Basalt and olivine dissolution under cold, salty, and acidic conditions: What can we learn about recent aqueous weathering on Mars?

To test which variables may be important for weathering on Mars, the effects of temperature (22°C, 6°C, and −19°C), high ionic strength, and oxygen concentrations were investigated in batch dissolution experiments containing forsterite, fayalite, and basalt glass. CaCl 2 ‐NaCl‐H 2 O brine can remain liquid to temperatures of −55°C and thus may be liquid in the cold, dry climate that currently characterizes Mars. To understand weathering under such conditions, dissolution rates were measured in experiments in distilled water with and without CaCl 2 and NaCl. As observed by others, dissolution rates increased with temperature, and only fayalite dissolution was significantly affected by the presence or absence of oxygen. Enhanced fayalite dissolution under anoxic conditions suggests that Fe‐rich olivine would dissolve more rapidly than Mg‐rich olivine on Mars. Dissolution in the two most dilute experimental solutions (deionized water and CaCl 2 ‐NaCl‐H 2 O solution of ionic strength = 0.7 m) were the same within uncertainty, but apparent dissolution rate constants in CaCl 2 ‐NaCl‐H 2 O brines were significantly slower. Steady silica concentrations are decreased in the brines, consistent with other work, and precipitation rates of silica decrease with decreasing temperatures. These results suggest that enhanced silica precipitation could be an indicator of high ionic strength solutions on Mars. Consistent with these observations, weathering of basalt has been observed to sometimes be accompanied by precipitated layers of silica in cold, dry environments on Earth. If dissolution on Mars occurs or occurred under conditions similar to our experiments, cation leaching would be expected to be accompanied by silica precipitates on weathering surfaces.