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USGS · 70218480

The contribution of water radiolysis to marine sedimentary life

Abstract

Water radiolysis continuously produces H 2 and oxidized chemicals in wet sediment and rock. Radiolytic H 2 has been identified as the primary electron donor (food) for microorganisms in continental aquifers kilometers below Earth’s surface. Radiolytic products may also be significant for sustaining life in subseafloor sediment and subsurface environments of other planets. However, the extent to which most subsurface ecosystems rely on radiolytic products has been poorly constrained, due to incomplete understanding of radiolytic chemical yields in natural environments. Here we show that all common marine sediment types catalyse radiolytic H 2 production, amplifying yields by up to 27X relative to pure water. In electron equivalents, the global rate of radiolytic H 2 production in marine sediment appears to be 1-2% of the global organic flux to the seafloor. However, most organic matter is consumed at or near the seafloor, whereas radiolytic H 2 is produced at all sediment depths. Comparison of radiolytic H 2 consumption rates to organic oxidation rates suggests that water radiolysis is the principal source of biologically accessible energy for microbial communities in marine sediment older than a few million years. Where water permeates similarly catalytic material on other worlds, life may also be sustained by water radiolysis.

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Justine F. Sauvage, Ashton F. Flinders, Arthur J. Spivack, Robert Pockalny, Ann G. Dunlea, Chloe H. Anderson, David Smith, Richard W. Murray, Steven D’Hondt. 2021-02-26. The contribution of water radiolysis to marine sedimentary life. https://doi.org/10.1038/s41467-021-21218-z

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