Subject |
has part mean Ni content of sulfide |
has weather resistance |
has part carbon |
has alteration temperature range |
has olivine shock metamorphism |
has part matrix |
has prototype |
is independent of |
has shock pressure |
has acronym |
has matrix abundance |
has sediment mechanism |
has image |
has weather |
has distinguishing feature |
has degree of secondary process |
has part feldspar |
has metal abundance |
has refractory inclusion abundance |
has relative abundance |
has fragmentation probability |
has chondrule mean diameter |
has metamorphism mechanism |
has weathering stage |
is a kind of |
has chondrule glass type |
has age |
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 degree of thermal metamorphism |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has degree of shock metamorphism |
has abundance |
has peak temperature |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has shock stage |
has part metal maximum bulk |
has homogeneity of olivine and low Ca pyroxene |
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 chondrule abundance |
has parent body |
has part chondrule |
has petrologic type range |
CK4 chondrite | in weight % | low | less than 0.2 % by weight | the range over at which the alteration took place | | transparent, recrystallized, small crystals | ??? meteorite | | | | 75 % by volume | agglomeration of particles, many of which record individual, diverse histories | | | elemental carbon | providing insight into geological evolution of parent asteroid | secondary, grains than 2 microns | 0.01 % by volume | 4 % by volume | 8 % of meteorite falls | high because it is more friable than iron meteorite | 0.7 millimeters | thermal metamorphism | | type 4 chondrite | devitrified, absent | oldest and most primitive rock in solar system | less than 0.5 % by weight | greater than 20 % by weight, kamacite and taenite in exsolution relationship | 36 | 4 | | less than 1.5 % by weight | weak | | | | rare relative to other chondrite types | less than 950 degree Celsius during its entire history since solidification | | 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 | | | in weight % | definition goes here | greater than 20 % monoclinic | | in degrees, minutes and seconds of lattitude and longitude | less than 5 % mean deviations | high because it is more friable than iron meteorite | 2577 kg | 15 % by volume | asteroid smaller than 100 km in diameter | chondrules well defined | which depends on degree of aqueous alteration and thermal metamorphism |
Dar al Gani meteorite | | which depends on its composition | | | | | | | | DaG | | | | can be severe due to long exposure time to environmental corrosion agents | | | | | | | during meteor phase which depends on composition | | | | Sahara meteorite | | | | | 1691 | | when the meteorite was found | | | | | | | | | based on the locale, region, or nearby town in which the fall occurred | | Dar al Gani plateau, Libyan Sahara Desert | | | | | | lower because the fall was not witnessed | in degrees, minutes and seconds of lattitude and longitude | | directly proportional to initial velocity | 485755 kg | | | | |
S2 shock stage chondrite | in weight % | which depends on its composition | in weight % | | undulatory extinction, irregular fractures | fine grained disequilibrium mixture of silicates, oxides, metal, sulfides and organic constituents | | the nature and degree of thermal metamorphism or aqueous alteration | 5 to 10 GPa | | in volume % | agglomeration of particles, many of which record individual, diverse histories | | | | providing insight into geological evolution of parent asteroid | usually plagioclase tectosilicate | in volume % | in volume % | | during meteor phase which depends on composition | millimeters | shock metamorphism | | S2 shock stage meteorite | | oldest and most primitive rock in solar system | | | 1691 | | | in weight % | | undulatory extinction, irregular fractures, some planar fractures | undulatory extinction, irregular fractures | very weakly shocked | | less than 950 degree Celsius during its entire history since solidification | 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 | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | | S2 | in weight % | definition goes here | definition goes here | | in degrees, minutes and seconds of lattitude and longitude | | directly proportional to initial velocity | 485755 kg | in volume % | asteroid smaller than 100 km in diameter | small sphere of about 1 mm diameter of formerly melted minerals | which depends on degree of aqueous alteration and thermal metamorphism |
DaG 275 | in weight % | which depends on its composition | less than 0.2 % by weight | the range over at which the alteration took place | undulatory extinction, irregular fractures | transparent, recrystallized, small crystals | ??? meteorite | the nature and degree of thermal metamorphism or aqueous alteration | 5 to 10 GPa | DaG | 75 % by volume | agglomeration of particles, many of which record individual, diverse histories |
 | can be severe due to long exposure time to environmental corrosion agents | elemental carbon | providing insight into geological evolution of parent asteroid | secondary, grains than 2 microns | 0.01 % by volume | 4 % by volume | | during meteor phase which depends on composition | 0.7 millimeters | shock metamorphism | W4 | | devitrified, absent | oldest and most primitive rock in solar system | 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 | undulatory extinction, irregular fractures, some planar fractures | undulatory extinction, irregular fractures | very weakly shocked | rare relative to other chondrite types | less than 950 degree Celsius during its entire history since solidification | orthopyroxene for enstatite chondrite | DaG 275 | before, during or after other types of metamorphism | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | S2 | in weight % | definition goes here | greater than 20 % monoclinic | lower because the fall was not witnessed | 27° 21.74' N., 16° 05.38' E. | less than 5 % mean deviations | directly proportional to initial velocity | 485755 kg | 15 % by volume | asteroid smaller than 100 km in diameter | chondrules well defined | which depends on degree of aqueous alteration and thermal metamorphism |