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- W2028145211 abstract "A Venus simulator has been constructed to duplicate the atmospheric temperature, pressure, and (approximate) gas composition for all surface elevations on Venus. Within the Simulator environment, particles are impacted against rock targets as a means of studying aeolian processes on the planet. Preliminary results show that particles are abraded even at the very low-impact velocities likely to occur on Venus. However, the same particles do not produce abrasion of basaltic rock when impact velocities are less than 1 m/sec. Instead, comminution debris from particles is transferred onto rock surfaces to form an accretionary layer. The lack of rock abrasion and the development of accretionary layers are interpreted to be a function of elevated temperature (>660°K). On Venus, accretionary material could effectively change the surface chemistry of rocks in aeolian regions and may act as a mechanical or chemical cushion against weathering processes." @default.
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- W2028145211 date "1988-06-01" @default.
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- W2028145211 title "Aeolian weathering of Venusian surface materials: Preliminary results from laboratory simulations" @default.
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- W2028145211 doi "https://doi.org/10.1016/0019-1035(88)90117-0" @default.
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