Name: Miller Range 11237 This is an OFFICIAL meteorite name. Abbreviation: MIL 11237 Observed fall: No Year found: 2011 Country: Antarctica [Collected by US Antarctic Search for Meteorites program (ANSMET)] Mass: 12.9 g
The exteriors of these carbonaceous chondrites have black/brown fusion crust with oxidation haloes and rusty areas. The interiors range from dark gray to black matrix with some oxidation and tiny white specks. Most are fine grained.
Thin Section Description (,2) - Cari Corrigan, Linda Welzenbach, Pamela Salyer
These sections consist of abundant, small (up to 1 mm) chondrules, chondrule fragments, and mineral grains in a dark matrix. The matrix appears to consist largely of Fe-rich olivine. Metals and sulfides occur both within and rimming the chondrules. These meteorites have distinctly less metals and sulfides than the larger CO3 pairing group (MIL 07099). Olivine ranges in composition from Fa0-61, with a continuous range of intermediate compositions. Pyroxenes range Fs0-9Wo1-3. These meteorites are CO3 chondrites and are likely paired.
JSC: Mailcode XI, 2101 NASA Parkway, NASA Johnson Space Center, Houston, TX 77058, United States; Website (institutional address; updated 28 Jul 2022) SI: Department of Mineral Sciences, NHB-119, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560, United States; Website (institutional address; updated 16 Jan 2012)
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