EGU26-7786, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-7786
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Thursday, 07 May, 08:45–08:55 (CEST)
 
Room G2
Direct marine geophysical constraints on the rupture of the 2012 Mw 8.6 Wharton basin earthquake
Saksham Rohilla1, Hélène Carton1, Satish Singh1, Muriel Laurencin2, Nugroho Hananto3, Mihai Roharik1, Yanfang Qin4, Sudipta Sarkar5, Mark Noble6, Mari Hamahashi7, and Paul Tapponnier
Saksham Rohilla et al.
  • 1Institut de physique du globe de Paris, Université Paris Cité, Paris, France (rohilla@ipgp.fr)
  • 2GEOxyz, Harelbbeekstraat 104 D 8550 Zwevegem, Belgium
  • 3Research Center for Deep Sea, Indonesian Institute of Sciences, Jakarta, Indonesia
  • 4Japan Agency for Marine‐Earth Science and Technology, Yokohama Institute for Earth Science, Yokohama, Japan.
  • 5Department of Earth and Climate Science, Indian Institute of Science Education and Research, Pune, India
  • 6Centre de Géosciences, MINES ParisTech, PSL University, Fontainebleau, France
  • 7Faculty of Global and Science Studies, Yamaguchi University, 1677-1 Yoshida, Yamaguchi 753-8541, Japan.

Current understanding of earthquake rupture and earthquake cycles is largely derived from continental fault systems, implicitly assuming their applicability to oceanic lithosphere. Futhermore, the limited geological and geophysical constraints on large oceanic earthquakes hinder robust assessment of how deformation, fault growth, and stress accumulation takes place in the oceanic lithosphere. The 2012 Mw 8.6 Wharton Basin earthquake, the largest instrumentally recorded strike-slip event, challenged prevailing views of intraplate deformation in the Indian Ocean by rupturing a complex network of faults at high angles to one another. Seismological and geodetic analyses revealed a deep centroid depth, high stress drop, and multi-fault rupture, yet the offshore setting severely limited constraints on fault geometry and rupture propagation. Here, we bridge short- and long-term deformation processes by integrating high-resolution bathymetry, multichannel seismic reflection, and sub-bottom profiler data. We present the surface and near-surface deformation along one of the faults ruptured during the Mw 8.6 earthquake, which runs ESE-WNW and initiates near the epicenter of the Mw 8.2 aftershock. The ~100-km-long fault displays well-preserved dextral offsets accumulated since ~4 - 5 Ma and an en-echelon segmented pattern forming a positive flower structure rooted in the oceanic mantle. We estimate slip rates of ~0.4 to 0.8 mm/yr suggest long recurrence intervals for large intraplate earthquakes. Coulomb stress modelling indicates substantial coseismic stress loading on the N-S fault that subsequently ruptured during the Mw 8.2 earthquake, thus establishing a mechanical relationship between the two events. Overall, our study shows that the oceanic lithosphere can deform slowly and extensively over long time scales, accumulating strain along slow-slipping faults that can produce very large, cascade-style earthquakes. Furthermore, our study offers key inputs for earthquake cycle and dynamic rupture models in oceanic settings by providing geological constraints on fault geometry and slip rates.

How to cite: Rohilla, S., Carton, H., Singh, S., Laurencin, M., Hananto, N., Roharik, M., Qin, Y., Sarkar, S., Noble, M., Hamahashi, M., and Tapponnier, P.: Direct marine geophysical constraints on the rupture of the 2012 Mw 8.6 Wharton basin earthquake, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7786, https://doi.org/10.5194/egusphere-egu26-7786, 2026.