Name: Miller Range 090031 This is an OFFICIAL meteorite name. Abbreviation: MIL 090031 Observed fall: No Year found: 2009 Country: Antarctica [Collected by US Antarctic Search for Meteorites program (ANSMET)] Mass: 500 g
Black fusion crust covers 60% of the exterior with oxidation haloes. Areas without fusion crust are rusty brown and fractures penetrate the surface. The interior matrix is dark gray to black with discontinuous oxidation rind and rusty areas. Some crystalline faces are visible in the coarse grained texture.
Thin Section Description (,2) - Cari Corrigan, Tim McCoy and Nicole Lunning
The section consists of an aggregate of large olivine and pyroxene grains up to 2 mm across. Individual olivine grains are rimmed by carbon-rich material containing traces of metal. The olivines have been mosaicized by shock. Olivines has cores of Fa20, with rims reduced to Fa15. Pigeonite (Fs17,Wo8) exhibits a blotchy appearance. The meteorite is a ureilite.
JSC: Mailcode KT, 2101 NASA Parkway, NASA Johnson Space Center, Houston, TX 77058, United States; Website (institutional address; updated 3 Sep 2013) 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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