Subject |
has sediment mechanism |
has weather resistance |
has metal abundance |
has part mean Ni content of sulfide |
has degree of shock metamorphism |
has age |
has refractory inclusion abundance |
has shock stage |
is an instance of |
has distinguishing feature |
has part feldspar |
has part metal maximum bulk |
has fragmentation probability |
has fall location |
has metamorphism mechanism |
has degree of secondary process |
has name |
has shock diagnostic mineral |
is independent of |
has olivine shock metamorphism |
has weather |
has weathering stage |
be shock |
has homogeneity of olivine and low Ca pyroxene |
has acronym |
has chondrule abundance |
has relative abundance |
has abundance |
has part chondrule |
has petrologic subtype |
has value |
has total mass of find |
has structural state of low Ca pyroxene |
has peak temperature |
has plagioclase shock metamorphism |
has orthopyroxene shock metamorphism |
has parent body |
has part matrix |
has matrix abundance |
has petrologic type range |
has fall coordinate |
has part carbon |
is a kind of |
has find date |
has part water |
has mass |
has image |
has number of find |
has ablative mass loss |
has shock pressure |
has chondrule mean diameter |
Dar al Gani meteorite | | which depends on its composition | | | | | | | | | | | during meteor phase which depends on composition | Dar al Gani plateau, Libyan Sahara Desert | | | based on the locale, region, or nearby town in which the fall occurred | | | | can be severe due to long exposure time to environmental corrosion agents | | | | DaG | | | | | | lower because the fall was not witnessed | 485755 kg | | | | | | | | | in degrees, minutes and seconds of lattitude and longitude | | Sahara meteorite | when the meteorite was found | | | | 1691 | directly proportional to initial velocity | | |
S2 shock stage chondrite | agglomeration of particles, many of which record individual, diverse histories | which depends on its composition | in volume % | in weight % | very weakly shocked | oldest and most primitive rock in solar system | in volume % | S2 | | | usually plagioclase tectosilicate | in weight % | during meteor phase which depends on composition | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | shock metamorphism | providing insight into geological evolution of parent asteroid | based on the locale, region, or nearby town in which the fall occurred | orthopyroxene for enstatite chondrite | the nature and degree of thermal metamorphism or aqueous alteration | undulatory extinction, irregular fractures | | | before, during or after other types of metamorphism | definition goes here | | in volume % | | | small sphere of about 1 mm diameter of formerly melted minerals | | | 485755 kg | definition goes here | less than 950 degree Celsius during its entire history since solidification | undulatory extinction, irregular fractures | undulatory extinction, irregular fractures, some planar fractures | asteroid smaller than 100 km in diameter | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | in volume % | which depends on degree of aqueous alteration and thermal metamorphism | in degrees, minutes and seconds of lattitude and longitude | in weight % | S2 shock stage meteorite | | in weight % | | | 1691 | directly proportional to initial velocity | 5 to 10 GPa | millimeters |
ungrouped carbonaceous chondrite | agglomeration of particles, many of which record individual, diverse histories | low | in volume % | in weight % | | oldest and most primitive rock in solar system | in volume % | | | elemental carbon | usually plagioclase tectosilicate | in weight % | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | | based on the locale, region, or nearby town in which the fall occurred | | | | | | | definition goes here | | in volume % | 8 % of meteorite falls | rare relative to other chondrite types | small sphere of about 1 mm diameter of formerly melted minerals | | | 2577 kg | definition goes here | less than 950 degree Celsius during its entire history since solidification | | | asteroid smaller than 100 km in diameter | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | in volume % | which depends on degree of aqueous alteration and thermal metamorphism | in degrees, minutes and seconds of lattitude and longitude | in weight % | carbonaceous chondrite | | in weight % | | | 36 | high because it is more friable than iron meteorite | | millimeters |
DaG 055 | agglomeration of particles, many of which record individual, diverse histories | which depends on its composition | in volume % | in weight % | very weakly shocked | oldest and most primitive rock in solar system | in volume % | S2 | S2 shock stage chondrite | elemental carbon | usually plagioclase tectosilicate | in weight % | during meteor phase which depends on composition | Dar al Gani plateau, Libyan Sahara Desert | shock metamorphism | providing insight into geological evolution of parent asteroid | DaG 055 | orthopyroxene for enstatite chondrite | the nature and degree of thermal metamorphism or aqueous alteration | undulatory extinction, irregular fractures | can be severe due to long exposure time to environmental corrosion agents | W1 | before, during or after other types of metamorphism | definition goes here | DaG | in volume % | 8 % of meteorite falls | rare relative to other chondrite types | small sphere of about 1 mm diameter of formerly melted minerals | 3 | lower because the fall was not witnessed | 2577 kg | definition goes here | less than 950 degree Celsius during its entire history since solidification | undulatory extinction, irregular fractures | undulatory extinction, irregular fractures, some planar fractures | asteroid smaller than 100 km in diameter | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | in volume % | which depends on degree of aqueous alteration and thermal metamorphism | 27° 16.03' N., 16° 25.22' E. | in weight % | | June 1995 | in weight % | 0.451 kg |
 | 36 | directly proportional to initial velocity | 5 to 10 GPa | millimeters |