Constraints on the Origin of Martian Clay Minerals from Thermal Infrared Spectroscopy and Thermal Inertia

Details Constraints on the Origin of Martian Clay Minerals from Thermal Infrared Spectroscopy and Thermal Inertia Constraints on the Origin of Martian Clay Minerals from Thermal Infrared Spectroscopy and Thermal Inertia

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpico1353.3036m&link_type=abstract

Seventh International Conference on Mars, held July 9-13, 2007 in Pasadena, California, LPI Contribution No. 1353, p.3036

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Scientific paper

Ancient clay mineral deposits of major geological and astrobiological
significance were previously discovered with OMEGA spectral data. We
investigate these deposits with TES and THEMIS data to further constrain
their mineralogy and geologic origin.

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