EGU24-6306, updated on 08 Mar 2024
https://doi.org/10.5194/egusphere-egu24-6306
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Coupling Timing and Tempo of Deccan Volcanism with the KPg Extinction: Evidence from Mercury and Tellurium Anomalies

Thierry Adatte1, Marcel Regelous2, Nils Baumann2, Hassan Hassan Khozyem3, Jorge E. Spangenberg4, Gerta Keller5, Uygar Karabeyoglu1, Blair Schoene5, and Syed Khadri6
Thierry Adatte et al.
  • 1Lausanne, Institute of Earth Sciences, ISTE, Lausanne, Switzerland (thierry.adatte@unil.ch)
  • 2Friedrich-Alexander-Universität Erlangen-Nürnberg, GeoZentrum Nordbayern, Schlossgarten 5, 91054 Erlangen, Germany
  • 3Department of Geology, Aswan University, 81528, Aswan, Egypt
  • 4IDYST, Institute of Earth Surface Dynamics, University of Lausanne, Lausanne, Switzerland
  • 5Department of Geosciences, Princeton University, USA.
  • 6VR Siddharta Engineering College, Vijaywada, India

Mercury (Hg) and more recently tellurium (Te) are indicator of large-scale volcanism in marine sediments and provide valuable insights into relative timing between biological and environmental changes, mass extinctions and delayed recovery. Several studies evaluated the relationship between Hg anomalies in sediments and LIP activity across mass extinction horizons. The bulk (80%) of Deccan Trap eruptions occurred over a relatively short time interval in magnetic polarity C29r. U-Pb zircon geochronology reveals the onset of this main eruption phase 350 ky before the Cretaceous-Tertiary (KT) mass extinction. Maximum eruption rates occurred before and after the K-Pg extinction, with one such pulse initiating tens of thousands of years prior to both the bolide impact and extinction, suggesting a cause-and-effect relationship. We present a comprehensive high-resolution analysis of Deccan Traps Hg-Te loading, climate change and end-Cretaceous (KPB) mass extinction from a transect, which includes 30 sections deposited in both shallow and deep environments located in France, Spain, Italia, Denmark, Israel and Tunisia. In all sections, our findings indicate that Hg concentrations are more than 2 orders of magnitude greater during the final 100ky of the Maastrichtian up to the early Danian P1a zone (first 380 Ky of the Paleocene). Notably, Hg anomalies generally show no correlation with clay or total organic carbon contents, suggesting that the mercury enrichments resulted from higher input of atmospheric Hg species into the marine realm, rather than being driven by organic matter scavenging and/or increased run-off. Significant and coeval Hg enrichments are observed in multiples basins characterized by proximal and distal, as well as shallow and deep-water settings, supporting a direct fallout from volcanic aerosols. Hg enrichments are not observed in the Indian redboles, confirming that it is not a proximal proxy for volcanism. But significant Hg anomalies have been found in more distal intertrapeans sediments at Anjar (Gujarat), Daiwal and Podgavan (SW Nagpur, Maharashtra). Significant Hg anomalies are also found in the more distal Megalaya section. Hg isotope data from Bidart confirm a direct Hg fallout from volcanic aerosols. Furthermore, Te/Th ratios measured in the Goniuk (Turkey), Elles (Tunisia), Gubbio (Italy) and Wadi Nukhul (Egypt) sections show the same trend as Hg/TOC and are consistent with a volcanic origin, albeit a minor extraterrestrial contribution of Hg at the boundary cannot be excluded. Hg and Te maximum loadings coincide with time of maximum Deccan emission rates and volumes determined by zircon dating. Hg and Te concentrations within sediments in conjunction with Te/Th and Hg/TOC ratios are therefore robust and useful proxies to trace intensity of volcanism.

How to cite: Adatte, T., Regelous, M., Baumann, N., Hassan Khozyem, H., Spangenberg, J. E., Keller, G., Karabeyoglu, U., Schoene, B., and Khadri, S.: Coupling Timing and Tempo of Deccan Volcanism with the KPg Extinction: Evidence from Mercury and Tellurium Anomalies, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-6306, https://doi.org/10.5194/egusphere-egu24-6306, 2024.