Subject |
has weather resistance |
has olivine shock metamorphism |
is independent of |
has shock pressure |
has image |
has weather |
has relative abundance |
has fragmentation probability |
has metamorphism mechanism |
has fall date |
has original mass |
have composition |
has find date |
has orthopyroxene shock metamorphism |
has plagioclase shock metamorphism |
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 value |
has fall coordinate |
has ablative mass loss |
has fall map |
Bluff (b) | low | | | | | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | recorded by eyewitness or inferred from dating methods | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | | | | | | | | 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 | L4 chondrite | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |
Dalgety Downs | low | | | |
 | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | recorded by eyewitness or inferred from dating methods | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | | | | | | | | Dalgety Downs | | Dalgety Downs, Australia | L4 chondrite | | | 37° S., 148° 30' E. | high because it is more friable than iron meteorite | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |
Gold Basin | low | | | |
 | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | recorded by eyewitness or inferred from dating methods | greater than 61 kg | olivine, Fa24±1; pyroxene Fs20Wo1; kamacite contains 0.72±0.09 wt% Co; weathering grade W2-3 | November 24, 1995 | | | | | | Gold Basin | | Mohave County, Arizona, USA | L4 chondrite | | | Latitude 35 degrees 52 minutes 30 seconds North, Longitude 114 degrees 14 minutes West | high because it is more friable than iron meteorite |
 |
Haxtun | which depends on its composition | weak mosaicism, planar fractures | the nature and degree of thermal metamorphism or aqueous alteration | 30 to 35 GPa |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | shock metamorphism | recorded by eyewitness or inferred from dating methods | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | | August 1975 | weak mosaicism, twinning on (100), planar fractures | undulatory extinction, partially isotropic, planar deformation features | moderately shocked | 15.53 kg | orthopyroxene for enstatite chondrite | Haxtun | before, during or after other types of metamorphism | 21 km SSE of Haxtun, Colorado | S4 shock stage chondrite | S4 | lower because the fall was not witnessed | 40° 27.4' N., 102° 34.7' W. | directly proportional to initial velocity | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |
Okechobee | which depends on its composition | | | |
 | can be severe due to long exposure time to environmental corrosion agents | | during meteor phase which depends on composition | thermal metamorphism | recorded by eyewitness or inferred from dating methods | which can over an order of magnitude greater than total mass of fragment(s) collected at the impact site | | 1916 | | | | 1 kg | | Okechobee | | | meteorite find | | lower because the fall was not witnessed | 26° 41' N., 80° 48' W. | directly proportional to initial velocity | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |
Saratov | low | | | |
 | | 85.7 % of meteorite falls | high because it is more friable than iron meteorite | thermal metamorphism | September 6, 1918, 1800 hrs | greater than 328 kg | | | | | | | | Saratov | | Near Donguz, Penza, Russia | L4 chondrite | | | in degrees, minutes and seconds of lattitude and longitude | high because it is more friable than iron meteorite | which appears as an elongated footprint which depends on impact angle, airbursts, and impact velocity |