- 1Dipartimento di Scienze Chimiche e Geologiche, Università di Modena e Reggio Emilia, Modena, Italy
- 2University of Naples Federico II, Department of Physics, Naples, Italy (grazia.delandro@unina.it)
- 3School of Science and Technology – Geology Division, University of Camerino, Camerino, Italy
- 4Istituto Nazionale di Geofisica e Vulcanologia, Rome, Italy
- 5DiSTAR, Università degli Studi di Napoli ‘Federico II’, Naples, Italy
- 6Lamont–Doherty Earth Observatory of Columbia University, Palisades, NY10964, USA
- 7Istituto Nazionale di Geofisicae Vulcanologia, L’Aquila, Italy
The Irpinia region is one of the most seismically active areas of Italy owing to continuing, late-orogenic extension in the axial zone of the Apennine mountain belt. However, the 3D architecture and the nature of the faults that drive this extension are still uncertain, posing challenges to seismic hazard assessment. Here, we address these uncertainties by integrating a new catalogue of high-resolution micro-seismicity (ML < 3.5), complemented by earthquake focal mechanisms, with existing 3D seismic velocity models and geological data. We found that micro-seismicity is primarily taking place along a segmented, approximately 60 km long, deep-seated, Mesozoic normal fault that was inverted during the shortening stages of the Apennine orogeny and then extensionally reactivated during the Quaternary. These findings suggest that multiple events of reactivation of long-lived faults can weaken their strength, making them prone to co-seismic remobilization under newly imposed strain fields in active mountain belts.
How to cite: Giovanni, C., De Landro, G., Mazzoli, S., Michele, M., Muzellec, T., Ascione, A., Schaff, D. P., Tarantino, S., and Zollo, A.: Active extension in the axial zone of the southern Apennines (Italy) is driven by the remobilization of inverted normal faults, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-18558, https://doi.org/10.5194/egusphere-egu25-18558, 2025.