The electron-proton bottleneck of photosynthetic oxygen evolution
- PMID: 37138082
- PMCID: PMC10191853
- DOI: 10.1038/s41586-023-06008-5
The electron-proton bottleneck of photosynthetic oxygen evolution
Abstract
Photosynthesis fuels life on Earth by storing solar energy in chemical form. Today's oxygen-rich atmosphere has resulted from the splitting of water at the protein-bound manganese cluster of photosystem II during photosynthesis. Formation of molecular oxygen starts from a state with four accumulated electron holes, the S4 state-which was postulated half a century ago1 and remains largely uncharacterized. Here we resolve this key stage of photosynthetic O2 formation and its crucial mechanistic role. We tracked 230,000 excitation cycles of dark-adapted photosystems with microsecond infrared spectroscopy. Combining these results with computational chemistry reveals that a crucial proton vacancy is initally created through gated sidechain deprotonation. Subsequently, a reactive oxygen radical is formed in a single-electron, multi-proton transfer event. This is the slowest step in photosynthetic O2 formation, with a moderate energetic barrier and marked entropic slowdown. We identify the S4 state as the oxygen-radical state; its formation is followed by fast O-O bonding and O2 release. In conjunction with previous breakthroughs in experimental and computational investigations, a compelling atomistic picture of photosynthetic O2 formation emerges. Our results provide insights into a biological process that is likely to have occurred unchanged for the past three billion years, which we expect to support the knowledge-based design of artificial water-splitting systems.
© 2023. The Author(s).
Conflict of interest statement
The authors declare no competing interests.
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Comment in
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Clues to how water splits during photosynthesis.Nature. 2023 May;617(7961):468-469. doi: 10.1038/d41586-023-01388-0. Nature. 2023. PMID: 37138059 No abstract available.
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