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- W97080652 abstract "Introduction: Spectral analysis of the Libya Montes/Isidis Planitia region using OMEGA spectra noted outcrops of olivine [1]. Observations by CRISM revealed a range of minerals in Libya Montes including olivine, pyroxene, and phyllosilicate minerals [2, 3]. Our spectral analyses of CRISM images in Libya Montes have identified carbonates as well [here and in 4]. We have also prepared laboratory mixtures of phyllosilicate-carbonate, carbonate-olivine, phyllosilicateolivine, and ternary samples and measured their spectra in order to better understand the Libya Montes spectra containing these compounds. Libya Montes is located on the southern rim of the Isidis Basin. Both the Isidis Basin and the mountains of Libya Montes formed in response to a large impact 4.6 – 3.5 Ga [5]. The rocks of Libya Montes are therefore very old and this site was chosen as the study area because it may hold clues for early Martian history. Different mineralogical units are exposed in Libya Montes due to the influences of wind, water, and smaller impact craters. We discuss these mineralogical units and their relationships. Methods: CRISM acquires spectral images ~10 km wide from 0.4 – 4.0 μm in 544 wavelengths with two detectors, one in the visible and one in the infrared, to produce images of 18 meter per pixel [6]. CRISM images were then processed to remove noise [7]. Mineral indicator maps were generated using band parameters selected to highlight specific mineral types [8] in order to identify likely minerals. Results and Discussion: Phyllosilicates, carbonates, olivine, and pyroxene were identified in CRISM images of Libya Montes in this study (e.g. Fig. 1)." @default.
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- W97080652 date "2010-03-01" @default.
- W97080652 modified "2023-09-24" @default.
- W97080652 title "Mineralogy of Libya Montes, Mars and Applications of Phyllosiliate-Carbonate-Olivine Mixtures" @default.
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