Subject |
has weather resistance |
has part carbon |
has alteration temperature range |
has olivine shock metamorphism |
has part matrix |
is independent of |
has shock pressure |
has acronym |
has degree of aqueous alteration |
has petrologic subtype |
has image |
has weather |
has degree of secondary process |
has part feldspar |
has relative abundance |
has fragmentation probability |
has metamorphism mechanism |
has weathering stage |
has chondrule glass type |
has part sulfide Ni content |
has part maximum bulk Ni in metal |
has number of find |
has petrologic type |
has find date |
has part water |
has comment |
has degree of thermal metamorphism |
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 shock stage |
has structural state of low Ca pyroxene |
has value |
has fall coordinate |
has olivine and low Ca pyroxene homogeneity |
has ablative mass loss |
has total mass of find |
has part chondrule |
Carlisle Lakes | low | in weight % | | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | | | | | | | | | usually plagioclase tectosilicate | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | | | | | 1030 | 3 to 6 | | 0 % by weight (approximately) | | | | | | | | 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 | R chondrite | | definition goes here | | in degrees, minutes and seconds of lattitude and longitude | | high because it is more friable than iron meteorite | 20461 kg | small sphere of about 1 mm diameter of formerly melted minerals |
DaG 013 | which depends on its composition | in weight % | | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | | | DaG | | 3.5 |
 | can be severe due to long exposure time to environmental corrosion agents | | usually plagioclase tectosilicate | | during meteor phase which depends on composition | | | | | | 1691 | 3 to 6 | 1994-1995 | 0 % by weight (approximately) | | | | | | 0.205 kg | | DaG 013 | | Dar al Gani plateau, Libyan Sahara Desert | Dar al Gani meteorite | | definition goes here | lower because the fall was not witnessed | 27° 07.77' N., 16° 20.61' E. | | directly proportional to initial velocity | 485755 kg | small sphere of about 1 mm diameter of formerly melted minerals |
HaH 119 | which depends on its composition | less than 0.2 % by weight | the range over at which the alteration took place | planar fractures, undulatory extinction, irregular fractures | transparent, recrystallized, small crystals | the nature and degree of thermal metamorphism or aqueous alteration | 15 to 20 GPa | HaH | | |
 | can be severe due to long exposure time to environmental corrosion agents | providing insight into geological evolution of parent asteroid | secondary, grains than 2 microns | | during meteor phase which depends on composition | thermal metamorphism | W4 | devitrified, absent | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | 1691 | 4 | April 1995 | less than 1.5 % by weight | unbecciated | weak | clinoenstatite lamellae on (100), undulatory extinction, planar fractures, irregular fractures | undulatory extinction | weakly shocked | 0.352 kg | orthopyroxene for enstatite chondrite | HaH 119 | before, during or after other types of metamorphism | Hammadah al Hamra | S3 shock stage chondrite | S3 | greater than 20 % monoclinic | lower because the fall was not witnessed | 28° 30.87' N., 12° 53.81' E. | less than 5 % mean deviations | directly proportional to initial velocity | 485755 kg | chondrules well defined |
Rumuruti | low | 0.2 to 1 % by weight | | | clastic and minor opaque | | | | none | | | | | minor primary grains only | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | | clear, isotropic, variable abundance | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | 1030 | 3 | | 0.3 to 3 % by weight | | none | | | | | | Rumuruti | | Sahara | type 3 chondrite | | predominantly monoclinic | | in degrees, minutes and seconds of lattitude and longitude | greater than 5 % deviations | high because it is more friable than iron meteorite | 20461 kg | chondrules very sharply defined |
Sahara 98248 | low | in weight % | | | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | | | | | | | | | usually plagioclase tectosilicate | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | | | | | | 1030 | 3 to 6 | | 0 % by weight (approximately) | | | | | | | | 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 | R chondrite | | definition goes here | | in degrees, minutes and seconds of lattitude and longitude | | high because it is more friable than iron meteorite | 20461 kg | small sphere of about 1 mm diameter of formerly melted minerals |