Articles | Volume 16, issue 9
https://doi.org/10.5194/se-16-841-2025
https://doi.org/10.5194/se-16-841-2025
Research article
 | 
10 Sep 2025
Research article |  | 10 Sep 2025

The influence of accretionary orogenesis on subsequent rift dynamics

Zoltán Erdős, Susanne J. H. Buiter, and Joya L. Tetreault

Data sets

The influence of accretionary orogenesis on subsequent rift dynamics - Animations and data assembly Zoltán Erdős et al. https://doi.org/10.5281/zenodo.14980545

Model code and software

The influence of accretionary orogenesis on subsequent rift dynamics - Animations and data assembly Zoltán Erdős et al. https://doi.org/10.5281/zenodo.14980545

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Short summary
We used computer models to study how mountains formed by the collision of tectonic plates can later affect the breakup of these same plates. Our results show that in large, warm mountain belts, new faults form due to the orogen being  weak overall, while in smaller, colder belts, breakup follows old fault zones. Microcontinents that were accreted during collision can create new continental fragments during extension. These findings help explain how past geological events shape continent margins.
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