The emergence of oxygenic photosynthesis through the lens of carbonate diagenesis

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The most important evolutionary innovation in Earth history was the emergence of oxygenic photosynthesis. The evolution of this microbial metabolism eventually drove the rise of oxygen in the atmosphere, fundamentally changing all biogeochemical cycles, and setting the stage for the subsequent evolution of multi-cellular life. However, the timing, causes, and consequences of this evolutionary singularity are largely unresolved. Currently, theories on the origin of oxygenic photosynthesis are divided. While some studies favor an early origin of oxygenic photosynthesis, ~600 million years prior to the rise of oxygen in the atmosphere, others have argued that oxygenic photosynthesis arose just prior to the Great Oxidation Event (~2.3-3.4 billion years ago). This controversy is intrinsically linked to the complications associated with interpreting geochemical data from billion-year-old Archean rocks. The history of oxygen on Earth has in part been reconstructed using geochemical data from ancient sediments, such carbonates. These chemical sediments are composed of cations (e.g., Ca2+, Mg2+) and carbonate ions whose composition, at least initially, reflects the chemical and isotopic composition of contemporaneous seawater. However, one of the main limitations in using this geochemical archive is the susceptibility of carbonate sediments to diagenesis, the process where unlithified sediments are transformed into the rocks we can study today. For billion-year-old carbonates diagenetic alteration is the rule rather than the exception and extensive recrystallization has modified the geochemical signals that are preserved in the rock record. These post-depositional processes are major obstacles for our ability to accurately infer oxygen levels before the GOE. In contrast to common attempts of trying to avoid diagenesis, the research program outlined in this proposal seeks to extract the primary chemical information from ancient carbonate sediments by mapping out and better understanding the diagenetic processes. By combining calcium isotope measurements, synchrotron X-ray analyses of Mn and Fe minerals, and numerical diagenetic models, it is possible to constrain the diagenetic history of carbonates. When paring these techniques with textural observations, it is possible to `see through' diagenesis and more accurately reconstruct past seawater chemistry. The pursuit of reconstructing ancient environments through the lens of carbonate diagenesis is not only relevant to Archean studies, but is pertinent to all studies using the geochemistry of carbonates as proxies for ancient environmental conditions. Consequently, this framework is both highly original and likely to lead to ground-breaking advances in our understanding of the emergence of oxygenic photosynthesis and the evolutionary history of life throughout Earth history.