26 Structural Geology and Tectonics (Posters)

Wednesday, 6 April 2016
8:30 AM - 12:30 PM
Ballroom C


A > 4 KM WIDE DUCTILE SHEAR ZONE IN THE CUESTA DE RANDOLFO: LATE-STAGE STRAIN LOCALIZATION IN THE FAMATINIAN OROGENY, ARGENTINA

Paper number: 26-11
Program: Technical Sessions
Time: 8:30 AM – 12:30 PM


Authors


Abstract

Orogen-scale NW-SE trending ductile shear zones affecting Ordovician Famatinian and older rocks have been identified in the central and northwestern region of Argentina. In the Cuesta de Randolfo area, southern Puna of Argentina, we documented in detail a > 4 km wide shear zone. Calc-alkaline, peraluminous, Famatinian arc related coarse-grained biotite ganodiorite, white mica- and tourmaline-rich granite and locally pelitic metasediments form the protoliths to the mylonitic shear zone. Weak to moderate magmatic fabrics are increasingly overprinted by NW-striking, moderate temperature subsolidus fabrics over a short distance what is mapped as the edge of the shear zone. Solid-state foliations form a fan-like structure and are in most parts more intensively developed than steeply plunging mineral lineations, which also show a spread in trends from ~ 85 to 220°. Preliminary thin section observations show that mica and quartz are intensively recrystallized, while feldspar deformation varies along the width of the shear zone from brittle cracking to minor subgrain formation. We thus infer temperatures of > 350 to <550 °C during ductile deformation. The presence of chlorite in veins and compositional banding further indicate fluid flow during retrograde metamorphic conditions. Kinematics in the field show in parts reverse motion, while in thin sections (e.g. porphyroclast-matrix relationship and shear bands), kinematics are variable with pure shear being dominant. Field and thin section work so far indicates that the shear fabrics define a positive flower structure or double-vergent ductile shear zone showing no significant strike-slip motion but recording localized contractional deformation during the closing of the Famatinian orogeny.

Geological Society of America Abstracts with Programs. Vol. 48, No. 4

doi: 10.1130/abs/2016CD-274460

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