2013
DOI: 10.1073/pnas.1308958110
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Anoxic photochemical oxidation of siderite generates molecular hydrogen and iron oxides

Abstract: Photochemical reactions of minerals are underappreciated processes that can make or break chemical bonds. We report the photooxidation of siderite (FeCO3) by UV radiation to produce hydrogen gas and iron oxides via a two-photon reaction. The calculated quantum yield for the reaction suggests photooxidation of siderite would have been a significant source of molecular hydrogen for the first half of Earth's history. Further, experimental results indicate this abiotic, photochemical process may have led to the fo… Show more

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Cited by 47 publications
(44 citation statements)
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“…3). In Archean oceans, H 2 was undoubtedly a major source of reducing power (17,18,39,40). Metabolic strategies among ancient microbial consortia (Fig.…”
Section: Does the Largest Subnetwork Contain Components Of Metabolicmentioning
confidence: 99%
“…3). In Archean oceans, H 2 was undoubtedly a major source of reducing power (17,18,39,40). Metabolic strategies among ancient microbial consortia (Fig.…”
Section: Does the Largest Subnetwork Contain Components Of Metabolicmentioning
confidence: 99%
“…Most researchers discuss Fe II photo-oxidation (Cairns-Smith 1978, and the later work of Braterman et al 1983;Borowska and Mauzerall 1986;Lundgreen et al 1989;Kim et al 2013). Short wave-length UV-C light (maximum at 267 nm; Kim et al 2013) in controlled laboratory experiments created Fe II photo-oxidation, as opposed to Fe III photo-reduction, which is induced by light over a wider range of wavelengths (200 to 450 nm, maximum at 300 nm, David and David 1976). In the absence of a protective ozone layer in the upper atmosphere, UV-C radiation could have easily penetrated Mars' thin atmosphere, as it presumably did the atmosphere of early Earth.…”
Section: Comparison Between Mineralogical Features Of Copahue-caviahumentioning
confidence: 99%
“…Much of the research on this type of metabolism has been conducted on mesophilic organisms; however, dissimilatory iron reduction is also an important terminal electron-accepting process in many geothermally heated ecosystems (3)(4)(5). Conditions in these hot environments are similar to those found on early Earth when Fe(III) was continuously being formed by photochemical oxidation of Fe(II) in archaean seas and from hydrothermal vent fluids (6)(7)(8). Therefore, any information regarding mechanisms involved in dissimilatory Fe(III) reduction by hyperthermophilic archaea isolated from these environments not only will shed light on present-day biogeochemical cycling patterns but also may provide information about what may have been occurring when life first appeared on the planet.…”
mentioning
confidence: 99%