Subject |
has reference |
is an instance of |
has orthopyroxene composition |
has fall location |
has fall date |
has name |
has olivine composition |
has fall description |
has weather |
has weathering stage |
has acronym |
has value |
has total mass of find |
paired with |
has fall coordinate |
has find date |
has mass |
has image |
has number of find |
has plagioclase |
has pigeonite composition |
has intergranular boundary |
has pyroxene content |
ALHA81101 | Berkley (1986), Saito and Takeda (1990) | meteorite find | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | based on the locale, region, or nearby town in which the fall occurred | Fo% 79 | | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | when the meteorite was found | | | 1691 | | Wo% 8.1 En% 78 | | |
DaG 084 | Weber and Bischoff (1996) | Dar al Gani meteorite | | Dar al Gani plateau, Libyan Sahara Desert | recorded by eyewitness or inferred from dating methods | DaG 084 | Fo% 79 | | can be severe due to long exposure time to environmental corrosion agents | W3 | DaG | lower because the fall was not witnessed | 9 kg (out of date) | | 27° 02.44' N., 16° 24.26' E. | 1995 | 0.277 kg |
 | 6 (out of date) | | Wo% 5.0 En% 81 | | |
Dyalpur | Berkley et. al (1980) | meteorite fall | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or instruments | based on the locale, region, or nearby town in which the fall occurred | Fo% 84 | what witnesses saw or what was recorded by instruments | negligible due to quick recovery of meteorite before corrosion begins | | | higher because the fall was witnessed | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | | | | 1691 | | Wo% 11 En% 76 | | 0.41 in modal pyroxene/(pryroxene+olivine) |
FRO 90036 | Baba et al. (1993), Folco (1992) | meteorite find | Wo% 3.0 En% 81 | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | based on the locale, region, or nearby town in which the fall occurred | Fo% 80 | | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | FRO 90168 meteorite | in degrees, minutes and seconds of lattitude and longitude | when the meteorite was found | | | 1691 | | | | |
Goalpara | Berkley et. al (1980) | meteorite find | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | based on the locale, region, or nearby town in which the fall occurred | Fo% 79 | | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | when the meteorite was found | | | 1691 | | Wo% 4.4 En% 76 | | 0.33 in modal pyroxene/(pryroxene+olivine) |
Havero | Berkley et. al (1980) | meteorite fall | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or instruments | based on the locale, region, or nearby town in which the fall occurred | Fo% 79 | what witnesses saw or what was recorded by instruments | negligible due to quick recovery of meteorite before corrosion begins | | | higher because the fall was witnessed | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | | | | 1691 | 0 % | Wo% 2.5 En% 81 clinobronzite | curved meeting in triple junctions | 0.17 in modal pyroxene/(pryroxene+olivine) |
LEW 86216 | Berkley (1990) | meteorite find | Wo% 1.7 En% 88 | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | based on the locale, region, or nearby town in which the fall occurred | Fo% 81 | | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | when the meteorite was found | | | 1691 | | | | 0.02 in modal pyroxene/(pryroxene+olivine) |
Y-74154 | Yanai and Kojima (1995b) | meteorite find | | strewn fields, elongated footprints which depends on impact angle, airbursts, and impact velocity | recorded by eyewitness or inferred from dating methods | based on the locale, region, or nearby town in which the fall occurred | Fo% 84 | | can be severe due to long exposure time to environmental corrosion agents | | | lower because the fall was not witnessed | 485755 kg | | in degrees, minutes and seconds of lattitude and longitude | when the meteorite was found | | | 1691 | | Wo% 8.1 En% 79 variable due to interstitial or shock melts | | |