This is an author version of the contribution published on:Questa è la versione dell'autore dell'opera: Festa et al. (2013)
Abstract 35We document in this study the internal structure of the Late Cretaceous-late Oligocene 36Ligurian accretionary wedge in northwestern Italy, and the occurrence in this exhumed wedge 37 of broken formation and three different types of mélanges that formed sequentially through 38 time. The Broken Formation is the oldest unit in the accretionary wedge and shows bedding-39 parallel boudinage structures, which developed as a result of layer-parallel extension at the 40 toe of the internal part of the Alpine wedge front during the Late Cretaceous-middle Eocene.
Introduction 62 63The shape and growth of the frontal wedge of the modern accretionary complexes repeatedly 64 change to maintain the dynamic equilibrium in the wedge through alternating tectonic and 65 sedimentary (i.e., gravitational) activities (e.g., Davis et al., 1983; Scholl et al., 1977; von 66 Huene and Lallemand, 1990; Gutscher et al., 1998; Cliff and Vannucchi, 2004; Wang and Hu, 67 2006;Buiter, 2012; Gravelau et al., 2012; Haq, 2012). Highly sheared, disrupted and 68 fragmented rock units and tectonic mélanges are the products of tectonics occurring along the 69 basal décollements in accretionary wedges and out-of-sequence thrust-faults, and within the 70 subduction channels (e.g., Karig and Sharman, 1975;Cloos, 1982; Moore and Byrne, 1987; 71 Taira et al., 1992; Dileonardo et al., 2002;Collot et al., 2011). Mass-transport deposits and 72 sedimentary mélanges result from slope instability in the trench-inner slope and in the upper 73 parts of frontal wedges (e.g., Lallemand et al., 1990; Duperret et al., 1995; Goldfinger et al., 74 2000;von Huene et al., 2000;Collot et al., 2001; McAdoo et al., 2004;Sage et al., 2006; 75 Mosher et al., 2008; Ogawa et al., 2011; Strasser et al., 2009Strasser et al., , 2011. Shale and mud 76 diapirism represent the upward rise of overpressured fluids migrating along the basal 77 décollement or channeled along megasplay faults (e.g., Brown and Westebrook, 1988; Moore 78 and Vrolijk, 1992; Kopf, 2002;Chamot-Rooke et al., 2006;Camerlenghi and Pini, 2009). showing a complex internal block-in-matrix fabric that may vary both laterally and vertically 82 (e.g., Maxwell, 1974;Cloos, 1984;Raymond, 1984;Cowan, 1985;Byrne and Fisher, 1990; 83 Barnes and Korsch, 1991; Onishi and Kimura, 1995; Ogawa, 1998; Dilek et al., 1999 Dilek et al., , 2005 84 Pini, 1999; Dilek and Robinson, 2003;Codegone et al., 2012aCodegone et al., , 2012b Dilek et al., 2012; 85 5 Festa et al., 2010a;Ukar, 2012;Wakabayashi, 2012;Singlengton and Cloos, 2013). The 86 primary internal structures of mélanges and mélange-forming processes are commonly 87 obscured by subsequent deformational events, resulting in superposed and mixed mélanges 88 types, such tectonic, sedimentary and diapirc mélanges. Much effort has been made to 89 establish a set of useful criteria by which to distinguish mélange t...