The electron-proton bottleneck of photosynthetic oxygen evolution

Abstract

Photosynthesis fuels life on Earth by storing solar energy in chemical form, inspiring technological schemes for sustainable fuel production. Today’s oxygen-rich atmosphere results from photosynthetic O2-production during water-splitting at the protein-bound manganese cluster of photosystem II. Formation of the O2 molecule starts from a state with four accumulated electron holes, the S4-state, postulated half a century ago1 and remaining enigmatic ever since. Here we resolve this missing key element in photosynthetic O2-formation and its crucial mechanistic role. We tracked 230,000 excitation cycles of dark-adapted photosystems with microsecond infrared spectroscopy. Combing these results with computational chemistry reveals that in S4 not only are four electron holes accumulated by metal ion and protein sidechain oxidation, but also a crucial proton vacancy is created through gated sidechain deprotonation. Subsequently, a reactive oxygen radical is formed in an astonishing single-electron multi-proton transfer event. This is the slowest step in photosynthetic O2-formation – despite its low energetic barrier – due to entropic slowdown. In conjunction with previous breakthroughs in experimental and computational investigations, a compelling atomistic picture of photosynthetic O2-formation emerges. Our results provide insight into a biological process that has probably operated in the same unique way for three billion years and are expected to support the knowledge-based design of artificial water-splitting systems.

Solar energy conversion by photosystem II: principles and structures

“…Three channel networks have been identified and variously named (Murray and Barber 2007 ; Ho and Styring 2008 ; Gabdulkhakov et al 2009 ; Guskov et al 2009 ; Vassiliev et al 2010 ; Umena et al 2011 ; Sakashita et al 2017a ). The Cl1 channel has been shown to be crucial for proton egress (Hussein et al 2021 ; Dau et al 2022 ), but also the O4 channel may have that function during the S 0 ⟶ S 1 transition (Sakashita et al 2017a ; Hussein et al 2021 ). All the three channels (Fig.…”

“…Interestingly, the slow kinetic of the S 3 → S 4 → S 0 transition appears to be connected to large entropic contributions rather than a high activation barrier. This indicates that a large number of conformational states may need to be sampled to find the optimal configuration of the Mn 4 CaO 5 cluster and the H-bonding network to allow generation of the S 4 state as well as O 2 formation and release (Zaharieva and Dau 2019 ; Dau et al 2022 ). Lastly, the S 3 → S 4 → S 0 transition is irreversible due to its large driving force (Haumann et al 2008 ; Kolling et al 2009 ; Shevela et al 2011 ; Nilsson et al 2016 ).…”