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Hunter–Bowen deformation in South Percy Island, northeastern Australia

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posted on 2018-02-16, 04:57 authored by D. Hoy, G. Rosenbaum, N. Mortimer, U. Shaanan

South Percy Island is located approximately 50 km off the central Queensland coast and comprises a disrupted ophiolite mass alongside a diverse array of metamorphosed felsic and mafic rocks that record several episodes of magmatism, volcanism and deformation from the Permian to Early Cretaceous. This paper aims to constrain the age, affinity and deformation history of these units, as well as to establish the tectonic significance of the terrane. The trace-element compositions of mafic and felsic meta-igneous rocks record a change from MORB-like prior to ca 277 Ma to subduction-related by ca 258 Ma. Overprinting relationships between intrusive phases and deformation features reveal a relative chronology for the tectonothermal evolution of the area, while U–Pb and 40Ar/39Ar geochronology provides absolute age constraints. Deformation is localised around a NNE-striking tectonic contact that separates serpentinised ultramafic rocks from metamorphosed pillow lavas. Early formed ductile fabrics associated with the main episode of deformation (D1) preserve bulk flattening strains at greenschist-facies conditions. Emplacement and post-kinematic cooling ages of a pre-D1 quartz-monzonite dyke constrain the age of D1/M1 deformation and metamorphism to the period between ca 258 and ca 248 Ma. Minor brittle deformation (D2) occurred at ca 230 Ma, based on U–Pb dating of a syn-D2 diorite dyke (ca 231 ± 10 Ma) and several ca 230 Ma 40Ar/39Ar cooling ages. The deformation, metamorphism, and supra-subduction zone magmatism preserved on South Percy Island is correlated with the nearby Marlborough Terrane and more broadly with the second pulse of the Hunter–Bowen Orogeny, which affected much of the central and northern parts of eastern Australia in the late Permian and Early Triassic. Our results support previous suggestions that the second pulse of the Hunter–Bowen Orogeny involved coeval thrust systems in both the inboard and outboard parts of the orogen.

Funding

This work was partly funded by the Australian Research Council [grant number DP130100130] and the University of Queensland Argon Geochronology in Earth Science laboratory. Hoy was supported by an Australian Government Research Training Programme Scholarship, and Mortimer was supported by Core Research Funding to GNS Science from the New Zealand Ministry of Business, Innovation and Employment.

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