Name: Miller Range 090076 This is an OFFICIAL meteorite name. Abbreviation: MIL 090076 Observed fall: No Year found: 2009 Country: Antarctica [Collected by US Antarctic Search for Meteorites program (ANSMET)] Mass: 378 g
The exterior has fractured brown/black fusion crust with evaporites. Flow lines are visible on one surface. Areas without fusion crust are weathered brown with some gray/black matrix visible. Some rusty areas are visible. The interior is a dark gray to black matrix with heavy oxidation and rusty areas. Metal is visible and this ureilite was very difficult to break.
Thin Section (,2) Description - Cari Corrigan, Tim McCoy and Linda Welzenbach
The section consists of an aggregate of large (up to 2.5 mm) olivine grains. Individual olivine grains are rimmed by carbon-rich material containing traces of metal. Metal forms veins between olivines. Olivine has cores of Fa22. Pigeonite grains have compositions of Fs11-18 and Wo5-11. The meteorite is a ureilite.
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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