Subject |
has iron metal and iron sulfide |
has sediment mechanism |
has weather resistance |
has metal abundance |
has part mean Ni content of sulfide |
has age |
has refractory inclusion abundance |
is an instance of |
has total iron content |
has olivine and low Ca pyroxene homogeneity |
has part feldspar |
has part metal maximum bulk |
has metal iron content |
has fragmentation probability |
has fall location |
has chondrule glass type |
has weather |
has homogeneity of olivine and low Ca pyroxene |
has acronym |
has chondrule abundance |
has relative abundance |
has abundance |
has part chondrule |
has degree of aqueous alteration |
has value |
has total mass of find |
has structural state of low Ca pyroxene |
has peak temperature |
has parent body |
has part matrix |
has degree of thermal metamorphism |
has petrologic type range |
has matrix abundance |
has part carbon |
has petrologic type |
has part maximum bulk Ni in metal |
has composition |
is a kind of |
has find date |
has part water |
has number of find |
has ablative mass loss |
has synonym |
has chondrule mean diameter |
has part sulfide Ni content |
Dar al Gani meteorite | | | which depends on its composition | | | | | | | | | | | during meteor phase which depends on composition | Dar al Gani plateau, Libyan Sahara Desert | | can be severe due to long exposure time to environmental corrosion agents | | DaG | | | | | | lower because the fall was not witnessed | 485755 kg | | | | | | | | | | | often minerals not found on Earth | Sahara meteorite | when the meteorite was found | | 1691 | directly proportional to initial velocity | | | |
LL3 chondrite | 20 % of total iron | agglomeration of particles, many of which record individual, diverse histories | low | 2 % by volume | in weight % | oldest and most primitive rock in solar system | 0.1 to 1 % by volume | | low | greater than 5 % deviations | minor primary grains only | in weight % | about 2 % | high because it is more friable than iron meteorite | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | clear, isotropic, variable abundance | | definition goes here | | 60 to 80 % by volume | 85.7 % of meteorite falls | most common chondrite observed from falls | chondrules very sharply defined | none | | 90 kg | predominantly monoclinic | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | clastic and minor opaque | none | which depends on degree of aqueous alteration and thermal metamorphism | 10 to 15 % by volume | 0.2 to 1 % by weight | 3 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | bronzite, olivine and minor oligoclase | type 3 chondrite | | 0.3 to 3 % by weight | 5 | high because it is more friable than iron meteorite | amphoterite | 0.9 millimeters | less than 0.5 % by weight |
DaG 180 | 20 % of total iron | agglomeration of particles, many of which record individual, diverse histories | which depends on its composition | 2 % by volume | in weight % | oldest and most primitive rock in solar system | 0.1 to 1 % by volume | Dar al Gani meteorite | low | greater than 5 % deviations | minor primary grains only | in weight % | about 2 % | during meteor phase which depends on composition | Dar al Gani plateau, Libyan Sahara Desert | clear, isotropic, variable abundance | can be severe due to long exposure time to environmental corrosion agents | definition goes here | DaG | 60 to 80 % by volume | | most common chondrite observed from falls | chondrules very sharply defined | none | lower because the fall was not witnessed | 90 kg | predominantly monoclinic | less than 950 degree Celsius during its entire history since solidification | asteroid smaller than 100 km in diameter | clastic and minor opaque | none | which depends on degree of aqueous alteration and thermal metamorphism | 10 to 15 % by volume | 0.2 to 1 % by weight | 3 | greater than 20 % by weight, kamacite and taenite in exsolution relationship | bronzite, olivine and minor oligoclase | | when the meteorite was found | 0.3 to 3 % by weight | 5 | directly proportional to initial velocity | amphoterite | 0.9 millimeters | less than 0.5 % by weight |