Subject |
has weather resistance |
has olivine shock metamorphism |
is independent of |
has shock pressure |
has acronym |
has olivine composition |
has weather |
has image |
has relative abundance |
has fragmentation probability |
has weathering stage |
have composition |
has number of fragment |
has find date |
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 value |
has fall coordinate |
has ablative mass loss |
classified by |
Correo | low | | | | | | | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | | | | | | | | | 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 | H4 chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | |
DaG 604 | 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% 18.1 | can be severe due to long exposure time to environmental corrosion agents |
 | | during meteor phase which depends on composition | W2 | | 1 | 1998 | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | weakly shocked | 0.180 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 | H4 chondrite | Fs% 16.4 | S3 | lower because the fall was not witnessed | 26° 58.74' N. 16° 18.65' E. | directly proportional to initial velocity | A. Sexton, Open University, UK. Meteoritical Bulletin No 83 |
DaG 638 | which depends on its composition | | | | DaG | Fa% 18.6 | can be severe due to long exposure time to environmental corrosion agents |
 | | during meteor phase which depends on composition | W2 | | 1 | 1998 | | | | 8.170 kg | | based on the locale, region, or nearby town in which the fall occurred | | Dar al Gani plateau, Libyan Sahara Desert | H4 chondrite | Fs% 16.6 Wo%2.4 | | lower because the fall was not witnessed | 26° 57' N. 16° 9' E. | directly proportional to initial velocity | A. Sexton, Open University, UK. Meteoritical Bulletin No 84 |
Dimmitt | low | | | | | | |
 | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | 24.8% iron, Olivine bronzite chondrite, brecciated | | | | | | | | Dimmitt | | Dimmitt, Castro County, Texas, USA | H4 chondrite | | | | 34° 35' N., 102° 10' W. | high because it is more friable than iron meteorite | |
Eustis | which depends on its composition | | | | | | can be severe due to long exposure time to environmental corrosion agents |
 | | during meteor phase which depends on composition | | | | 1918 | | | | 0.502 kg | | Eustis | | Eustis, Florida | meteorite find | | | lower because the fall was not witnessed | 28° 50' N., 81° 41' W. | directly proportional to initial velocity | |
Selma | which depends on its composition | | | | | | can be severe due to long exposure time to environmental corrosion agents |
 | | during meteor phase which depends on composition | | | | 1906 | | | | 140.7 kg | | Selma | | Dallas County, Alabama, 2 miles N. of Selma near the Summerfield road | meteorite find | | | lower because the fall was not witnessed | 32° 24' N., 87° 0' W. | directly proportional to initial velocity | |