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Allan Hills A77307 | |||||||||||||||||||||||||||||||||
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Basic information | Name: Allan Hills A77307 This is an OFFICIAL meteorite name. Abbreviation: ALHA77307 This meteorite may also be called Allan Hills 77307 (ALH 77307) in publications. Observed fall: No Year found: 1977 or 1978 Country: Antarctica [Collected jointly by ANSMET (US) and NIPR (Japan)] Mass: 181.3 g | ||||||||||||||||||||||||||||||||
Classification history: |
This is 1 of 22 approved meteorites classified as CO3.0. [show all] Search for other: Carbonaceous chondrites, Carbonaceous chondrites (type 3), CM-CO clan chondrites, and CO chondrites | ||||||||||||||||||||||||||||||||
Writeup |
Writeup from AMN 1(3):
This text was reprinted from AMN 1(3) in AMN 4(1). In some cases, it may be an updated version from the original. Sample No.: ALHA77307 Location: Allan Hills Field No.: 78010702 Weight (gms): 181.3 Meteorite Type: Carbonaceous Chondrite - Type C-3
Physical Description: The rounded specimen is covered with a dull black fusion crust 1-2 mm thick over post of the surface. Specimen is complete with the exception of one end where a fracture surface covers 1/8 of the specimen's total surface area. The fusion crust has polygonal fractures over most of the exterior surface. In a few places this fusion crust has been broken away revealing a black fine-grained matrix. Specimen shows several large fractures. On the surface neighboring one of these fractures there is a white material which may be an evaporite deposit. The side of the specimen that was in contact with the ice at the time of recovery is slightly reddish. Dimensions: 4.5 x 4.0 x 5.0 cm. Small, irregular white inclusions and several chondrules are apparent on a freshly broken surface.
Petrographic Description: Brain Mason the section shows a closely-packed aggregate of mineral grains (up to 0.2 mm), mineral aggregates (up to 0.8 mm), and rather sparse small (0.1-0.5 mm) chondrules, set in a dark brown to black opaque matrix; the matrix makes up 40-50% of the section. The mineral grains, aggregates, and chondrules consist of olivine and polysynthetically-twinned clinopyroxene in approximately equal amounts. Microprobe analyses show that most of the olivine has forsterite composition, Fa~1, with a few grains ranging up to Fa30; the average for 30 grains is Fa5. The pyroxene is mostly clinoenstatite, Fs~l, but with a few more iron-rich grains. A little (1-2%) nickel-iron is present in the matrix as scattered grains, many partly altered to brown limonite. Fine-grained sulfide (~5%) is dispersed through the matrix. Fusion crust, 0.5 mm thick, is present along one edge of the section. The meteorite is a carbonaceous chondrite; an X-ray powder photograph shows that the matrix consists largely of olivine and pyroxene with some magnetite, which indicates a C3 classification. | ||||||||||||||||||||||||||||||||
Data from: MB76 Table 2 Line 256: |
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References: | Published in Antarctic Meteorite Newsletter 1(3) (1978), JSC, Houston Published in Meteoritical Bulletin, no. 76, Meteoritics 29, 100-143 (1994)
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Geography: |
Statistics: This is 1 of 45260 approved meteorites from Antarctica (plus 3472 unapproved names) | ||||||||||||||||||||||||||||||||
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