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Formation of carbonate chimneys in the Mediterranean Sea linked to deep-water oxygen depletion

A Publisher Correction to this article was published on 05 July 2023

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Abstract

Marine sediments at ocean margins vent substantial amounts of methane1,2. Microbial oxidation of the methane released can trigger the precipitation of carbonate within sediments and support a broad diversity of seafloor ecosystems3,4. The factors controlling microbial activity and carbonate precipitation associated with the seepage of submarine fluid over geological time remain poorly constrained. Here, we characterize the petrology and geochemistry of rocks sampled from metre-size build-ups of methane-derived carbonate chimneys located at the Amon mud volcano on the Nile deep-sea fan. We find that these carbonates comprise porous structures composed of aggregated spherules of aragonite, and closely resemble microbial carbonate reefs forming at present in the anoxic bottom waters of the Black Sea5. Using U-series dating, we show that the Amon carbonate build-ups formed between 12 and 7 thousand years ago, contemporaneous with the deposition of organic-rich sediments in the eastern Mediterranean, the so-called sapropel layer S1. We propose that the onset of deep-water suboxic or anoxic conditions associated with sapropel formation resulted in the development of intense anaerobic microbial activity at the sea floor, and thus the formation of carbonate chimneys.

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Figure 1: Bathymetric map of Amon MV and location of studied carbonate samples.
Figure 2: Amon MV carbonate chimneys.
Figure 3: U–Th ages for selected polished sections (build-up 1).

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Acknowledgements

We thank the crews of RV Meteor and ROV QUEST4000 (MARUM, University of Bremen, Germany), and all participants of the BIONIL cruise (M70/2; chief scientist: A. Boetius), for their assistance at sea. We acknowledge Y. Germain, E. Rongemaille, A. Roubi and C. Bassoullet for help in the laboratory at IFREMER and Institut Universitaire Européen de la Mer (I.U.E.M.), respectively. We are very grateful to G. M. Henderson for providing the U–Th spike, and also thank A. Crémière, E. Ducassou, J-P. Foucher, T. Himmler and V. Liebetrau for helpful discussions. This work was financially supported through the ESF EUROCORES project MEDIFLUX, the EU 6th FP HERMES project (GOCE-CT-2005-511234-1), the EU 7th FP HERMIONE project (contract 226354) and IFREMER. Further financial support came from the Liebniz programme of the DFB to A.B. and Max Planck Society.

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G.B., S.D., J.M. and A.B. conceived the project and participated in the BIONIL cruise (RV Meteor). G.B. performed sample/chemical preparation, and wrote the article. G.B., E.P., J.E., S.C. and C.P. analysed the samples. All authors contributed to discussions, interpretation of the results and manuscript writing.

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Correspondence to Germain Bayon.

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Bayon, G., Dupré, S., Ponzevera, E. et al. Formation of carbonate chimneys in the Mediterranean Sea linked to deep-water oxygen depletion. Nature Geosci 6, 755–760 (2013). https://doi.org/10.1038/ngeo1888

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