Science - Rich Mission Sites within South Pole - Aitken Basin , Part 1 : Antoniadi
نویسندگان
چکیده
CRATER. A. L. Fagan, M. E. Ennis, J. N. Pogue, S. Porter, J. F. Snape, C. R. Neal, and D. A. Kring; Department of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, IN, USA [email protected]; Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN, USA [email protected]; Earth and Planetary Sciences Department, University of California, Santa Cruz, CA, USA [email protected]; School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA [email protected]; Department of Earth Sciences, University College London, UK [email protected]; 6 Department of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, IN, USA [email protected]; 7 Lunar and Planetary Institute, Houston, TX, USA [email protected].
منابع مشابه
Potential Sample Sites for South Pole–aitken Basin Impact Melt within the Schrödinger Basin
anomaly that coincides with the SPA interioris exposed in the eastern and southeastern portion of this basin. This FeOenriched signature is interpreted to represent SPA-derived material, and samples collected within this region may be analyzed to determine the age of the oldest basin preserved on the Moon. Red and pink pixels indicate the presence of pyroxene and plagioclase [10], a signature t...
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CRATER. J. F. Snape, A. L. Fagan, M. E. Ennis, J. N. Pogue, S. Porter, C. R. Neal, and D. A. Kring; Department of Earth Sciences, University College London, UK [email protected]; Department of Civil Engineering and Geological Sciences, University of Notre Dame, Notre Dame, IN, USA [email protected]; Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN, USA mennis2@ut...
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The distribution and the geological context of the olivine-rich exposures in the South Pole-Aitken (SPA) Basin on the Moon were investigated based on the spectral data obtained from the Spectral Profiler (SP) and Multiband Imager (MI) onboard the Japanese lunar explorer Kaguya/SELENE. The olivine-rich exposures are found only in the peak rings or central peaks of the Schrödinger basin and Zeema...
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Introduction: Lunar meteorite Dhofar 961, a complex, lithic-clast-rich impact breccia [1,2], was called out by [3-6] as a candidate for an origin in the South Pole – Aitken (SPA) Basin region of the Moon (the SPA Terrane) on the basis of its relatively mafic, but nonmare lithologic and major-element chemical composition. It also has an incompatible-element signature that differs from the KREEP-...
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