GEOCHEMICAL MODELING OF SERPENTINIZATION REACTIONS THAT INFLUENCE THE CHEMISTRY AND MICROBIAL ECOSYSTEMS OF THE HYPERALKALINE AQUA DE NEY SPRING, NORTHERN CALIFORNIA, USA
The Ney Spring consists of a sodium bicarbonate water (TDS ~40,000 ppm) with significant amounts of chloride (~8000 ppm) and silica (~4000 ppm). The Ney waters are very distinct in their oxygen and hydrogen stable isotope geochemistry (δ18O = 5.5‰, δD = -14‰) in comparison with local meteoric waters (δ18O = -12.1‰, δD = -85‰), suggesting a potential marine component to the fluids. One distinguishing feature of the Ney Spring is that, in addition to the high pH (>12) fluids, it also emits a large fraction (>80 mole % of the noncondensable gas) of methane. Two distinct processes have been identified as potential mechanisms to generate methane. The first is via an abiotic process, where hydrogen generated by the oxidation of Fe2+ is then reacted with CO2 to form methane. An alternative process would involve microbes that consume hydrogen as an energy source, producing methane as a byproduct.
The Ney Spring has seen renewed interest recently for its potential value as an analog for the briny, subsurface oceans of icy moons in our outer solar system, which have the potential to support chemosynthetic microbial life. The primary focus of our research project is the microbial communities and their metabolisms that persist in the Ney Spring waters. However, for this presentation, we will summarize our geochemical modeling to evaluate how abiotic processes have led to the generation of this unusual spring chemistry.