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LEW 85440 comparison table |
Subject | is paired with | has shock texture | has olivine inclusion | has reference | has minerology | has degree of shock metamorphism | has shock stage | is an instance of | has distinguishing feature | has orthopyroxene composition | has olivine grain characteristic | has metamorphism mechanism | has likely origin | has solidification mechanism | has shock diagnostic mineral | has olivine composition | has olivine shock metamorphism | has weather | has letter designation | has texture | has value | has total mass of find | has matrix composition | has characteristic mineral | is a kind of | has find date | has augite composition | has number of find | has origin | has shock pressure | has solidification timescale | has plagioclase | has definition | has intergranular boundary | has gain size | has pyroxene content | has petrology | has pyroxene inclusion |
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meteorite find | can be severe due to long exposure time to environmental corrosion agents | lower because the fall was not witnessed | 485755 kg | meteorite | when the meteorite was found | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | a meteorite whose fall was not witnessed | ||||||||||||||||||||||||||||||
monomict-poikilitic ureilite | silicates show minor fracturing, undulatory extinction and kink bands primarily in olivine | small rounded pyroxene grains (poikilitic) | olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite) | low | S2-S3 | no chondrules | reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal | shock metamorphism | partial melting residue | cooling in deep underground chambers | small euhedral graphite crystals can sometimes be distinguished | fracturing, undulatory extinction and kink bands | AURE | large, anhedral olivine and pyroxene grains | 9 kg (out of date) | carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume | olivine-pigeonite about 90% by volume | low shock ureilite | 6 (out of date) | asteroid | less than 20 GPa | very slow | 0 % | curved meeting in triple junctions | 1 mm | coarse-grained granular | small rounded olivine grains (poikilitic) | |||||||||||
LEW 85440 | LEW 88012 meteorite | silicates show minor fracturing, undulatory extinction and kink bands primarily in olivine | small rounded pyroxene grains (poikilitic) | Takeda et al. (1992), Takeda (1989), Takeda et al. (1988b), AMN13-2, AMN 13-3 | olivine, pyroxene (some combination of pigeonite, orthopyroxene, augite) | low | S2-S3 | meteorite find | no chondrules | Wo% 5.0 En% 87 | reduced rims contacting carbonaceous matrix material 0.1 mm FeO-free olivine and/or enstatite rims riddled with tiny inclusions of low-Ni metal | shock metamorphism | partial melting residue | cooling in deep underground chambers | small euhedral graphite crystals can sometimes be distinguished | Fo% 92 | fracturing, undulatory extinction and kink bands | can be severe due to long exposure time to environmental corrosion agents | AURE | large, anhedral olivine and pyroxene grains | lower because the fall was not witnessed | 485755 kg | carbon, metal, sulfides small silicate grains along grain boundaries less than 10% by volume | olivine-pigeonite about 90% by volume | when the meteorite was found | Wo% 36 En% 59 | 1691 | meteoroid from interplanetary space or fragment dislodged from another planet, moon or planetesimal | less than 20 GPa | very slow | 0 % | curved meeting in triple junctions | 1 mm | 0.43, 0.50 in modal pyroxene/(pryroxene+olivine) | coarse-grained granular | small rounded olivine grains (poikilitic) |
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