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Identification of Martian surface minerals can contribute to understand the Martian environmental change and geological evolution as well as explore the habitability of the Mars. The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) aboard the Mars Reconnaissance Orbiter (MRO) is covers the visible to near infrared wavelengths along with enhanced spectral resolution, which provides ability...
Gale Crater on Mars has the layered structure of deposit covered by the Noachian/Hesperian boundary. Mineral identification and classification at this region can provide important constrains on environment and geological evolution for Mars. Although Curiosity rove has provided the in-situ mineralogical analysis in Gale, but it restricted in small areas. Compact Reconnaissance Imaging Spectrometer...
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