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Allan Hills A77289 | |||||||||||||||||||||||||||||
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Basic information | Name: Allan Hills A77289 This is an OFFICIAL meteorite name. Abbreviation: ALHA77289 This meteorite may also be called Allan Hills 77289 (ALH 77289) in publications. Observed fall: No Year found: 1977 or 1978 Country: Antarctica [Collected jointly by ANSMET (US) and NIPR (Japan)] Mass: ![]() | ||||||||||||||||||||||||||||
Classification history: |
This is 1 of 120 approved meteorites classified as Iron, IAB-MG. [show all] Search for other: IAB complex irons, Iron meteorites, and Metal-rich meteorites | ||||||||||||||||||||||||||||
Writeup![]() |
Writeup from AMN 3(2):
This text was reprinted from AMN 3(2) in AMN 4(1). In some cases, it may be an updated version from the original. Sample No.: ALHA77289 Location: Allan Hills Field No.: 78010401 Weight (gms): 2186.0 Meteorite Type: Iron - Group I or Og
Physical Description: The sample is angular and oblong (22x10x5 cm). It is orangish-brown and has many regmaglypts. The B surface has radial and transverse flow lines resulting from its orientation during atmospheric entry. The B surface also shows a zone of preferential melting (?) ~1 cm wide, that penetrates through the sample to the T surface. However, the zone of melting is only ~0.5 cm wide on the T surface.
Tentative Classification: Roy S. Clarke, Jr. An area of approximately 25 cm2 of macroetched surface was examined. Kamacite band widths are difficult to measure as the kamacite crystals tend to be stubby and irregular in outline. Estimated band widths are in the 2 to 3 mm range. Patches of α2 produced by atmospheric ablation are present along about half of the rim of the slice. Neumann bands are present. The dominant surface feature to the unaided eye is a highly speckled appearance due to abundant recrystallized kamacite fairly uniformly distributed over the surface. Modest amounts of grain boundary taenite and occasional small comb plessite areas are present. Schreibersite is present along grain boundaries. No large troilite or schreibersite are present and cohenite was not observed. External weathering is moderately severe. The specimen is a coarse octahedrite, a Group I or Og meteorite. | ||||||||||||||||||||||||||||
Data from: MB76 Table 2 Line 239: |
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References: | Published in Antarctic Meteorite Newsletter 3(2) (1980), JSC, Houston Published in Meteoritical Bulletin, no. 76, Meteoritics 29, 100-143 (1994)
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Geography:![]() |
Statistics: This is 1 of 44248 approved meteorites from Antarctica (plus 3802 unapproved names) | ||||||||||||||||||||||||||||
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