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Grosvenor Mountains 85201 | |||||||||||||||||||||||||
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Basic information | Name: Grosvenor Mountains 85201 This is an OFFICIAL meteorite name. Abbreviation: GRO 85201 Observed fall: No Year found: 1985 Country: Antarctica [Collected by US Antarctic Search for Meteorites program (ANSMET)] Mass: ![]() | ||||||||||||||||||||||||
Classification history: |
This is 1 of 338 approved meteorites classified as Iron, IIIAB. [show all] Search for other: IIIAB irons, Iron meteorites, and Metal-rich meteorites | ||||||||||||||||||||||||
Writeup![]() |
Writeup from AMN 10(2):
Sample No.: GRO85201 Location: Grosvenor Mountains Weight (g): 1400.7 Dimensions (cm): 13 x 8 x 3.5 Field No.: 2010 Meteorite Type: Octahedrite, probably IIIAB
Macroscopic Description: Roy S. Clarke, Jr. The specimen is flat and roughly the shape of a slightly curved extended hand with closed fingers and thumb. The convex surface was the anterior surface during stable oriented flight. A distinct stagnation point is present at the center of this surface from which streamers of melt flowed to a circumferential lip that separates the anterior and posterior surfaces. The anterior surface is a dark reddish brown due to the presence of terrestrial oxides with patches of black fusion crust. The posterior surface is darker and has a uniform matte appearance. The specimen has been exposed to long terrestrial weathering, but its delicate ablation-produced markings are remarkably well preserved.
Polished Section Description: Roy S. Clarke, Jr. A slice was removed from the narrow end of the specimen giving an area of 11 cm2 for examination. A regular Widmanstätten pattern with band widths from 0.8 to 1.5 mm is present. Plessite areas and centers of taenite bands have a martensitic structure. Grain boundary schreibersite and occasional large rhabdites are present. Weathering has penetrated along grain boundaries into the interior. The anterior edge has a coating of intermittent terrestrial oxide generally less than 0.1 mm thick and containing remnant fusion crust in some few areas. The posterior edge is uniformly covered with a layered, lightly weathered fusion crust 1.0 to 1.5 mm thick. Interior to both edges is an α2 structure typical of a heat-altered zone. This α2 structure blends into a much coarser martensite structure that is present throughout the kamacite in the section. The meteorite is a medium octahedrite, probably a IIIAB meteorite. | ||||||||||||||||||||||||
Data from: MB76 Table 2 Line 2850: |
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References: | Published in Antarctic Meteorite Newsletter 10(2) (1987), JSC, Houston Published in Meteoritical Bulletin, no. 76, Meteoritics 29, 100-143 (1994)
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Geography:![]() |
Statistics: This is 1 of 43856 approved meteorites from Antarctica (plus 3802 unapproved names) | ||||||||||||||||||||||||
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