Hydrothermal Signatures at Gale Crater, Mars, and Possible In-Situ Formation of Tridymite

The occurrence of tridymite, a high temperature SiO2 polymorph definitively identified by the Curiosity rover in the Buckskin mudstone sample at Gale crater, Mars, has been attributed to detrital accumulation of rhyolitic material. This interpretation of a detrital origin is revisited in light of the observation that the tridymite-hosting sediments appear to have interacted with the same fluids that produced alteration halos in the overlying sandstone. The alteration halos in the Stimson sandstone are light-toned, elevated silica zones within 50 cm of a central fracture. They have likely experienced chemical leaching under acidic conditions resulting in depletion of metals (including Al), retention of Ti, formation of amorphous iron sulfates, 50% reduction of the pyroxene:plagioclase ratio, a factor of two increase in the Fe/Mn ratio, and passive enrichment of Si. This alteration is not constrained (nor precluded) to have occurred at elevated temperatures, but there are abundant indicators of hydrothermal activity within Gale crater. High concentrations of Ge, Zn, Ni, Pb, Cu, Se and Ga in a variety of samples analyzed by the Alpha Particle X-ray Spectrometer are indicative of mobility in hydrothermal solutions. Mineralogy of Gale crater samples determined by the CheMin X-ray diffraction instrument includes phases which may be associated with hydrothermal activity (smectites, anhydrite, hematite), but definitive detections of mineral assemblages that are necessarily hydrothermal in origin remain absent. The nearly identical patterns of enriched and depleted elements of the Stimson alteration halos (relative to parent rocks) and the tridymite-bearing unit (relative to typical mudstone samples) require the consideration of co-genetic origins. Cristobalite, a SiO2 polymorph stable above 1470°C found in the Buckskin sample, is known to form in hydrothermal solutions at temperatures well below its stability field (Henderson et al., 1971). Formation of well-crystalline tridymite at temperatures below its thermodynamic stability range (870-1470°C) has not been established, but cannot be excluded. Thus, the possibility that the fluids responsible for the passive enrichment of silica in the Stimson alteration halos also resulted in the in-situ formation of tridymite deserves further consideration.