EGU26-835, updated on 13 Mar 2026
https://doi.org/10.5194/egusphere-egu26-835
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Friday, 08 May, 08:30–10:15 (CEST), Display time Friday, 08 May, 08:30–12:30
 
Hall X5, X5.185
Planktonic foraminifera luminescence as a new paleoclimate proxy for oceanic and atmospheric conditions off South America
Tatiana de Lourdes Campese1, Marília de Carvalho Campos1, Carlos Ortiz2, Bruna Borba Dias3, Cristiano Mazur Chiessi3, Breno de Souza Marques1, Laura Kraft1, Viviane Querollaine Pires Turman1, Gelvam Hartmann1, Svetlana Radionovskaya4, Luke Skinner4, Aline Govin5, Vinícius Ribau Mendes6, Thays Desirée Mineli7, André Bahr8, Stefan Mulitza9, and André Oliveira Sawakuchi7
Tatiana de Lourdes Campese et al.
  • 1Institute of Geosciences, University of Campinas, Brazil
  • 2Department of Physics, Technical University of Denmark, Risø Campus, 4000 Roskilde, Denmark
  • 3School of Arts, Sciences and Humanities, University of São Paulo, Brazil
  • 4Department of Earth Sciences, University of Cambridge, Cambridge, United Kingdom
  • 5Laboratoire des Sciences du Climat et de l'Environnement (LSCE, CEA-CNRS-UVSQ), Paris-Saclay University, Gif sur Yvette, France
  • 6Institute of Marine Science, Federal University of São Paulo, Santos, Brazil
  • 7Institute of Geosciences, University of São Paulo, Brazil
  • 8Institute of Earth Sciences, Heidelberg University, Germany
  • 9Center for Marine Environmental Sciences, University of Bremen, Bremen, Germany

Luminescence emitted by minerals has long been used in paleoenvironmental studies, particularly thermoluminescence (TL) from carbonates. TL emission in calcite is controlled by the type and quantity of defects in the crystal lattice, which may act as charge traps and/or recombination centers. These defects can be influenced by environmental conditions prevailing at the time of crystallization, for example through the incorporation of impurities substituting calcium in the calcite lattice (e.g., Mg, Mn, Fe). In this context, this study investigates the potential of TL signals emitted from the calcite of the planktonic foraminifera Globigerinoides ruber (white sensu stricto, 250–350 μm) as a paleoclimate proxies. This species was selected due to its widespread use in paleoclimate reconstructions, high abundance, and known sensitivity to environmental variability. We analyzed samples from three marine sediment cores from the western Atlantic, encompassing different spatial and temporal contexts. Two cores represent modern conditions under contrasting oceanographic settings: MD23-3669MC (equatorial Atlantic) and GeoB6211-1 (subtropical South Atlantic). The third core, CDH-89 (equatorial Atlantic), spans the penultimate glacial–interglacial transition (143–122 ka), allowing the comparison between modern and paleoclimatic signal.

The resulting TL intensity curves (light emitted per unit mass and unit radiation dose) exhibit peaks at approximately 65°C and 400°C. These TL signals were compared with classical paleoceanographic proxies, i.e., Mg/Ca, Mn/Ca, Fe/Ca and stable isotope data, measured on shells of the same planktonic foraminifera species. Principal component analysis indicates that the 400°C peak is primarily controlled by sea surface temperature variations, whereas the 65°C peak is associated with proxies related to continental input to the ocean. These results demonstrate that TL signals in planktonic foraminifera preserve environmental signatures, supporting their potential as new paleoclimate proxies. Further systematic testing across environments and experimental conditions is required to fully validate and advance these proxies for broader paleoenvironmental applications.

How to cite: Campese, T. D. L., Campos, M. D. C., Ortiz, C., Dias, B. B., Chiessi, C. M., Marques, B. D. S., Kraft, L., Turman, V. Q. P., Hartmann, G., Radionovskaya, S., Skinner, L., Govin, A., Mendes, V. R., Mineli, T. D., Bahr, A., Mulitza, S., and Sawakuchi, A. O.: Planktonic foraminifera luminescence as a new paleoclimate proxy for oceanic and atmospheric conditions off South America, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-835, https://doi.org/10.5194/egusphere-egu26-835, 2026.