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Carbon isotopic evidence for methane hydrate instability during quaternary interstadials
1Geological Sciences and Marine Science Institute, University of California, Santa Barbara, CA 93106, USA. Department of Geological Sciences, California State University, Long Beach, CA 90840, USA.
Methane hydrate dissociation in marine sediments caused large carbon isotopic shifts over 60,000 years. These events, linked to climate shifts, released methane, impacting atmospheric composition.
Area of Science:
- Paleoceanography
- Marine geochemistry
- Climate science
Background:
- Millennial-scale carbon isotopic oscillations observed in benthic foraminifera from the Santa Barbara Basin.
- These oscillations suggest changes in sedimentary methane gradients and gas hydrate dissociation over the last 60,000 years.
Purpose of the Study:
- To investigate the causes of millennial-scale carbon isotopic oscillations in the Santa Barbara Basin.
- To understand the role of gas hydrate dissociation in these oscillations and their potential impact on atmospheric methane.
Main Methods:
- Analysis of benthic and planktonic foraminiferal carbon isotopes over the last 60,000 years.
- Correlation of isotopic data with paleoceanographic proxies and climate records.
Main Results:
- Large millennial-scale carbon isotopic oscillations (approx. 5 per mil) reflect methane outgassing from gas hydrate dissociation during interstadials.
- Brief, negative excursions (up to -6 per mil) indicate massive methane releases from basin sediments.
- Gas hydrate stability was influenced by intermediate-water temperature changes linked to thermohaline circulation shifts.
Conclusions:
- Methane hydrate dissociation and subsequent methane release significantly impacted millennial-scale carbon cycles.
- These processes likely contributed to widespread atmospheric methane oscillations along the California margin and potentially globally.
- Thermohaline circulation played a key role in modulating gas hydrate stability.
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