Name: Miller Range 11193 This is an OFFICIAL meteorite name. Abbreviation: MIL 11193 Observed fall: No Year found: 2011 Country: Antarctica [Collected by US Antarctic Search for Meteorites program (ANSMET)] Mass: 5.8 g
All of these carbonaceous chondrites have black fusion crust on exterior surfaces. A few have evaporites. The interiors are a black matrix with gray to white inclusion/chondrules and some oxidation.
Thin Section Description (,2) - Cari Corrigan, Tim McCoy, Pamela Salyer
These sections consist of abundant small (up to 1 mm) chondrules, chondrule fragments and mineral grains in a dark matrix. Metal and sulfide occur both within and rimming the chondrules. Olivine ranges in composition from Fa0-68, with a continuous range of intermediate compositions. Pyroxenes range Fs1-10Wo1-3 with one outlier of Fs46. The matrix appears to consist largely of Fe-rich olivine. These meteorites are CO3 chondrites and are likely paired with the large MIL CO3 pairing group.
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)
Catalogs:
Search for this meteorite in the NASA/JSC database (U.S.):