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Applicability of 26Al and 10Be for depositional age dating in deep-sea records

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Abstract

Reliable depositional age dating is essential for studying million-year-old geologic records. Where methods such as biostratigraphy, magnetostratigraphy, or radiometric dating are insufficient or inapplicable, the atmospheric long-lived cosmogenic radionuclide 10Be (t1/2 = 1.4 million years) has become an important additional dating tool. The cosmogenic radionuclide 26Al (t1/2 = 0.7 million years), which is also produced in the atmosphere, has not been thoroughly investigated as a dating tool. In this study, we measured the concentrations of 10Be and 26Al, along with their stable counterparts 9Be and 27Al, in four deep-sea sediment cores from the Indian Ocean, one Central Pacific ferromanganese crust, and six ferromanganese nodules from the Atlantic Ocean. Our results show that 26Al-based dating is, in principle, similarly applicable to 10Be-based dating but has one major drawback: nucleogenic in-situ 26Al production leads to increasingly unreliable ages in sediments older than approximately 3 million years, with interferences occurring even earlier in ferromanganese deposits. Furthermore, in deep-sea sediments only the 26Al/27Al and 10Be/9Be ratios yield reliable ages, whereas 26Al and 10Be concentrations or the 26Al/10Be ratio are affected by signal dilution due to pelagic carbonates. Thus, we conclude that the primary advantage of measuring 26Al is to corroborate and improve 10Be/9Be ratio-derived ages using 26Al/27Al ratios, but only for deep-sea sediments younger than approximately 3 million years.
Original languageEnglish
Article number120233
Number of pages13
JournalEarth and Planetary Science Letters
Volume692
DOIs
Publication statusPublished - 15 Oct 2026

Funding

This work was supported by the Austrian Science Fund (FWF) , Project P20434 and I428 (EUROCORES project EuroGENESIS, subproject CoDustMas, funded via the European Science Foundation; the University of Vienna (Abschlussstipendium 2014) and by the Australian Research Council’s Discovery scheme, project numbers DP180100495 and DP180100496 . Partially funded by the European Union (ERC, NoSHADE, 101077668). Views and opinions expressed are however those of the author(s) only and do not necessarily reflect those of the European Union or the European Research Council. Neither the European Union nor the granting authority can be held responsible for them. DK was supported by an AINSE Ltd. Postgraduate Research Award (PGRA). This research used sediment samples and data provided by the Antarctic Marine Geology Research Facility (AMGRF) at Florida State University. The AMGRF is sponsored by the U.S. National Science Foundation. Open Access funding enabled and organized by Project DEAL. We thank Wolfgang Schöner for sampling the ferromanganese crust VA13/2–237KD in 1976, and Thomas Kuhn and Andreas Lückge (Federal Institute for Geosciences and Natural Resources, Germany) for providing the crust sample. The nodules were provided by the Senckenberg Society for Nature Research (SNG). Parts of this research were carried out at the Ion Beam Centre (IBC) at the Helmholtz-Zentrum Dresden-Rossendorf e.V., a member of the Helmholtz Association. We would like to thank the DREAMS accelerator staff, Stefan Pavetich and René Ziegenrücker at HZDR for their support. Parts of the nodule sample preparation was performed with the help of Lisa Michel and Rebecca Schmidt (TU Dresden). Furthermore, we thank Aline Ritter, Sabrina Beutner (HZDR) and Valéry Guillou (CEREGE) for stable isotope measurements. We acknowledge Didier Bourlès and Régis Braucher (CEREGE), Beate Patzer (Technical University Berlin), Keith Fifield (ANU) and Patrick De Deckker for helpful discussions. In memoriam to Didier Bourlès: The cosmogenic rock star will be remembered.

FundersFunder number
Fonds zur Förderung der wissenschaftlichen Forschung (FWF)10.55776/I428, 10.55776/P20434

Austrian Fields of Science 2012

  • 103014 Nuclear physics
  • 105105 Geochemistry

Keywords

  • Be
  • Al
  • AMS
  • Depositional dating
  • Ferromanganese crust and nodules
  • Sediments

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