PP12A-08:
Oxygen Oases Before and After the GOE: Insights From Metals and Models

Monday, 15 December 2014: 12:05 PM
Stephanie L Olson1, Christopher T Reinhard2, Noah J Planavsky3, Timothy W Lyons1, Moutusi Roy4 and Ariel D Anbar4, (1)University of California Riverside, Riverside, CA, United States, (2)Georgia Institute of Technology, Atlanta, GA, United States, (3)Yale University, New Haven, CT, United States, (4)Arizona State University, Tempe, AZ, United States
Abstract:
The evolution of oxygenic photosynthesis fundamentally changed the structure of the marine biosphere and the chemistry of Earth’s ocean-atmosphere system. Atmospheric oxygenation, however, was decoupled from the onset of biological O2 production—possibly lagging by as much as half a billion years—and O2 remained low for two billion years following initial O2 accumulation. Although uncertainties remain regarding the fate of biogenic O2 during the Precambrian, it is becoming clear that the consequences of oxygenesis were both spatially and temporally variable. Several lines of evidence support the existence of aerobic ecosystems associated with O2 oases within an otherwise anoxic Archean ocean; however—with notable exceptions—atmospheric O2 remained low enough to severely curtail oxidative weathering processes on long-term average throughout the Archean. During the subsequent Great Oxidation Event (GOE) in the early Paleoproterozoic, atmospheric O2 irreversibly increased above the sensitivity thresholds of several well-established proxies, but the level at which O2 eventually stabilized remains unclear. Consequently, the dynamics of O2 cycling are poorly characterized both before and after the GOE. Nevertheless, recent analytical and numerical results suggest exceptionally low O2 levels that may have favored Archean-style O2 oases in the mid-Proterozoic.

We used Fe speciation and trace metal records from Precambrian shales, including data from two new cores that target the 2.7 Ga Roy Hill Shale, to investigate pre- and post- GOE redox heterogeneity in Earth’s surface environments. Fe speciation supports the reconstruction of local marine redox conditions, and, in this context, trace metals can allow glimpses of redox conditions beyond the local environment, which may have throttled the supply of key redox-sensitive trace metals to the ocean. Then, using O2 constraints derived from these inorganic proxies, we use an Earth System model to explore C, O, and nutrient cycling in the late Archean and into the mid-Proterozoic. Although our results allow profound perturbation to several biogeochemical cycles and the climate system as a result of the GOE, we find that the GOE may have had only minor significance for the long-term average O2 content of typical surface seawater in the Proterozoic.