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Allan Hills A77003 | |||||||||||||||||||||||||||||||||||||
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Basic information | Name: Allan Hills A77003 This is an OFFICIAL meteorite name. Abbreviation: ALHA77003 This meteorite may also be called Allan Hills 77003 (ALH 77003) in publications. Observed fall: No Year found: 1977 Country: Antarctica [Collected jointly by ANSMET (US) and NIPR (Japan)] Mass: ![]() | ||||||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 8 approved meteorites classified as CO3.6. [show all] Search for other: Carbonaceous chondrites, Carbonaceous chondrites (type 3), CM-CO clan chondrites, and CO chondrites | ||||||||||||||||||||||||||||||||||||
Writeup![]() |
Writeup from AMN 4(1):
Sample No.: ALHA77003 Location: Allan Hills Field No.: 77122920 Weight (gms): 779.6 Meteorite Type: H3 Chondrite
Physical Description: Specimen is very well rounded. No surface fissures are present. Fusion crust covers 33% of the meteorite's surface, (~100% T surface, 30% N and W surfaces, and 10% of E surface) and ranges from 1 to 3 mm thick. The crust is medium black and slightly glassy. The fusion crust is preserved on the surface (s) that were uppermost at the time of discovery (see field photo). The remaining surface of the meteorite is smooth, brownish-black, and has little iron-oxide staining. This surface is polished and may be the lower part of a fusion crust or a wind-polished surface. In an area ~l cm x 2 cm this surface has been removed, revealing an interior surface that is partially iron-oxide stained. This is a well indurated specimen. Repeated attempts to chip this meteorite for thin section samples were all partially successful.
Petrographic Description: Brian Mason Numerous and well-defined chondrules, 0.1-0.6 mm in diameter, along with mineral clasts are present in a fine-grained groundmass colored brown with limonitic material. The chondrules exhibit a variety of form and structure, the commonest consisting of granular aggregates of olivine and polysynthetically twinned clinopyroxene; some chondrules have pale brown transparent glass interstitial to the olivine and pyroxene grains. Microprobe analyses show that both olivine and pyroxene are highly variable in composition. Olivine ranges from Fa4 to Fa48 with a mean of Fa22; pyroxene ranges from Fs2 to Fs25, with a mean of Fs14, and its calcium content averages 1% CaO. The highly variable composition of olivine and pyroxene indicates a type 3 chondrite, and the mean composition of the olivine and small amount of nickel-iron suggest L group, so the meteorite is tentatively classified L3; however, certain assignment of group should await further investigation. | ||||||||||||||||||||||||||||||||||||
Data from: MB76 Table 2 Line 12: |
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Catalogs: |
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References: | Published in Antarctic Meteorite Newsletter 4(1) (1981), 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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