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Allan Hills A77249 | |||||||||||||||||||||||||
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Basic information | Name: Allan Hills A77249 This is an OFFICIAL meteorite name. Abbreviation: ALHA77249 This meteorite may also be called Allan Hills 77249 (ALH 77249) in publications. Observed fall: No Year found: 1977 Country: Antarctica [Collected jointly by ANSMET (US) and NIPR (Japan)] Mass: 504 g | ||||||||||||||||||||||||
Classification history: |
This is 1 of 98 approved meteorites classified as L3.5. [show all] Search for other: L chondrites, L chondrites (type 3), Ordinary chondrites, and Ordinary chondrites (type 3) | ||||||||||||||||||||||||
Writeup |
Writeup from AMN 2(1):
This text was reprinted from AMN 2(1) in AMN 4(1). In some cases, it may be an updated version from the original. Sample No.: ALHA77249 Location: Allan Hills Field No.: 77122925 Weight (gms): 503.6 Meteorite Type: L3 Chondrite
Physical Description: This is not a complete specimen. The S and T surfaces have very thin, dull, patches of fusion crust. The B surface has thin, shiny black fusion crust, portions of which have weathered to reddish-brown. There are numerous inclusions, both chondrules and lithic clasts, visible through the reddish-brown oxidation rind. The largest chondrule is approximately 0.5 cm in diameter and is lighter colored than the surrounding matrix. A few inclusions that are darker than the matrix are also observed; however, they are not as numerous or as large. The sample is angular, 11.0x6.5x5.0 cm, and has many obvious fractures on the exterior surface.
Petrographic Description: Brian Mason The thin section shows an aggregate of well-defined chondrules, 0.3-2.1 mm in diameter, set in a small amount of fine-grained groundmass. A wide variety of chondrule types is present, the commonest being barred olivine, porphyritic olivine, granular olivine-pyroxene, and fine-grained pyroxene. The olivine chondrules frequently have interstitial glass, usually turbid and partly de-vitrified, but occasionally transparent with a pale brown color. Pyroxene grains show polysynthetic twinning. Sparse nickel-iron and troilite is concentrated on the surfaces of chondrules. Limonitic staining pervades the section, and scattered grains of red-brown limonite are present. Microprobe analyses show a wide range in the composition of olivine (Fa7-Fa35, average Fa17) and pyroxene (Fs2-Fs25, average Fs11). This range of composition, together with the presence of glass and twinned clinopyroxene, indicates type 3, and the small amount of nickel-iron suggests L group; the meteorite is therefore tentatively classified as an L3 chondrite. | ||||||||||||||||||||||||
Data from: MB76 Table 2 Line 200: |
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Catalogs: |
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References: | Published in Antarctic Meteorite Newsletter 2(1) (1979), JSC, Houston Published in Meteoritical Bulletin, no. 76, Meteoritics 29, 100-143 (1994)
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Geography: |
Statistics: This is 1 of 44547 approved meteorites from Antarctica (plus 3802 unapproved names) | ||||||||||||||||||||||||
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Revision history: |
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