight the range over at which the alteration took place transparent, recrystallized, small crystals??? meteoriteDaG 75 % by volume  
can be severe due to long exposure time to environmental corrosion agentselemental carbonsecondary, grains than 2 microns0.01 % by volume4 % by volume  0.7 millimetersshock metamorphismrecorded by eyewitness or inferred from dating methodsW4 devitrified, absent  less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationship 169141997 less than 1.5 % by weight weak rare relative to other chondrite typesDaG 275Dar al Gani plateau, Libyan Sahara DesertS2 shock stage chondrite often minerals not found on Earthgreater than 20 % monocliniclower because the fall was not witnessed27° 21.74' N., 16° 05.38' E.less than 5 % mean deviations485755 kg15 % by volumechondrules well defined  
Dag 596less than 0.2 % by weightamphoteritethe range over at which the alteration took place transparent, recrystallized, moderate size crystals DaG 10 to 15 % by volume Fa% 29.6
can be severe due to long exposure time to environmental corrosion agents secondary, 2 to 50 micron grains2 % by volume0.1 to 1 % by volume  0.9 millimetersthermal metamorphismrecorded by eyewitness or inferred from dating methodsW1 devitrified, absent 1less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiplow951998 less than 1.5 % by weight20 % of total ironmoderate0.189 kgmost common chondrite observed from fallsbased on the locale, region, or nearby town in which the fall occurredDar al Gani plateau, Libyan Sahara DesertLL5 chondriteFs% 22.5bronzite, olivine and minor oligoclaseless than 20 % monocliniclower because the fall was not witnessed27° 12.82' N. 16°16.89' E.homogeneous184 kg60 to 80 % by volumechondrules readily delineatedabout 2 %A. Sexton, Open University, UK. Meteoritical Bulletin No 83
Dag 597less than 0.2 % by weightbronzite chondritethe range over at which the alteration took place transparent, recrystallized, moderate size crystals DaG 10 to 15 % by volume Fa% 19.9
can be severe due to long exposure time to environmental corrosion agents secondary, 2 to 50 micron grains10 % by volume0.1 to 1 % by volume  0.3 millimetersthermal metamorphismrecorded by eyewitness or inferred from dating methodsW2 devitrified, absent 1less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiphigh7651998contains small metal flakesless than 1.5 % by weight75 % of total ironmoderate0.672 kgmost common chondrite observed from fallsbased on the locale, region, or nearby town in which the fall occurredDar al Gani plateau, Libyan Sahara DesertH5 chondriteFs% 17.4often minerals not found on Earthless than 20 % monocliniclower because the fall was not witnessed26° 50.15' N. 16° 37.59' E.homogeneous1267 kg60 to 80 % by volumechondrules readily delineated12 to 21 %A. Sexton, Open University, UK. Meteoritical Bulletin No 83
DaG 600less than 0.2 % by weightbronzite chondritethe range over at which the alteration took place transparent, recrystallized, moderate size crystals DaG 10 to 15 % by volume Fa% 19.5
can be severe due to long exposure time to environmental corrosion agents secondary, 2 to 50 micron grains10 % by volume0.1 to 1 % by volume  0.3 millimetersthermal metamorphismrecorded by eyewitness or inferred from dating methodsW2 devitrified, absent 1less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiphigh7651998 less than 1.5 % by weight75 % of total ironmoderate1.190 kgmost common chondrite observed from fallsbased on the locale, region, or nearby town in which the fall occurredDar al Gani plateau, Libyan Sahara DesertH5 chondriteFs% 17.3often minerals not found on Earthless than 20 % monocliniclower because the fall was not witnessed26° 54.98' N. 16° 40.49' E.homogeneous1267 kg60 to 80 % by volumechondrules readily delineated12 to 21 %Open University, UK. Meteoritical Bulletin No 83
DaG 608less than 0.2 % by weighthypersthene chondritethe range over at which the alteration took place transparent, recrystallized, coarse crystals DaG 10 to 15 % by volume Fa% 25.1
can be severe due to long exposure time to environmental corrosion agents secondary, grains greater than 50 microns5 % by volume0.1 to 1 % by volume  0.7 millimetersthermal metamorphismrecorded by eyewitness or inferred from dating methodsW3 devitrified, absent 1less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiplow15561998shock veinsless than 1.5 % by weight50 % of total ironstrong1.870 kgmost common chondrite observed from fallsbased on the locale, region, or nearby town in which the fall occurredDar al Gani plateau, Libyan Sahara DesertL6 chondriteFs% 21.5often minerals not found on Earthorthorhombiclower because the fall was not witnessed26° 58.22' N. 16° 21.65' E.homogeneous4673 kg60 to 80 % by volumechondrules poorly defined5 to 10 %Open University, UK. Meteoritical Bulletin No 83
Dag 633less than 0.2 % by weightamphoteritethe range over at which the alteration took place transparent, recrystallized, moderate size crystals DaG 10 to 15 % by volume Fa% 27.1
can be severe due to long exposure time to environmental corrosion agents secondary, 2 to 50 micron grains2 % by volume0.1 to 1 % by volume  0.9 millimetersthermal metamorphismrecorded by eyewitness or inferred from dating methodsW2 devitrified, absent 1less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiplow951998contains angular fragmentsless than 1.5 % by weight20 % of total ironmoderate0.210 kgmost common chondrite observed from fallsbased on the locale, region, or nearby town in which the fall occurredDar al Gani plateau, Libyan Sahara DesertLL5 chondriteFs% 23.4bronzite, olivine and minor oligoclaseless than 20 % monocliniclower because the fall was not witnessed26° 55.14' N. 16° 40.65' E.homogeneous184 kg60 to 80 % by volumechondrules readily delineatedabout 2 %A. Sexton, Open University, UK. Meteoritical Bulletin No 84
DaG 734less than 0.2 % by weightE chondritethe range over at which the alteration took place0.45 mmtransparent, recrystallized, small crystals DaG less than 2 to 15 % by volume  
can be severe due to long exposure time to environmental corrosion agents secondary, grains than 2 microns15 % by volume0.1 to 1 % by volume zero0.6 millimetersshock metamorphismrecorded by eyewitness or inferred from dating methodsW4 devitrified, absenthighly reduced with very little FeO less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiplow53 to 6Winter 1996/97 less than 1.5 % by weight weak1.378 kg DaG 734Dar al Gani plateau, Libyan Sahara DesertS2 shock stage chondrite often minerals not found on Earthgreater than 20 % monocliniclower because the fall was not witnessed27° 7.91' N., 16° 3' E.less than 5 % mean deviations143 kg60 to 80 % by volumechondrules well defined  
HaH 180in weight %   fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents HaH in volume %  
can be severe due to long exposure time to environmental corrosion agents usually plagioclase tectosilicatein volume %in volume %85.7 % of meteorite falls millimetersshock metamorphismrecorded by eyewitness or inferred from dating methodsW4       3 April 1996 in weight %  0.936 kg HaH 180Hammadah al HamraS2 shock stage chondrite often minerals not found on Earthdefinition goes herelower because the fall was not witnessed28° 36.21' N., 13° 18.04' E. 27 kgin volume %small sphere of about 1 mm diameter of formerly melted minerals  
Lahmada 011less than 0.2 % by weightbronzite chondritethe range over at which the alteration took place transparent, recrystallized, moderate size crystals DaG 10 to 15 % by volume Fa% 19.3
can be severe due to long exposure time to environmental corrosion agents secondary, 2 to 50 micron grains10 % by volume0.1 to 1 % by volume  0.3 millimetersthermal metamorphismrecorded by eyewitness or inferred from dating methodsW1 devitrified, absent 1less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiphigh7651999 less than 1.5 % by weight75 % of total ironmoderate1.520 kgmost common chondrite observed from fallsbased on the locale, region, or nearby town in which the fall occurredLahmada, western SaharaH5 chondriteFs% 16.9often minerals not found on Earthless than 20 % monocliniclower because the fall was not witnessed27° 13.82' N. 9°45.03' E.homogeneous1267 kg60 to 80 % by volumechondrules readily delineated12 to 21 %Open University, UK. Meteoritical Bulletin No 84
Pillistferless than 0.2 % by weightE chondritethe range over at which the alteration took place transparent, recrystallized, coarse crystals   less than 2 to 15 % by volume  
negligible due to quick recovery of meteorite before corrosion begins secondary, grains greater than 50 microns15 % by volume0.1 to 1 % by volume zero0.6 millimetersshock metamorphism12:30 pm August 8, 1868 what witnesses saw or what was recorded by instrumentsdevitrified, absenthighly reduced with very little FeO less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationshiplow16913 to 6  less than 1.5 % by weight strong23.25 kg PillistferAukoma, Kurla, Wahhe, and Sawiauk in Estonian SSRS2 shock stage chondrite often minerals not found on Earthorthorhombichigher because the fall was witnessed58° 40' N., 25° 44' E.homogeneous485755 kg60 to 80 % by volumechondrules poorly defined  
Renazzo0.8 to 2.6 % by weight   mostly fine, opaque??? meteorite moderate30 to 50 % by volume  
negligible due to quick recovery of meteorite before corrosion beginselemental carbonminor primary grains only5 to 8 % by volume0.5 % by volume  0.7 millimetersshock metamorphismJanuary 15, 1824 8:30 pm what witnesses saw or what was recorded by instrumentspreserved  greater than 0.5 % by weightless than 20 % by weight; taenite minor or absent 16912  2 to 16 % by weight  10 kgrare relative to other chondrite typesRenazzoRenazzo, ItalyS2 shock stage chondrite often minerals not found on Earthpredominantly monoclinichigher because the fall was witnessed44° 46' N., 11° 17' E.greater than 5 % deviations485755 kg50 to 60 % by volumechondrules very sharply defined  
Vigarano0.2 to 1 % by weightCV3R chondrite  clastic and minor opaqueVigarano meteorite weak40 % by volume3.3 
negligible due to quick recovery of meteorite before corrosion beginselemental carbonminor primary grains only0 to 5 % by volume10 % by volume  1.0 millimetersshock metamorphismJanuary 22, 1910 9:30 pm what witnesses saw or what was recorded by instrumentsclear, isotropic, variable abundance  less than 0.5 % by weightgreater than 20 % by weight, kamacite and taenite in exsolution relationship 16913  0.3 to 3 % by weight none16 kgrare relative to other chondrite typesVigaranoEmilia, ItalyS2 shock stage chondrite often minerals not found on Earthpredominantly monoclinichigher because the fall was witnessed44° 51' N., 11° 24' E.greater than 5 % deviations485755 kg45 % by volumechondrules very sharply defined  

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