Subject |
has part carbon |
has alteration temperature range |
has synonym |
has part matrix |
has acronym |
has degree of aqueous alteration |
has petrologic subtype |
has olivine composition |
has image |
has weather |
has part feldspar |
has metal abundance |
has chondrule mean diameter |
has fall date |
has weathering stage |
has fall description |
has chondrule glass type |
has number of fragment |
has total iron content |
has number of find |
has petrologic type |
has find date |
has part water |
has degree of thermal metamorphism |
has iron metal and iron sulfide |
has mass |
has name |
has fall location |
has pyroxene composition |
has composition |
has structural state of low Ca pyroxene |
has value |
has fall coordinate |
has olivine and low Ca pyroxene homogeneity |
has total mass of find |
has part chondrule |
has metal iron content |
classified by |
DaG 632 | 0.2 to 1 % by weight | | amphoterite | clastic and minor opaque | DaG | none | 3.2 - 3.4 | Fa% 4.7 - 35.9 |
 | can be severe due to long exposure time to environmental corrosion agents | minor primary grains only | 2 % by volume | 0.9 millimeters | recorded by eyewitness or inferred from dating methods | W2 | | clear, isotropic, variable abundance | 1 | low | 5 | 3 | 1998 | 0.3 to 3 % by weight | none | 20 % of total iron | 0.340 kg | based on the locale, region, or nearby town in which the fall occurred | Dar al Gani plateau, Libyan Sahara Desert | Fs% 17.7 | bronzite, olivine and minor oligoclase | predominantly monoclinic | lower because the fall was not witnessed | 26° 54.46' N. 16° 42.10' E. | greater than 5 % deviations | 90 kg | chondrules very sharply defined | about 2 % | A. Sexton, Open University, UK. Meteoritical Bulletin No 84 |
Haxtun | less than 0.2 % by weight | the range over at which the alteration took place | hypersthene chondrite | transparent, recrystallized, small crystals | | | | |
 | can be severe due to long exposure time to environmental corrosion agents | secondary, grains than 2 microns | 5 % by volume | 0.7 millimeters | recorded by eyewitness or inferred from dating methods | | | devitrified, absent | | low | 21 | 4 | August 1975 | less than 1.5 % by weight | weak | 50 % of total iron | 15.53 kg | Haxtun | 21 km SSE of Haxtun, Colorado | | often minerals not found on Earth | greater than 20 % monoclinic | lower because the fall was not witnessed | 40° 27.4' N., 102° 34.7' W. | less than 5 % mean deviations | 1197 kg | chondrules well defined | 5 to 10 % | |
Monahans (1998) | less than 0.2 % by weight | the range over at which the alteration took place | bronzite chondrite | transparent, recrystallized, moderate size crystals | | | | |
 | negligible due to quick recovery of meteorite before corrosion begins | secondary, 2 to 50 micron grains | 10 % by volume | 0.3 millimeters | 6:47 pm March 22, 1998 | | what witnesses saw or what was recorded by instruments | devitrified, absent | | high | 76 | 5 | | less than 1.5 % by weight | moderate | 75 % of total iron | 2.587 kg | Monahans (1998) | Allen Street, Monahans, Texas | | often minerals not found on Earth | less than 20 % monoclinic | higher because the fall was witnessed | 102° 53.5' W., 31° 36.5' N. | homogeneous | 1267 kg | chondrules readily delineated | 12 to 21 % | |
Moorabie | 0.2 to 1 % by weight | | hypersthene chondrite | clastic and minor opaque | | none | 3.8 | |
 | can be severe due to long exposure time to environmental corrosion agents | minor primary grains only | 5 % by volume | 0.7 millimeters | recorded by eyewitness or inferred from dating methods | | | clear, isotropic, variable abundance | | low | 10 | 3 | before 1965 | 0.3 to 3 % by weight | none | 50 % of total iron | 14.1 kg | Moorabie | 130 miles north of Broken Hill close to Boolka, 10 miles south of Moorabie Bore, New South Wales | | often minerals not found on Earth | predominantly monoclinic | lower because the fall was not witnessed | 30° 6' S., 141° 4' E. | greater than 5 % deviations | 131 kg | chondrules very sharply defined | 5 to 10 % | |