Subject |
has weather resistance |
has olivine shock metamorphism |
is independent of |
has shock pressure |
has acronym |
has olivine composition |
has image |
has weather |
has relative abundance |
has fragmentation probability |
has metamorphism mechanism |
has weathering stage |
has number of fragment |
has find date |
has comment |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has degree of shock metamorphism |
has mass |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has pyroxene composition |
has shock stage |
has composition |
has value |
has fall coordinate |
has ablative mass loss |
classified by |
DaG 222 | which depends on its composition | planar fractures, undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 15 to 20 GPa | DaG | |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | shock metamorphism | W3 | | 1996 | breccia | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | weakly shocked | 0.837 kg | orthopyroxene for enstatite chondrite | DaG 222 | before, during or after other types of metamorphism | Dar al Gani plateau, Libyan Sahara Desert | S3 shock stage chondrite | | S3 | bronzite, olivine and minor oligoclase | lower because the fall was not witnessed | 27° 27.20' N., 16° 18.76' E. | directly proportional to initial velocity | |
Dag 596 | which depends on its composition | undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 5 to 10 GPa | DaG | Fa% 29.6 |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | thermal metamorphism | W1 | 1 | 1998 | | undulatory extinction, irregular fractures, some planar fractures | undulatory extinction, irregular fractures | very weakly shocked | 0.189 kg | 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 | Dar al Gani plateau, Libyan Sahara Desert | LL5 chondrite | Fs% 22.5 | S2 | bronzite, olivine and minor oligoclase | lower because the fall was not witnessed | 27° 12.82' N. 16°16.89' E. | directly proportional to initial velocity | A. Sexton, Open University, UK. Meteoritical Bulletin No 83 |
Dag 633 | which depends on its composition | undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 5 to 10 GPa | DaG | Fa% 27.1 |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | thermal metamorphism | W2 | 1 | 1998 | contains angular fragments | undulatory extinction, irregular fractures, some planar fractures | undulatory extinction, irregular fractures | very weakly shocked | 0.210 kg | 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 | Dar al Gani plateau, Libyan Sahara Desert | LL5 chondrite | Fs% 23.4 | S2 | bronzite, olivine and minor oligoclase | lower because the fall was not witnessed | 26° 55.14' N. 16° 40.65' E. | directly proportional to initial velocity | A. Sexton, Open University, UK. Meteoritical Bulletin No 84 |
DaG 639 | which depends on its composition | planar fractures, undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 15 to 20 GPa | DaG | Fa% 26.8 |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | thermal metamorphism | W2 | 1 | 1998 | | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | weakly shocked | 0.237 kg | 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 | Dar al Gani plateau, Libyan Sahara Desert | LL5 chondrite | Fs% 22.1 | S3 | bronzite, olivine and minor oligoclase | lower because the fall was not witnessed | 26° 56.41' N. 16° 25.14' E. | directly proportional to initial velocity | A. Sexton, Open University, UK. Meteoritical Bulletin No 84 |
Lazbuddie | low | | | | | | | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | | | | | | | | | | 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 | LL5 chondrite | | | bronzite, olivine and minor oligoclase | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | |
Roosevelt Co 094 | low | | | | | | | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | | | | | | | | | | 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 | LL5 chondrite | | | bronzite, olivine and minor oligoclase | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | |
Sahara 97021 | which depends on its composition | planar fractures, undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 15 to 20 GPa | | |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | shock metamorphism | W2 | | February 1997 | | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | weakly shocked | 0.895 kg | orthopyroxene for enstatite chondrite | Sahara 97021 | before, during or after other types of metamorphism | Sahara Desert | S3 shock stage chondrite | | S3 | often minerals not found on Earth | lower because the fall was not witnessed | y° 08' 52" N., x° 28' 49" W. | directly proportional to initial velocity | |
Tuxtuac | low | | | | | | | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | | | | | | | | | | 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 | LL5 chondrite | | | bronzite, olivine and minor oligoclase | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | |