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- W1680853612 abstract "After two years of operation, the OMEGA imaging spectrometer on-board Mars Express has acquired data coverage of the Martian surface with spatial resolution varying between 300 m and 4.8 km depending on the pericentre altitude of the spacecraft's elliptical orbit. We report the global surface distributions of some minerals using the OMEGA observations in the Visible and Near Infrared (VNIR) wavelength domains (0.35-2.5 μm). Global maps of ferric phases, mafic minerals (pyroxenes, olivines) and hydrated minerals have been derived from spectral parameters. The limits of detection in term of abundance for some minerals of different grain size distributions are given. The distribution of pyroxenes is in general agreement with the mineral maps of previous telescopic and space observations. The Fe absorption feature in the visible wavelength region is present everywhere on the surface. The spectra of the bright regions compare with anhydrous nanophase ferric oxides. Terrains with water bearing minerals cover a very small fraction of the Martian surface. Olivine (Mg-rich compositions) is detected in more extensive regions of the pyroxene-rich zones than" @default.
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- W1680853612 date "2006-12-01" @default.
- W1680853612 modified "2023-09-26" @default.
- W1680853612 title "Martian Surface Mineralogy from OMEGA/MEx: Global mineral maps" @default.
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