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This version was published on November 1, 2009
GSA Bulletin; November 2009; v. 121; no. 11-12; p. 1475-1490; DOI: 10.1130/B26420.1
© 2009 Geological Society of America
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Structural evolution of the sedimentary accretionary wedge of the alpine system in Eastern Sicily: Thermal and thermochronological constraints

Sveva Corrado1,{dagger}, Luca Aldega1, Maria Laura Balestrieri2, Rosanna Maniscalco3 and Mario Grasso3

1 Dipartimento di Scienze Geologiche, Università "Roma Tre," Largo San Leonardo Murialdo 1, 00146 Roma, Italy
2 C.N.R., Istituto di Geoscienze e Georisorse, Sezione Firenze, Via La Pira 53, 50121 Firenze, Italy
3 Dipartimento di Scienze Geologiche, Università di Catania, Corso Italia 55, 95129 Catania, Italy

Correspondence: {dagger}E-mail: corrado{at}uniroma3.it

Temperature-dependent clay-mineral assemblages, vitrinite reflectance, and apatite fission-track data have been used to investigate levels of diagenesis and time of exhumation of the double-verging Sicilide-Antisicilide accretion-ary wedge in Eastern Sicily. The integration of organic and inorganic thermal indicators allowed us to distinguish parts of the accre-tionary wedge with different thermal signature and evolution. We recognize a warmer core made up of the Mount Soro and Troina units and two colder rims (Antisicilide and far-traveled Sicilide units). The Antisicilide unit was thrust back toward the hinterland, and the far-traveled Sicilide units were gravity-driven toward the Hyblean Plateau.

In detail, the highest percentages of vitrinite reflectance (VRo) values (0.60%–0.96%) and percentages of illite layers in illite-smectite (I-S; 60%–85%) are found in the Mount Soro and Troina units. Apatite fission-track data, together with the paleotemperature estimates from vitrinite-reflectance data and clay-mineral–based geothermometers, indicate that fission tracks were partially to totally annealed during wedge accretion and that the subsequent exhumation occurred mainly in Burdigalian times.

Low VRo values (0.35%–0.50%) and percentages of illite layers in I-S (30%–60%) occur in early thrust-top deposits (Reitano Flysch) that unconformably overlie the Sicilide Complex, as well as the far-traveled Sicilide and Antisicilide units. Apatite fission-track data for the Antisicilide unit confirm low paleo-temperature values. Thus the far-traveled Sicilide and Antisicilide units were probably at higher structural levels in the original accretionary prism and were remobilized since late Aquitanian–Burdigalian times.







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