Shawn Wright Institute of Meteoritics Department of Earth and Planetary Sciences University of New Mexico
Wednesday, May 6th
1pm CSL 422
Hundreds of thousands of impact craters dominate the surfaces of the Moon, Mercury, and Mars. There exists much geomorphic and spectral evidence for basalt on those surfaces, so basaltic target rocks are most likely common. However, little work has been done on the thermal infrared (TIR) spectroscopy of shocked basalt metamorphosed by meteorite impact. more...
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