Article ID Journal Published Year Pages File Type
10701605 Icarus 2013 11 Pages PDF
Abstract
► Gypsum is resistant to dehydration on Mars due to low temperatures. ► Gypsum dehydration is limited to local areas which experienced high temperatures. ► Anhydrite remains stable below 1%RH. ► Bassanite is the expected dehydration product. ► Bassanite is likely restricted to mid and low latitudes.
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Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Space and Planetary Science
Preview
Constraints on the distribution of CaSO4·nH2O phases on Mars and implications for their contribution to the hydrological cycle
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