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Letter
Nature 448, 1033-1036 (30 August 2007) | doi:10.1038/nature06058; Received 21 February 2007; Accepted 29 June 2007
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Increased subaerial volcanism and the rise of atmospheric oxygen 2.5 billion years ago
Lee R. Kump1 & Mark E. Barley2
- NASA Astrobiology Institute and Department of Geosciences, Pennsylvania State University, 535 Deike Building, University Park, Pennsylvania 16802, USA
- School of Earth and Geographical Sciences, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
Correspondence to: Lee R. Kump1 Correspondence and requests for materials should be addressed to L.R.K. (Email: lkump@psu.edu).
Abstract
The hypothesis that the establishment of a permanently oxygenated atmosphere at the Archaean–Proterozoic transition (
2.5 billion years ago) occurred when oxygen-producing cyanobacteria evolved1 is contradicted by biomarker evidence for their presence in rocks 200 million years older2. To sustain vanishingly low oxygen levels despite near-modern rates of oxygen production from
2.7–2.5 billion years ago thus requires that oxygen sinks must have been much larger than they are now. Here we propose that the rise of atmospheric oxygen occurred because the predominant sink for oxygen in the Archaean era—enhanced submarine volcanism—was abruptly and permanently diminished during the Archaean–Proterozoic transition. Observations3, 4, 5 are consistent with the corollary that subaerial volcanism only became widespread after a major tectonic episode of continental stabilization at the beginning of the Proterozoic. Submarine volcanoes are more reducing than subaerial volcanoes6, so a shift from predominantly submarine to a mix of subaerial and submarine volcanism more similar to that observed today would have reduced the overall sink for oxygen and led to the rise of atmospheric oxygen.
- NASA Astrobiology Institute and Department of Geosciences, Pennsylvania State University, 535 Deike Building, University Park, Pennsylvania 16802, USA
- School of Earth and Geographical Sciences, The University of Western Australia, 35 Stirling Highway, Crawley, WA 6009, Australia
Correspondence to: Lee R. Kump1 Correspondence and requests for materials should be addressed to L.R.K. (Email: lkump@psu.edu).
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