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Impact of iron corrosion on the mineralogical evolution of Callovo-Oxfordian claystone: in situ MCO experiment
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  • Published: 02 April 2026

Impact of iron corrosion on the mineralogical evolution of Callovo-Oxfordian claystone: in situ MCO experiment

  • Isabella Pignatelli1,
  • Enrico Mugnaioli2,
  • Mustapha Abdelmoula3,
  • Delphine Neff4,
  • John Moine5,
  • Nicolas Michau6 &
  • …
  • Yannick Linard6 

npj Materials Degradation , Article number:  (2026) Cite this article

We are providing an unedited version of this manuscript to give early access to its findings. Before final publication, the manuscript will undergo further editing. Please note there may be errors present which affect the content, and all legal disclaimers apply.

Subjects

  • Chemistry
  • Engineering
  • Environmental sciences
  • Materials science
  • Solid Earth sciences

Abstract

The MCO experiment was carried out over a period of 12 years in the Underground Research Laboratory (URL) of Andra to investigate long-term effects of iron-claystone interactions. The test chamber consisted of two cylinders: the external cylinder (EC) was made up of Callovo-Oxfordian claystone (COx); the internal cylinder (IC) was a mixture of crushed COx and iron grains. A central heater system and water seepage simulated the heat released by the radioactive decay and the circulation of clay porewater respectively. A multi-technique characterization indicates that the EC showed very little changes in comparison with the pristine claystone. The clay particles of IC become enriched in Fe3+ and evolve towards a composition close to odinite/berthierine. Several corrosion products are identified but no magnetite is observed, although this mineral is thought to be at the origin of the passivation effect playing a role in the corrosion rate and porosity clogging. The released iron remains in the IC and migrates up to the interface between the two cylinders. This underlines that the effect of iron corrosion on the surrounding host-rock is restrained to a small portion of COx, whereas the rest of the rock preserve its properties suitable for a HLW repository.

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Data availability

The data related to the findings of this study are available within the paper on in Supplementary material, and any other supporting data could be provided by the corresponding author on reasonable request.

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Acknowledgements

This research was financially supported by the Agence Nationale pour la Gestion des Déchets Radioactifs (ANDRA). We thank the Center of Instrument Sharing for the University of Pisa (CISUP) for support with FIB sectioning and TEM imaging, and Dr. Marc Ulrich for his help in collection and treatment of μ-XRF data. This is CRPG contribution #2894.

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Authors and Affiliations

  1. CRPG UMR 7358 CNRS-UL, Université de Lorraine, Vandœuvre-lès-Nancy cedex, France

    Isabella Pignatelli

  2. Dipartimento di Scienze della Terra, Università di Pisa, Pisa, Italy

    Enrico Mugnaioli

  3. LCPME UMR 7564 CNRS-UL, Université de Lorraine, Nancy, France

    Mustapha Abdelmoula

  4. LAPA-NIMBE/IRAMAT, CEA, CNRS, Université Paris-Saclay, Gif-sur-Yvette, France

    Delphine Neff

  5. LSE UMR 1120, INRAE, Université de Lorraine, Vandœuvre-lès-Nancy cedex, France

    John Moine

  6. Agence Nationale pour la Gestion des Déchets Radioactifs (ANDRA), Research & Development Division, 1/7 rue Jean Monnet, Châtenay-Malabry, France

    Nicolas Michau & Yannick Linard

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  1. Isabella Pignatelli
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Contributions

The study was conceived by N.M., Y.L., and I.P. The materials were previously produced by Y.L. and N.M. I.P., E.M., M.A., D.N., and J.M. performed sample preparation, data acquisition and analysis. I.P. wrote the paper first draft, revised by all. All authors approved the final version.

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Correspondence to Isabella Pignatelli.

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Pignatelli, I., Mugnaioli, E., Abdelmoula, M. et al. Impact of iron corrosion on the mineralogical evolution of Callovo-Oxfordian claystone: in situ MCO experiment. npj Mater Degrad (2026). https://doi.org/10.1038/s41529-026-00776-x

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  • Received: 07 December 2025

  • Accepted: 14 March 2026

  • Published: 02 April 2026

  • DOI: https://doi.org/10.1038/s41529-026-00776-x

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