Abstract

Abstract. Geological records reveal a number of ancient, large and rapid negative excursions of the carbon-13 isotope. Such excursions can only be explained by massive injections of depleted carbon to the Earth system over a short duration. These injections may have forced strong global warming events, sometimes accompanied by mass extinctions such as the Triassic-Jurassic and end-Permian extinctions 201 and 252 million years ago, respectively. In many cases, evidence points to methane as the dominant form of injected carbon, whether as thermogenic methane formed by magma intrusions through overlying carbon-rich sediment or from warming-induced dissociation of methane hydrate, a solid compound of methane and water found in ocean sediments. As a consequence of the ubiquity and importance of methane in major Earth events, Earth system models for addressing such events should include a comprehensive treatment of methane cycling but such a treatment has often been lacking. Here we implement methane cycling in the Danish Center for Earth System Science (DCESS) model, a simplified but well-tested Earth system model of intermediate complexity. We use a generic methane input function that allows variation in input type, size, timescale and ocean–atmosphere partition. To be able to treat such massive inputs more correctly, we extend the model to deal with ocean suboxic/anoxic conditions and with radiative forcing and methane lifetimes appropriate for high atmospheric methane concentrations. With this new model version, we carried out an extensive set of simulations for methane inputs of various sizes, timescales and ocean–atmosphere partitions to probe model behavior. We find that larger methane inputs over shorter timescales with more methane dissolving in the ocean lead to ever-increasing ocean anoxia with consequences for ocean life and global carbon cycling. Greater methane input directly to the atmosphere leads to more warming and, for example, greater carbon dioxide release from land soils. Analysis of synthetic sediment cores from the simulations provides guidelines for the interpretation of real sediment cores spanning the warming events. With this improved DCESS model version and paleo-reconstructions, we are now better armed to gauge the amounts, types, timescales and locations of methane injections driving specific, observed deep-time, global warming events.

Highlights

  • Analyses of carbonate and organic carbon samples have revealed, with ever-finer time resolution, a number of large and rapid negative carbon isotope excursions since the Cambrian radiation of life about 540 million years ago

  • As for oxidation with dissolved oxygen in the original Danish Center for Earth System Science (DCESS) model (Shaffer et al, 2008), we consider that organic matter formed in the ocean surface layer consists of proteins and lipids in addition to carbohydrates and adopt the mean composition proposed by Anderson (1995)

  • Additional bisulfide is produced by microbes for anoxic conditions by way of anoxic methane oxidation (AMO)

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Summary

Introduction

Analyses of carbonate and organic carbon samples have revealed, with ever-finer time resolution, a number of large and rapid negative carbon isotope excursions since the Cambrian radiation of life about 540 million years ago. The most likely explanations for the carbon isotope excursions and associated global warming events involve thermogenic methane and/or methane hydrate inputs (Berner, 2002; Hesselbo et al, 2000; McElwain et al, 2005; Retallack and Jahren, 2008; Ruhl et al, 2011; Svensen, H. et al, 2004; Shaffer et al, 2016). Thermogenic methane and carbon dioxide are produced when magma intrudes into overlying sediments containing old organic carbon Many more such intrusions would be expected in association with increased volcanism that creates large igneous provinces and such provinces tend to correlate in time with the ancient carbon isotope excursions (Svensen et al, 2004). We present some test simulations of deep-time global warming events using this extended model to illustrate ways forward for future model data analyses

The DCESS model up to now
Atmosphere
Simplified nitrogen and sulfur cycling
Methane oxidation and air–sea gas exchange
Methane input specification
Pre-event steady state and a long sample simulation
Modeled ocean distributions
Modeled ocean sediment properties and synthetic sediment cores
Findings
Discussion and conclusions
Full Text
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