Abstract
Evidence continues to emerge for the production and low-level accumulation of molecular oxygen (O(2)) at Earth’s surface before the Great Oxidation Event. Quantifying this early O(2) has proven difficult. Here, we use the distribution and isotopic composition of molybdenum in the ancient sedimentary record to quantify Archean Mo cycling, which allows us to calculate lower limits for atmospheric O(2) partial pressures (PO(2)) and O(2) production fluxes during the Archean. We consider two end-member scenarios. First, if O(2) was evenly distributed throughout the atmosphere, then PO(2) > 10(–6.9) present atmospheric level was required for large periods of time during the Archean eon. Alternatively, if O(2) accumulation was instead spatially restricted (e.g., occurring only near the sites of O(2) production), then O(2) production fluxes >0.01 Tmol O(2)/year were required. Archean O(2) levels were vanishingly low according to our calculations but substantially above those predicted for an abiotic Earth system.