4.1 Article

The origin of young mare basalts inferred from lunar meteorites Northwest Africa 4734, 032, and LaPaz Icefield 02205

Journal

METEORITICS & PLANETARY SCIENCE
Volume 49, Issue 2, Pages 261-291

Publisher

WILEY
DOI: 10.1111/maps.12239

Keywords

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Funding

  1. NASA Earth and Space Science Fellowship [NNX12AO15H]
  2. NASA [NNX10AI77G, NNX09AB92G]
  3. U.S. D.O.E. by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]
  4. Lunar Advanced Science and Exploration Research (LASER) [NNX13AK32G]
  5. Ann and Gordon Getty Foundation
  6. NM Space Grant Consortium
  7. NASA [120561, 132119, NNX09AB92G, NNX10AI77G] Funding Source: Federal RePORTER

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Northwest Africa (NWA) 4734 is an unbrecciated basaltic lunar meteorite that is nearly identical in chemical composition to basaltic lunar meteorites NWA 032 and LaPaz Icefield (LAP) 02205. We have conducted a geochemical, petrologic, mineralogic, and Sm-Nd, Rb-Sr, and Ar-Ar isotopic study of these meteorites to constrain their petrologic relationships and the origin of young mare basalts. NWA 4734 is a low-Ti mare basalt with a low Mg* (36.5) and elevated abundances of incompatible trace elements (e.g., 2.00ppm Th). The Sm-Nd isotope system dates NWA 4734 with an isochron age of 3024 +/- 27Ma, an initial epsilon(Nd) of +0.88 +/- 0.20, and a source region Sm-147/Nd-144 of 0.201 +/- 0.001. The crystallization age of NWA 4734 is concordant with those of LAP 02205 and NWA 032. NWA 4734 and LAP 02205 have very similar bulk compositions, mineral compositions, textures, and ages. Their source region Sm-147/Nd-144 values indicate that they are derived from similar, but distinct, source materials. They probably do not sample the same lava flow, but rather are similarly sourced, but isotopically distinct, lavas that probably originate from the same volcanic complex. They may have experienced slightly different assimilation histories in route to eruption, but can be source-crater paired. NWA 032 remains enigmatic, as its source region Sm-147/Nd-144 definitively precludes a simple relationship with NWA 4734 and LAP 02205, despite a similar bulk composition. Their high Ti/Sm, low (La/Yb)(N), and Cl-poor apatite compositions rule out the direct involvement of KREEP. Rather, they are consistent with low-degree partial melting of late-formed LMO cumulates, and indicate that the geochemical characteristics attributed to urKREEP are not unique to that reservoir. These and other basaltic meteorites indicate that the youngest mare basalts originate from multiple sources, and suggest that KREEP is not a prerequisite for the most recent known melting in the Moon.

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