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- W2247648988 abstract "Sulphate minerals could be the key to understanding aqueous processes and identifying habitable zones on Mars. Major advances in our knowledge of Martian sulphates have recently been made by the Mars Exploration Rover team (Squyres et al., 2004) and the Mars Express team (Bibring et al., 2005) but many puzzling problems still remain. Could hydrated sulphates be the source of mid-latitude hydrogen found by the Mars Odyssey Neutron Detector? (Feldman et al., 2004; Vaniman et al., 2004) Could Martian sulphate deposits provide favorable conditions for life? (Clark, 1978; Rothschild, 1990; Benison and La Clair, 2003) Did sulphate deposits form as evaporites - left behind when water disappeared from Mars, or as hydrothermal deposits - where water, driven by subsurface heat, deposited sulphate minerals on the surface of Mars? Martian maps showing sulphate hydration state and cation type could help answer all these questions. The next generation of Mars spacecraft is now on its way to Mars. Onboard is the most advanced space borne reflectance spectrometer ever built. This project is designed to study the absorption bands of various key sulfate minerals in order to learn more about their origin, cation and hydration states by studying several low hydration Ca and Mg sulphates. This information will be used to interpret future Mars data and expand the understanding of the Martian hydrological cycle." @default.
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- W2247648988 date "2005-01-01" @default.
- W2247648988 modified "2023-10-14" @default.
- W2247648988 title "Hyperspectral Imaging of Sulphates on Mars" @default.
- W2247648988 hasPublicationYear "2005" @default.
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