CHLORIDE HYDRATES -- SOURCE MATERIALS FOR RECURRING SLOPE LINEAE (RSL) ON MARS
We conducted two sets of experiments to test this hypothesis: (1) deliquescence of six chloride hydrates at three temperatures (T) and ten relative humidity (RH) levels; (2) formation of chloride hydrates at low T (-78°C) through vapor-solid reaction. We found that at 5°C< T <50°C, deliquescence-solid boundaries of many chloride hydrates occur near 33%RH. For comparison, the similar boundary of Mg-, Fe2+-, Fe3+-sulfates occur at 85-95%RH, 95-100% RH, 75-80%RH. It means the deliquescence of chloride hydrates is much easier to start at the raising of T, than the deliquescence of sulfates, and the mid-high RH maintained in a subsurface salty layer can provide suitable RH environment for it at present-day Mars. Furthermore, we found the rate of deliquescence of chloride hydrates has strong temperature dependence. At T range relevant to RSL sites during Mars summer, the deliquescence of CaCl2.2H2O and MgCl2.6H2O can accomplish within hours or days. Finally, we have successfully demonstrated the formations of several MgCl2.xH2O at -78°C through vapor-solid reactions.
These experimental results support a model that the deliquescence of subsurface chloride hydrates would generate RSL on equator-facing slope during Mars summer, then recharging could happen during cold seasons by cold-trapping atmospheric H2O vapor.