Subject |
has weather resistance |
has olivine shock metamorphism |
is independent of |
has shock pressure |
has acronym |
has petrologic subtype |
has image |
has weather |
has degree of secondary process |
has relative abundance |
has fragmentation probability |
has metamorphism mechanism |
has fall date |
has weathering stage |
has fall description |
has number of find |
has find date |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
has identification date |
has degree of shock metamorphism |
has mass |
has shock diagnostic mineral |
has name |
be shock |
has fall location |
is an instance of |
has shock stage |
has curatorial location |
has value |
has fall coordinate |
has ablative mass loss |
has total mass of find |
Acfer 094 | low | | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | | 36 | | | | | | | | 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 | ungrouped carbonaceous chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
Adelaide | low | | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | | 36 | | | | | | | | 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 | ungrouped carbonaceous chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
Bench Crater | low | | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | | 36 | | | | | | | | 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 | ungrouped carbonaceous chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
Coolidge | low | | | | | | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | | 36 | | | | | | | | Coolidge | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | ungrouped carbonaceous chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
DaG 055 | which depends on its composition | undulatory extinction, irregular fractures | the nature and degree of thermal metamorphism or aqueous alteration | 5 to 10 GPa | DaG | 3 |
 | can be severe due to long exposure time to environmental corrosion agents | providing insight into geological evolution of parent asteroid | 8 % of meteorite falls | during meteor phase which depends on composition | shock metamorphism | recorded by eyewitness or inferred from dating methods | W1 | | 36 | June 1995 | undulatory extinction, irregular fractures, some planar fractures | undulatory extinction, irregular fractures | | very weakly shocked | 0.451 kg | orthopyroxene for enstatite chondrite | DaG 055 | before, during or after other types of metamorphism | Dar al Gani plateau, Libyan Sahara Desert | S2 shock stage chondrite | S2 | | lower because the fall was not witnessed | 27° 16.03' N., 16° 25.22' E. | directly proportional to initial velocity | 2577 kg |
LEW 85332 | which depends on its composition | | | | | | | | | | during meteor phase which depends on composition | | recorded by eyewitness or inferred from dating methods | | | 1691 | 1985 | | | | | | | LEW 85332 | | indicated by letters in the beginning of name | Antarctic meteorite | | | | in degrees, minutes and seconds of lattitude and longitude | directly proportional to initial velocity | 485755 kg |
Mulga West | low | | | | | 5 | | | | 8 % of meteorite falls | high because it is more friable than iron meteorite | | recorded by eyewitness or inferred from dating methods | | | 36 | | | | | | | | 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 | ungrouped carbonaceous chondrite | | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | 2577 kg |
Ningqiang | which depends on its composition | | | | | 3.3 |
 | negligible due to quick recovery of meteorite before corrosion begins | | | during meteor phase which depends on composition | | June 25, 1983 7:00 pm | | what witnesses saw or what was recorded by instruments | 1691 | | | | | | 4.61 kg | | Ningqiang | | Ningqiang County, Shaanxi Province, China | meteorite fall | | Zijin Shan Observatory, Academia Sinica, in Nanjing, Jiangsu Province, China | higher because the fall was witnessed | 32° 55.5' N., 105° 54.4' E. | directly proportional to initial velocity | 485755 kg |