TSK 11 Göttingen 2006 Structural contacts in the Late Paleozoic accretionary wedge of central Chile and their tectonic significance for the evolution of the accre- tionary complex Vortrag Peter P. Richter1 Uwe Ring2 Arne P. Willner3 Bernd Leiss4 The Chilean accretionary wedge is part of a Late Paleozoic subduction complex that developed during subduction of the Pacific plate underneath South Amer- ica. The wedge is commonly subdivided into a structurally lower Western Series and an upper Eastern Series. Under- standing the contact between both se- ries has been a long standing problem and is fundamental for the understand- ing of the evolution of the wedge sys- tem. We show the progressive develop- ment of structures and finite strain from the least-deformed rocks in the eastern part of the Eastern Series of the accre- tionary wedge to higher grade schist of the Western Series at the Pacific coast. Upright chevron folds of sedimentary layering are associated with a penetra- tive axial-plane foliation, S1. As the F1 folds became slightly overturned to the west, S1 was folded about recum- bent open F2 folds and an S2 axial-plane foliation developed. Near the contact between the Western and Eastern se- ries S2 represents a prominent subhor- izontal transposition foliation. Towards the structural deepest units in the west 1 Institut für Geowissenschaften, Johannes Gutenberg-Universität, 55099 Mainz, Germany 2 Department of Geological Sciences, Canter- bury University, Christchurch, New Zealand 3 Institut für Geologie, Mineralogie und Geo- physik, Ruhr-Universität, 44870 Bochum, Germany 4 Zentrum für Geowissenschaften, Universität Göttingen, Göttingen, Germany the transposition foliation became pro- gressively flattened. Finite-strain data as obtained by Rf/φ analysis in meta- greywacke and X-ray texture goniome- try in phyllosilicate-rich rocks show a smooth and gradual increase in strain magnitude from east to west. There is no evidence for normal faulting or signif- icant structural breaks across the con- tact. We interpret the progressive struc- tural and strain evolution between both series to reflect a continuous change in the mode of accretion in the subduction wedge. Before ca. 320-290Ma the rocks of the Eastern Series were frontally ac- creted to the Andean margin. Frontal accretion caused horizontal shortening and upright folds and axial-plane foli- ations developed. At ca. 320–290Ma the mode of accretion changed and the rocks of the Western Series were under- plated below the Andean margin. This basal accretion caused a major change in the flow field within the wedge and gave rise to vertical shortening and the development of the penetrative subhor- izontal transposition foliation. 1