Laboratory‐simulated acid‐sulfate weathering of basaltic materials: Implications for formation of sulfates at Meridiani Planum and Gusev crater, Mars

Acid‐sulfate weathering of basaltic materials is a candidate formation process for the sulfate‐rich outcrops and rocks at the MER rover Opportunity and Spirit landing sites. To determine the style of acid‐sulfate weathering on Mars, we weathered basaltic materials (olivine‐rich glassy basaltic sand and plagioclase feldspar‐rich basaltic tephra) in the laboratory under different oxidative, acid‐sulfate conditions and characterized the alteration products. We investigated alteration by (1) sulfuric‐acid vapor (acid fog), (2) three‐step hydrothermal leaching treatment approximating an “open system,” and (3) single‐step hydrothermal batch treatment approximating a “closed system.” In acid fog experiments, Al‐, Fe‐, and Ca‐sulfates and amorphous silica formed from plagioclase‐rich tephra, and Mg‐ and Ca‐sulfates and amorphous silica formed from the olivine‐rich sands. In three‐step leaching experiments, only amorphous Si formed from the plagioclase‐rich basaltic tephra, and jarosite, Mg‐, and Ca‐sulfates and amorphous silica formed from olivine‐rich basaltic sand. Amorphous silica formed under single‐step experiments for both starting materials. On the basis of our experiments, jarosite formation in Meridiani outcrop is potential evidence for an open system acid‐sulfate weathering regime. Waters rich in sulfuric acid percolated through basaltic sediment, dissolving basaltic phases (e.g., olivine) and forming jarosite, other sulfates, and iron oxides. Aqueous alteration of outcrops and rocks on the West Spur of the Columbia Hills may have occurred when vapors rich in SO 2 from volcanic sources reacted with basaltic materials. Soluble ions from the host rock (e.g., olivine) reacted with S to form Ca‐, Mg‐, and other sulfates along with iron oxides and oxyhydroxides.