Characterization of ferric hydroxysulfate on Mars and implications of the geochemical environment supporting its formation

This dataset contains the files associated with the journal article "Bishop et al (2025). Characterization of ferric hydroxysulfate on Mars and implications of the geochemical environment supporting its formation. Nature Communications"

Sulfate minerals are significant components of the martian surface and provide clues about the martian geochemical environment. One unusual Fe-sulfate phase has been intriguing Mars scientists for over a decade due to its unique spectral bands that are distinct from any known minerals and its occurrence in layered sedimentary rocks. Ferric hydroxysulfate (Fe³⁺SO₄OH) is formed by heating hydrous Fe²⁺ sulfates to 100 °C or above and has a strong spectral band at 2.236 µm, similar to the spectral feature observed on Mars at Aram Chaos and on the plateau above Juventae Chasma. We describe here detection of this new ferric hydroxysulfate phase and its implications for the geochemical history of Mars. Hydrated sulfates at these locations likely formed through evaporative processes or low-temperature alteration. In contrast, Fe³⁺SO₄OH is more consistent with heating and oxidation of hydrated ferrous sulfates, potentially through deposition of lava, ash, or through hydrothermal processes.