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Published July 2021 | Supplemental Material + Published
Journal Article Open

Carbon cycle inverse modeling suggests large changes in fractional organic burial are consistent with the carbon isotope record and may have contributed to the rise of oxygen

Abstract

Abundant geologic evidence shows that atmospheric oxygen levels were negligible until the Great Oxidation Event (GOE) at 2.4–2.1 Ga. The burial of organic matter is balanced by the release of oxygen, and if the release rate exceeds efficient oxygen sinks, atmospheric oxygen can accumulate until limited by oxidative weathering. The organic burial rate relative to the total carbon burial rate can be inferred from the carbon isotope record in sedimentary carbonates and organic matter, which provides a proxy for the oxygen source flux through time. Because there are no large secular trends in the carbon isotope record over time, it is commonly assumed that the oxygen source flux changed only modestly. Therefore, declines in oxygen sinks have been used to explain the GOE. However, the average isotopic value of carbon fluxes into the atmosphere–ocean system can evolve due to changing proportions of weathering and outgassing inputs. If so, large secular changes in organic burial would be possible despite unchanging carbon isotope values in sedimentary rocks. Here, we present an inverse analysis using a self‐consistent carbon cycle model to determine the maximum change in organic burial since ~4 Ga allowed by the carbon isotope record and other geological proxies. We find that fractional organic burial may have increased by 2–5 times since the Archean. This happens because O₂‐dependent continental weathering of ¹³C‐depleted organics changes carbon isotope inputs to the atmosphere–ocean system. This increase in relative organic burial is consistent with an anoxic‐to‐oxic atmospheric transition around 2.4 Ga without declining oxygen sinks, although these likely contributed. Moreover, our inverse analysis suggests that the Archean absolute organic burial flux was comparable to modern, implying high organic burial efficiency and ruling out very low Archean primary productivity.

Additional Information

© 2021 The Authors. Geobiology published by John Wiley & Sons Ltd. This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited. Issue Online: 21 June 2021; Version of Record online: 25 March 2021; Manuscript accepted: 09 March 2021; Manuscript revised: 08 February 2021; Manuscript received: 08 September 2020. DCC, JKT, and MAK were supported by NSF Frontiers in Earth System Dynamics award No. 1338810. This work was also supported by NASA Exobiology grant NNX15AL23G and Simons Foundation SCOL Awards 511570 and 511570FY20 to DCC. MAK acknowledges support from an NSF Graduate Research Fellowship and an Agouron Institute postdoctoral fellowship. This work was also supported by the NASA Astrobiology Program Grant Number 80NSSC18K0829 and benefited from participation in the NASA Nexus for Exoplanet Systems Science research coordination network. The authors declare no conflict of interest. Data Availability Statement: The Python code used for this analysis is available on the lead author's Github upon publication: https://github.com/joshuakt/Carbon-isotopes-inverse-model

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Published - gbi.12440.pdf

Supplemental Material - gbi12440-sup-0001-supinfo.pdf

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Additional details

Created:
August 22, 2023
Modified:
October 23, 2023