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The influence of sediment thermal maturity and hydrocarbon formation on Hg behaviour in the stratigraphic record
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  • Asri Oktavioni Indraswari,
  • Joost Frieling,
  • Tamsin A. Mather,
  • Alexander Dickson,
  • Hugh Jenkyns,
  • Erdem Idiz
Asri Oktavioni Indraswari
University of Oxford

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Joost Frieling
University of Oxford
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Tamsin A. Mather
University of Oxford
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Alexander Dickson
Royal Holloway University of London
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Hugh Jenkyns
Oxford University
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Erdem Idiz
University of Oxford
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Abstract

While Hg in sediments is increasingly used as a proxy for deep-time volcanic activity, the behaviour of Hg in OM-rich sediments as they undergo thermal maturation is not well understood. In this study, we evaluate the effects of thermal maturation on sedimentary Hg contents and, thereby, the impact of thermal maturity on the use of the Hg/TOC proxy for large igneous province (LIP) volcanism. We investigate three cores (marine organic matter) with different levels of thermal maturity in lowermost Toarcian sediments (Posidonienschiefer) from the Lower Saxony Basin in Germany. We present Hg content, bulk organic geochemistry, and total sulfur in three cores with different levels of thermal maturity. The comparison of Hg data between the three cores indicates that Hg content in the mature/overmature sediments have increased > 2-fold compared to Hg in the immature deposits. Although difficult to confirm with the present data, we speculate that redistribution within the sedimentary sequence caused by the mobility and volatility of the element under relatively high temperatures may have contributed to Hg enrichment in distinct stratigraphic levels of the mature cores. Regardless of the exact mechanism, elevated Hg content together with organic-carbon loss by thermal maturation exaggerate the value of Hg/TOC in mature sediments, suggesting that thermal effects have to be considered when using TOC-normalised Hg as a proxy for far-field volcanic activity.