Introduction: Since January 2004, OMEGA/Mars Express data has revealed a diverse and complex Martian surface mineralogy [1]. The important findings, together with Thermal Emission Spectrometer (TES), Thermal Emission Imaging System (THEMIS), and insitu observations from Mars Exploration Rovers, include but not limited to (1) hydrated sulfates [1, 2, 3, 4, 5, 6, 7]; (2) iron oxides and oxhydroxi...