The nakhlite hydrothermal brine on Mars

Water is the basis of habitability; and formation conditions of hydrous alteration minerals are key to temperature and chemical conditions of that water. Using new, detailed observations on nakhlite martian meteorite alteration, composition, temperature and redox conditions of the water that formed the observed hydrous alteration can be determined through thermochemical modelling. We show that the nakhlite parent rocks on Mars encountered a CO2-rich hydrothermal fluid at 150≤T≤200°C, pH 6–8 with a water:rock ratio (W/R) ≤300. Under these conditions, Fe-rich carbonate was precipitated within brittle fractures. As the fluid cooled to 50°C, at pH 9 and W/R of 6, Fe-rich phyllosilicate precipitated, followed in turn by rapid precipitation of an amorphous gel. It was enriched in the most soluble species (e.g. K, Na), of alkaline pH, and similar to terrestrial, i.e. not seawater-influenced, dilute brines in basaltic terrains on Earth. Our results show that environments associated with this type of fluid were habitable, unlike those associated with acid-sulphate fluids. Considering the timing of the nakhlite alteration, the most likely cause is impact-generated hydrothermal alteration of the nakhlite pile at the margins of an impact crater. The martian subsurface fluid forming phyllosilicates provided habitable temperatures and many of the nutrients required for life. ► The first quantitative-determination of a Mars fluid. ► This Mars fluid determination is based on detailed nakhlite meteorite mineralogy. ► The brine is representative of a major subsurface alteration fluid on Mars. ► The brine was dilute and reached 150–200°C. ► The T, pH, and nutrients mean this fluid type was potentially habitable.