EGU25-13146, updated on 15 Mar 2025
https://doi.org/10.5194/egusphere-egu25-13146
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 28 Apr, 16:15–18:00 (CEST), Display time Monday, 28 Apr, 14:00–18:00
 
Hall X2, X2.10
Syn-rift magmatism and spreading initiation controlled by rift obliquity: insights from 3D thermo-mechanical modelling and observations
Éva Oravecz1,2, Attila Balázs2, Taras Gerya2, and László Fodor1,3
Éva Oravecz et al.
  • 1Eötvös Loránd Univeristy of Sciences, Department of Geology, Budapest, Hungary (orav.eva@gmail.com)
  • 2ETH Zürich, Department of Earth and Planetary Sciences, Zürich, Switzerland
  • 3HUN-REN Institute of Earth Physics and Space Science, Sopron, Hungary

Continental rifting is often oblique, influenced by the strain localization effects of the various structural, compositional and thermal heterogeneity zones pre-existing in the lithosphere. Oblique rifting generates strain partitioning and leads to the along-strike segmentation of the rift structure, including the development of strike-slip transfer zones and en echelon fault geometries. While previous modelling studies have explored the relation between the rift obliquity and crustal fault patterns, its effects on the syn-rift magmatism and the oceanic spreading initiation have remained underexplored.

In this study, we conducted a series of high resolution 3D numerical models using the I3ELVIS-FDSPM numerical code to compare the continental rift evolution and spreading initiation in orthogonal and oblique rift settings. The code handles visco-plastic rheologies, staggered finite differences and marker-in-cell techniques to solve the mass, momentum and energy conservation equations for incompressible media. Oblique rifting is linked to strain localization along a pre-defined hydrated weak zone in the mantle lithosphere that simulates an inherited suture zone, while the applied two-way coupling between the thermo-mechanical and surface processes models allows for the quantification of the dynamic feedbacks between rift obliquity, crustal strain patterns, magmatism, and the erosion-sedimentation processes.

The models show that oblique rifting delays the onset of melting and continental break-up. Due to the feedbacks between crustal deformation, thermal evolution and melting, increasing rift obliquity leads to the non-linear reduction of the crustal melt supply, while at higher rift obliquity (α>30°), the en echelon arrangement of the elongated magma chambers in the crust suggests a strong structural control over the spatial distribution of crustal melts. When the rift evolution enters the spreading stage, first continental break-up occurs along the offset sub-orthogonal rift segments, and the individual embryonic oceanic segments are subsequently merged by the two-directional along-strike propagation of the incipient spreading ridges. The rate of this propagation changes in space and time, driven by the variable efficiency of strain localization. Above 30° obliquity, deformation along the offset spreading ridges is accommodated by oceanic transform faults that develop spontaneously, without a precursory lithospheric inhomogeneity in their place during the latest stage of spreading initiation. These inferences are in line with observations from the Woodlark Basin and Main Ethiopian Rift.

How to cite: Oravecz, É., Balázs, A., Gerya, T., and Fodor, L.: Syn-rift magmatism and spreading initiation controlled by rift obliquity: insights from 3D thermo-mechanical modelling and observations, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-13146, https://doi.org/10.5194/egusphere-egu25-13146, 2025.