EGU22-8021, updated on 28 Mar 2022
https://doi.org/10.5194/egusphere-egu22-8021
EGU General Assembly 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

Impacts of the Toba super-eruption on the pH of the Andaman Sea

Ana Alves1, Matthieu Buisson2, Pascale Louvat3, Claire Rollion-Bard4, Franck Bassinot4, Eva Moreno5, Guillaume Paris6, Benoit Caron7, Giulia Del Manzo2, Anne Le Friant2, and Annachiara Bartolini1
Ana Alves et al.
  • 1Centre de recherche en paléontologie - Paris UMR7207, CNRS, MNHN, Sorbonne Université, France
  • 2Université de Paris, Institut de physique du globe de Paris, CNRS, UMR 7154, Paris, France
  • 3IPREM Pau UMR 5254 CNRS Université de Pau et des Pays de l’Adour, France
  • 4LSCE UMR 8212 CEA CNRS IPSL UVSQ Université Paris-Saclay, France
  • 5LOCEAN Sorbonne Université CNRS IPSL IRD MNHN, France
  • 6CRPG Nancy UMR 7358 Université de Lorraine, France
  • 7ISTEP UMR 7193 CNRS Sorbonne Université, France

The Toba volcano super-eruption on the island of Sumatra occurred about 74,000 years ago[1], close to the transition between interglacial Marine Isotope Stage (MIS) 5 and glacial MIS 4. This eruption, called Youngest Toba Tuff (YTT), is currently described as the largest cataclysmic eruption of the Quaternary. However, the impact of this super-eruption on climate is widely debated and its effects on the ocean remains poorly understood.

The aim of this work is to estimate its impact on oceanic pH at a site near the eruption center. To do so, we measured δ11B values (pH proxy) on monospecific samples of planktonic foraminifera Globigerinoides ruber and Pulleniatina obliquiloculata from sediment core BAR94-25 (Andaman Sea) using a recently developed method at the Institut de Physique du Globe de Paris (IPGP)[2]. G. ruber is a species that thrives preferentially in surface waters, while P. obliquiloculata lives at the thermocline. Therefore, δ11B measurements on their shells can reconstruct pH variations in surface and thermocline waters, respectively.

We selected the interval from 258 to 355 cm, corresponding to an age between 57 and 82 ka. This interval contains two clearly visible tephra layers corresponding to the YTT, at the transition from MIS 5 to MIS 4, and to a post-YTT explosive activity during MIS 4. These layers are correlated with a significant decrease in carbonate content (CaCO3). Our results indicate a complex pH response during the two concerned volcanic episodes. Thermocline seawater doesn’t show significant pH decrease during the volcanic episodes compared to the overall signal recorded throughout the studied interval. Conversely, surface seawater shows a much more important pH decrease during part of the volcanic episodes than during the all studied interval. Such decrease in pH during the transition to a glacial state is particularly surprising because an increase in pH, due to the global reduction in atmospheric CO2, is rather expected, as shown by previous foraminifera δ11B records[3].

The coupling of CaCO3 and pH decrease during tephra levels suggests acidification in the Andaman Sea as a consequence of the Toba volcanic eruptive activity. The seawater surface seems much more sensitive to pH changes than the thermocline zone. However, the reduction of carbonate in the two tephra layers may also be due to dilution from ash falling into the sediment. Other analyses, such as measuring the variation of calcification intensity in planktonic foraminifera, are therefore necessary to better interpret these paleo-pH data.

[1] Storey et al., 2012, PNAS, 109 (46), 18684-18688

[2] Buisson et al., 2021, JAAS, 36, 2116-2131

[3] Foster et al., 2008, EPSL, 271, 254-266

How to cite: Alves, A., Buisson, M., Louvat, P., Rollion-Bard, C., Bassinot, F., Moreno, E., Paris, G., Caron, B., Del Manzo, G., Le Friant, A., and Bartolini, A.: Impacts of the Toba super-eruption on the pH of the Andaman Sea, EGU General Assembly 2022, Vienna, Austria, 23–27 May 2022, EGU22-8021, https://doi.org/10.5194/egusphere-egu22-8021, 2022.