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Allan Hills 83015 | |||||||||||||||||||||||||
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Basic information | Name: Allan Hills 83015 This is an OFFICIAL meteorite name. Abbreviation: ALH 83015 Observed fall: No Year found: 1983 Country: Antarctica [Collected by US Antarctic Search for Meteorites program (ANSMET)] Mass: ![]() | ||||||||||||||||||||||||
Classification history: |
This is 1 of 79 approved meteorites classified as Aubrite. [show all] Search for other: Achondrites, Aubrites, Enstatite achondrites, and Enstatite-rich meteorites | ||||||||||||||||||||||||
Writeup![]() |
Writeup from AMN 8(1):
Sample No.: ALH83015 Location: Allan Hills Weight (g): 3.1 Field No.: 2138 Dimensions (cm): 1.5 x 1.5 x 1 Meteorite Type: Aubrite (?)
Macroscopic Description: Roberta Score This specimen is white in color and is identical in appearance to ALH83009.
Thin Section (,2) Description: Jeremy Delaney ALH83015 is a pyroxenite breccia with clasts up to 1-5 mm. Matrix is very fine-grained with brown/green staining common. Pyroxene grains often contain submicron to 10 micron opaque (troilite?) inclusions on healed cracks. One heavily clouded pyroxene is also present. Areas of fine-grained breccia against coarse-grained breccia occur. Tiny olivine-troilite clasts are present, as are small matrix olivines. Large orthopyroxene clasts have mottled appearance and appear shocked. The pyroxene has no micron or larger scale exsolution and appears to be orthopyroxene. Brown staining caused by weathering of metal/troilite stains most grain boundaries and large troilite or metal clasts often have "rusty" halos. This specimen may be similar to the 83009 aubrite. Minor phases include daubreelite, alabandite, metal and Ti-bearing troilite. | ||||||||||||||||||||||||
Data from: MB76 Table 2 Line 898: |
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References: | Published in Antarctic Meteorite Newsletter 8(1) (1985), JSC, Houston Published in Meteoritical Bulletin, no. 76, Meteoritics 29, 100-143 (1994)
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Geography:![]() |
Statistics: This is 1 of 44048 approved meteorites from Antarctica (plus 3802 unapproved names) | ||||||||||||||||||||||||
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