Subject |
has part mean Ni content of sulfide |
has weather resistance |
has part carbon |
has part matrix |
has prototype |
has shock pressure |
has acronym |
has degree of aqueous alteration |
has matrix abundance |
has sediment mechanism |
has weather |
has image |
has distinguishing feature |
has part feldspar |
has metal abundance |
has refractory inclusion abundance |
has relative abundance |
has fragmentation probability |
has chondrule mean diameter |
has metamorphism mechanism |
has fall date |
has weathering stage |
has chondrule glass type |
has age |
has number of fragment |
has part sulfide Ni content |
has part maximum bulk Ni in metal |
has petrologic type |
has find date |
has part water |
has comment |
has degree of thermal metamorphism |
has degree of shock metamorphism |
has mass |
has abundance |
has peak temperature |
has name |
has fall location |
has pyroxene composition |
has shock stage |
has part metal maximum bulk |
has homogeneity of olivine and low Ca pyroxene |
has composition |
has structural state of low Ca pyroxene |
has value |
has fall coordinate |
has olivine and low Ca pyroxene homogeneity |
has ablative mass loss |
has chondrule abundance |
has parent body |
has part chondrule |
classified by |
has petrologic type range |
Camel Donga 003 | in weight % | low | 0.2 to 1 % by weight | clastic and minor opaque | ??? meteorite | | | none | 75 % by volume | agglomeration of particles, many of which record individual, diverse histories | |
 | elemental carbon | minor primary grains only | 0.01 % by volume | 4 % by volume | 8 % of meteorite falls | high because it is more friable than iron meteorite | 0.7 millimeters | | recorded by eyewitness or inferred from dating methods | | clear, isotropic, variable abundance | 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 | 3 | 1984 | 0.3 to 3 % by weight | | none | | | rare relative to other chondrite types | less than 950 degree Celsius during its entire history since solidification | Camel Donga | Camel Donga, West Australia, Australia | | | in weight % | definition goes here | silicates (with very few exceptions) | predominantly monoclinic | | in degrees, minutes and seconds of lattitude and longitude | greater than 5 % deviations | high because it is more friable than iron meteorite | 15 % by volume | asteroid smaller than 100 km in diameter | chondrules very sharply defined | | which depends on degree of aqueous alteration and thermal metamorphism |
DaG 609 | | which depends on its composition | | | | 15 to 20 GPa | DaG | | | | can be severe due to long exposure time to environmental corrosion agents |
 | no chondrules | | | | | during meteor phase which depends on composition | | shock metamorphism | recorded by eyewitness or inferred from dating methods | W2 | | | 2 | | | | 1998 | | iron-rich, monomict, with chromite grains | | weakly shocked | 0.696 kg | | | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | Fs% 27-63 | S3 | | | often minerals not found on Earth | | lower because the fall was not witnessed | 26° 53.13' N. 16° 34.81' E. | | directly proportional to initial velocity | | | | A. Sexton, Open University, UK. A. Sexton, Meteoritical Bulletin No 83 | |
Millbillillie | | low | | | | | | | | | |
 | no chondrules | | | | 7.1 % of meteorite falls | high because it is more friable than iron meteorite | | | October 1960 | | | | | | | | | | | | | | | | Millbillillie | Millbillillie Station 11 kilometers from Wiluna, Western Australia | | | | | silicates (with very few exceptions) | | | in degrees, minutes and seconds of lattitude and longitude | | high because it is more friable than iron meteorite | | | | | |