4.1 Article

New lunar meteorite NWA 10986: A mingled impact melt breccia from the highlands-A complete cross section of the lunar crust

Journal

METEORITICS & PLANETARY SCIENCE
Volume 54, Issue 12, Pages 3018-3035

Publisher

WILEY
DOI: 10.1111/maps.13406

Keywords

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Funding

  1. NASA [NNX15AL98G]
  2. Vanderbilt University [3800-019687]
  3. NASA [NNX15AL98G, 807902] Funding Source: Federal RePORTER

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Northwest Africa (NWA) 10986 is a new mingled lunar meteorite found in 2015 in Western Sahara. This impact melt breccia contains abundant impact melt glass and clasts as large as 0.75 mm. Clasts are predominantly plagioclase and pyroxene-rich and represent both highland and basalt lithologies. Highland lithologies include troctolites, gabbronorites, anorthositic norites, and troctolitic anorthosites. Basalt lithologies include crystalline clasts with large zoned pyroxenes representing very low titanium to low titanium basalts. In situ geochemical analysis of minerals within clasts indicates that they represent ferroan anorthosite, Mg-suite, and gabbronorite lithologies as defined by the Apollo sample collection. Clasts representing magnesian anorthosite, or gap lithologies, are prevalent in this meteorite. Whole rock and in situ impact glass measurements indicate low incompatible trace element concentrations. Basalt clasts also have low incompatible trace element concentrations and lack evolved KREEP mineralogy although pyroxferroite grains are present. The juxtaposition of evolved, basaltic clasts without KREEP signatures and highland lithologies suggests that these basaltic clasts may represent cryptomare. The lithologies found in NWA 10986 offer a unique and possibly a complete cross section view of the Moon sourced outside of the Procellarum KREEP Terrane.

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