Cenozoic Fault Growth Mechanisms in the Outer Apulian Platform

Author:

Agosta Fabrizio12ORCID,Petrullo Angela Vita23,La Bruna Vincenzo4,Prosser Giacomo1ORCID

Affiliation:

1. Department of Sciences, University of Basilicata, Via dell’Ateten Lucano 10, 85100 Potenza, Italy

2. Geosmart Italia S.r.l.s., Via Di Giura 54, 85100 Potenza, Italy

3. Agenzia per la Protezione Ambientale della Basilicata, 75100 Matera, Italy

4. Department of Geophysics, Federal University of Rio Grande do Norte, Natal 1524, RN, Brazil

Abstract

This work focuses on a ca. 55 km-long extensional fault zone buried underneath the foredeep deposits of the southern Apennines, Italy, with the goal of deciphering the Cenozoic fault growth mechanisms in the Outer Apulian Platform. By considering public 2D seismic reflection profiles, well logs, and isochron maps data, the study normal fault zone is interpreted as made up of four individual fault segments crosscutting Top Cretaceous, Top Eocene, Top Miocene, and Top Pliocene chrono-stratigraphic surfaces. The computed cumulative throw profiles form either bell-shaped or flat-shaped geometries along portions of the single fault segments. The computed incremental throw profiles also show an initial fault segmentation not corresponding with the present-day structural configuration. Data are consistent with the initial, post-Cretaceous fault segments coalescing together during Miocene–Pliocene deformation and with fault linkage processes localizing at the stepover/relay zones. Pleistocene faulting determined the evolution of a coherent fault system. The computed n-values obtained for the single time intervals by considering the maximum fault throw–fault length relations indicate that the fault segments formed scale-dependent geometries. Variations of these computed values are interpreted as due to the higher degree of maturity reached by the entire fault system during Miocene to Pleistocene deformation.

Funder

Basilicata and Camerino universities, Italy

Publisher

MDPI AG

Subject

General Earth and Planetary Sciences

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