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 005 | 0.2 to 1 % by weight | | | | clastic and minor opaque | Ornans meteorite | DaG | none | 34 % by volume | | |
 | can be severe due to long exposure time to environmental corrosion agents | elemental carbon | minor primary grains only | 1 to 5 % by volume | 13 % by volume | 8 % of meteorite falls | | 0.15 millimeters | shock metamorphism | recorded by eyewitness or inferred from dating methods | W2 | | clear, isotropic, variable abundance | | | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | | 36 | 3 | 1995 | | 0.3 to 3 % by weight | | none | | rare relative to other chondrite types | DaG 005 | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | | often minerals not found on Earth | predominantly monoclinic | lower because the fall was not witnessed | 27° 09.39' N., 15° 57.15' E. | greater than 5 % deviations | 2577 kg | 48 % by volume | chondrules very sharply defined | | |
DaG 055 | in 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 agents | elemental carbon | usually plagioclase tectosilicate | in volume % | in volume % | 8 % of meteorite falls | | millimeters | shock metamorphism | recorded by eyewitness or inferred from dating methods | W1 | | | | | | | | 36 | | June 1995 | | in weight % | | | 0.451 kg | rare relative to other chondrite types | DaG 055 | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | | often minerals not found on Earth | definition goes here | lower because the fall was not witnessed | 27° 16.03' N., 16° 25.22' E. | | 2577 kg | in volume % | small sphere of about 1 mm diameter of formerly melted minerals | | |
DaG 275 | less than 0.2 % by weight | | the range over at which the alteration took place | | transparent, recrystallized, small crystals | ??? meteorite | DaG | | 75 % by volume | | |
 | can be severe due to long exposure time to environmental corrosion agents | elemental carbon | secondary, grains than 2 microns | 0.01 % by volume | 4 % by volume | | | 0.7 millimeters | shock metamorphism | recorded by eyewitness or inferred from dating methods | W4 | | devitrified, absent | | | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | | 1691 | 4 | 1997 | | less than 1.5 % by weight | | weak | | rare relative to other chondrite types | DaG 275 | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | | often minerals not found on Earth | greater than 20 % monoclinic | lower because the fall was not witnessed | 27° 21.74' N., 16° 05.38' E. | less than 5 % mean deviations | 485755 kg | 15 % by volume | chondrules well defined | | |
Dag 596 | less than 0.2 % by weight | amphoterite | the 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 grains | 2 % by volume | 0.1 to 1 % by volume | | | 0.9 millimeters | thermal metamorphism | recorded by eyewitness or inferred from dating methods | W1 | | devitrified, absent | | 1 | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | low | 9 | 5 | 1998 | | less than 1.5 % by weight | 20 % of total iron | moderate | 0.189 kg | most common chondrite observed from falls | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | LL5 chondrite | Fs% 22.5 | bronzite, olivine and minor oligoclase | less than 20 % monoclinic | lower because the fall was not witnessed | 27° 12.82' N. 16°16.89' E. | homogeneous | 184 kg | 60 to 80 % by volume | chondrules readily delineated | about 2 % | A. Sexton, Open University, UK. Meteoritical Bulletin No 83 |
Dag 597 | less than 0.2 % by weight | bronzite chondrite | the 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 grains | 10 % by volume | 0.1 to 1 % by volume | | | 0.3 millimeters | thermal metamorphism | recorded by eyewitness or inferred from dating methods | W2 | | devitrified, absent | | 1 | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | high | 76 | 5 | 1998 | contains small metal flakes | less than 1.5 % by weight | 75 % of total iron | moderate | 0.672 kg | most common chondrite observed from falls | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | H5 chondrite | Fs% 17.4 | often minerals not found on Earth | less than 20 % monoclinic | lower because the fall was not witnessed | 26° 50.15' N. 16° 37.59' E. | homogeneous | 1267 kg | 60 to 80 % by volume | chondrules readily delineated | 12 to 21 % | A. Sexton, Open University, UK. Meteoritical Bulletin No 83 |
DaG 600 | less than 0.2 % by weight | bronzite chondrite | the 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 grains | 10 % by volume | 0.1 to 1 % by volume | | | 0.3 millimeters | thermal metamorphism | recorded by eyewitness or inferred from dating methods | W2 | | devitrified, absent | | 1 | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | high | 76 | 5 | 1998 | | less than 1.5 % by weight | 75 % of total iron | moderate | 1.190 kg | most common chondrite observed from falls | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | H5 chondrite | Fs% 17.3 | often minerals not found on Earth | less than 20 % monoclinic | lower because the fall was not witnessed | 26° 54.98' N. 16° 40.49' E. | homogeneous | 1267 kg | 60 to 80 % by volume | chondrules readily delineated | 12 to 21 % | Open University, UK. Meteoritical Bulletin No 83 |
DaG 608 | less than 0.2 % by weight | hypersthene chondrite | the 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 microns | 5 % by volume | 0.1 to 1 % by volume | | | 0.7 millimeters | thermal metamorphism | recorded by eyewitness or inferred from dating methods | W3 | | devitrified, absent | | 1 | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | low | 155 | 6 | 1998 | shock veins | less than 1.5 % by weight | 50 % of total iron | strong | 1.870 kg | most common chondrite observed from falls | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | L6 chondrite | Fs% 21.5 | often minerals not found on Earth | orthorhombic | lower because the fall was not witnessed | 26° 58.22' N. 16° 21.65' E. | homogeneous | 4673 kg | 60 to 80 % by volume | chondrules poorly defined | 5 to 10 % | Open University, UK. Meteoritical Bulletin No 83 |
Dag 633 | less than 0.2 % by weight | amphoterite | the 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 grains | 2 % by volume | 0.1 to 1 % by volume | | | 0.9 millimeters | thermal metamorphism | recorded by eyewitness or inferred from dating methods | W2 | | devitrified, absent | | 1 | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | low | 9 | 5 | 1998 | contains angular fragments | less than 1.5 % by weight | 20 % of total iron | moderate | 0.210 kg | most common chondrite observed from falls | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | LL5 chondrite | Fs% 23.4 | bronzite, olivine and minor oligoclase | less than 20 % monoclinic | lower because the fall was not witnessed | 26° 55.14' N. 16° 40.65' E. | homogeneous | 184 kg | 60 to 80 % by volume | chondrules readily delineated | about 2 % | A. Sexton, Open University, UK. Meteoritical Bulletin No 84 |
DaG 734 | less than 0.2 % by weight | E chondrite | the range over at which the alteration took place | 0.45 mm | transparent, 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 microns | 15 % by volume | 0.1 to 1 % by volume | | zero | 0.6 millimeters | shock metamorphism | recorded by eyewitness or inferred from dating methods | W4 | | devitrified, absent | highly reduced with very little FeO | | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | low | 5 | 3 to 6 | Winter 1996/97 | | less than 1.5 % by weight | | weak | 1.378 kg | | DaG 734 | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | | often minerals not found on Earth | greater than 20 % monoclinic | lower because the fall was not witnessed | 27° 7.91' N., 16° 3' E. | less than 5 % mean deviations | 143 kg | 60 to 80 % by volume | chondrules well defined | | |
HaH 180 | in 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 tectosilicate | in volume % | in volume % | 85.7 % of meteorite falls | | millimeters | shock metamorphism | recorded by eyewitness or inferred from dating methods | W4 | | | | | | | | 3 | | April 1996 | | in weight % | | | 0.936 kg | | HaH 180 | Hammadah al Hamra | S2 shock stage chondrite | | often minerals not found on Earth | definition goes here | lower because the fall was not witnessed | 28° 36.21' N., 13° 18.04' E. | | 27 kg | in volume % | small sphere of about 1 mm diameter of formerly melted minerals | | |
Lahmada 011 | less than 0.2 % by weight | bronzite chondrite | the 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 grains | 10 % by volume | 0.1 to 1 % by volume | | | 0.3 millimeters | thermal metamorphism | recorded by eyewitness or inferred from dating methods | W1 | | devitrified, absent | | 1 | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | high | 76 | 5 | 1999 | | less than 1.5 % by weight | 75 % of total iron | moderate | 1.520 kg | most common chondrite observed from falls | based on the locale, region, or nearby town in which the fall occurred | Lahmada, western Sahara | H5 chondrite | Fs% 16.9 | often minerals not found on Earth | less than 20 % monoclinic | lower because the fall was not witnessed | 27° 13.82' N. 9°45.03' E. | homogeneous | 1267 kg | 60 to 80 % by volume | chondrules readily delineated | 12 to 21 % | Open University, UK. Meteoritical Bulletin No 84 |
Pillistfer | less than 0.2 % by weight | E chondrite | the 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 microns | 15 % by volume | 0.1 to 1 % by volume | | zero | 0.6 millimeters | shock metamorphism | 12:30 pm August 8, 1868 | | what witnesses saw or what was recorded by instruments | devitrified, absent | highly reduced with very little FeO | | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | low | 1691 | 3 to 6 | | | less than 1.5 % by weight | | strong | 23.25 kg | | Pillistfer | Aukoma, Kurla, Wahhe, and Sawiauk in Estonian SSR | S2 shock stage chondrite | | often minerals not found on Earth | orthorhombic | higher because the fall was witnessed | 58° 40' N., 25° 44' E. | homogeneous | 485755 kg | 60 to 80 % by volume | chondrules poorly defined | | |
Renazzo | 0.8 to 2.6 % by weight | | | | mostly fine, opaque | ??? meteorite | | moderate | 30 to 50 % by volume | | |
 | negligible due to quick recovery of meteorite before corrosion begins | elemental carbon | minor primary grains only | 5 to 8 % by volume | 0.5 % by volume | | | 0.7 millimeters | shock metamorphism | January 15, 1824 8:30 pm | | what witnesses saw or what was recorded by instruments | preserved | | | greater than 0.5 % by weight | less than 20 % by weight; taenite minor or absent | | 1691 | 2 | | | 2 to 16 % by weight | | | 10 kg | rare relative to other chondrite types | Renazzo | Renazzo, Italy | S2 shock stage chondrite | | often minerals not found on Earth | predominantly monoclinic | higher because the fall was witnessed | 44° 46' N., 11° 17' E. | greater than 5 % deviations | 485755 kg | 50 to 60 % by volume | chondrules very sharply defined | | |
Vigarano | 0.2 to 1 % by weight | CV3R chondrite | | | clastic and minor opaque | Vigarano meteorite | | weak | 40 % by volume | 3.3 | |
 | negligible due to quick recovery of meteorite before corrosion begins | elemental carbon | minor primary grains only | 0 to 5 % by volume | 10 % by volume | | | 1.0 millimeters | shock metamorphism | January 22, 1910 9:30 pm | | what witnesses saw or what was recorded by instruments | clear, isotropic, variable abundance | | | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | | 1691 | 3 | | | 0.3 to 3 % by weight | | none | 16 kg | rare relative to other chondrite types | Vigarano | Emilia, Italy | S2 shock stage chondrite | | often minerals not found on Earth | predominantly monoclinic | higher because the fall was witnessed | 44° 51' N., 11° 24' E. | greater than 5 % deviations | 485755 kg | 45 % by volume | chondrules very sharply defined | | |