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4 F. NIGRO

 STRUCTURAL SETTING OF THE SICILY                              ary basinal carbonatic sequences (Sicanian domain-derived
                    THRUSTBELT                                 structural units).;

     The main tectoniƩ domains characterising the Centrai           8 - the deepest element of the Eastern Sicilian Belt,
Mediterranean, that may be recognised on land and under        formed by prevalently Oligocene to Miocene clastic se-
the sea around Sicily (Fig. 2), are (from the south):          quences, Messinian evaporites and Pliocene to Pleistocene
                                                               basinal sequences ("Gela Thrust System"; Catalano et al.,
     - an undeformed, or weakly deformed foreland extend-      1993b.).
ing from north-eastern Tunisia to south-eastern Sicily and
partly inflected below;                                             9 - the gently deformed Hyblean foreland.
                                                                    From the top, the geometry ofthe Western Sicily Belt is
     - the strongly deformed Sicily Belt, trending E-W from    due to the superposition of:
the Egadi Islands to the Malta Escarpment, and northwards           l - severa! tectonic units derived of deformation of the
as far as the Southern Sardinia Channel;                       "pre-Panormide" domain;
                                                                    2 - a set of tectonic units prevalently consisting of Tri-
     - the Kabilias and the Calabrian-Peloritani Are forming   assic to Neogene carbonates, derived from deformation of
the submerged Drepano Smt. (Compagnoni et al., 1986) and       the Panormide domain;
the Elimi Chain (Beccaluva et al., 1984), interpreted as an         3 - severa! tectonic units made up of Triassic to Neo-
intennediate element in the African Maghrebide-Sicily-         gene basinal sequences, derived from deformation of the
Apenninic Belt;                                                Imerese domain;
                                                                    4 - another set of tectonic units of Triassic to Neogene
     -the European-Sardinia Domain (Auzende et al., 1974;      prevalently carbonatic sequences derived from deformation
Barberi et al., 1984) thrust over the submerged Kabilo-        of the Trapanese domain;
Calabrian domain.                                                   5- severa! tectonic units composed ofMesozoic to Ter-
                                                               tiary basinal carbonatic sequences, derived from deforma-
Fig. 2. Schematic tectonic map ofthe Centrai Mediterranean     tion ofthe Sicanian domain;
                                                                    6 - the Meso-Cainozoic defonned foreland (Saccense
     Two tectonic piles, derived from the deformation of dif-  domain-derived tectonic units);
ferent African palaeogeographic domains, characterise the           7 - the Gela Thrust System.
western and the eastern sectors of the Sicilian Belt (for re-       Fig. 3 shows two simplified deep structural sections
cent lithologic columns, with indicated periods oftectonism    across the western and eastern Sicily. The structural style re-
see Catalano et al., 1993b).                                   cently recognised in the island is comparable to the thin-
                                                               skinned deformational mode!; the overall folds and thrust
     The Eastern Sicily Belt consists of several thrust sys-   belt show ramp and flat geometries, different duplex levels,
tems made up (from the top) of:                                some regional-propagated detachment surfaces, and a
                                                               marked disharmonic folding. A multiduplex configuration
     l - a set of prevalently Hercynian crystalline tectonic   has also been recognised in different sectors of the Sicilian
units ofthe Peloritani sector ofthe Calabrian Are;             chain (Lentini et al., 1990; Catalano et al., 1993b), as well
                                                               as in the surrounding submerged areas (Catalano et al.,
     2 - severa! tectonic units of Cretaceous to Paleogene     1993c).
flysch-like sequences (Flysch di Monte Soro);                       In the deep structural sections (Fig. 3), the main pa-
                                                               laegeographic domains-derived tectonic units are repre-
     3 - severa! tectonic units of very strongly deformed      sented, together with the main "out-of-sequence" low angle
Cretaceous claystones and "Sicilidi Variegated Shales";        reverse faults (<1>), that may be the result of back-stop-iike
                                                               processes, probably active since the Langhian (age of se-
     4- severa! tectonic units of Oligocene to Miocene fore-   quences overlying the back-thrusted "Antisicilidi units").
land siliciclastic turbidites (Flysch Numidico);               Out-of-sequence faulting repeated the previous deformed
                                                               tectonic complex and might have produced the subsequent
     5- some prevalently Triassic to Neogene carbonate tec-    superposition of the more external units (e.g. Panormide
tonic units (Panormide domain-derived structural units);       units) over the most internai ones (Fig. 3B), as well as the
                                                               Trapanese units over the Sicanian units.
     6- severa! tectonic units consisting ofTriassic to Neo-
gene basinal sequences (Imerese domain-derived structural         OLIGO-MIOCENE KINEMATICS AND
units);                                                        THE BACK-STOP MODEL SUPPORT FOR

     7 - severa! tectonic units formed by Mesozoic to Terti-                    THE SICILY BELT

                                                                    The kinematic history of the Sicilian Maghrebides is
                                                               comparable to the thrust envelopment mode! in the litera-
                                                               ture. During the Miocene, the collisional processes induced
                                                               the deformation of the African domains, expressed by the
                                                               activation of some thrust families linking in different de-
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