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Geological Society, London, Special Publications; 2009; v. 327; p. 343-369;
DOI: 10.1144/SP327.15
© 2009 Geological Society of London

Palaeozoic/Neoproterozoic orogens

Rheic Ocean mafic complexes: overview and synthesis

J. Brendan Murphy1,*, Gabriel Gutiérrez-Alonso2, R. Damian Nance3, Javier Fernández-Suárez4, J. Duncan Keppie5, Cecilio Quesada6, Jaroslav Dostal7 & James A. Braid1

1 Department of Earth Sciences, St. Francis Xavier University, Antigonish, Nova Scotia, B2G 2W5 Canada
2 Departamento de Geología, Universidad de Salamanca, 33708 Salamanca, Spain
3 Department of Geological Sciences, Ohio University, Athens, Ohio 45701, USA
4 Departamento de Petrología y Geoquímica, Universidad Complutense, 28040, Madrid, Spain
5 Departamento de Geología Regional, Instituto de Geologia, Universidad Nacional Autonoma de Mexico, 04510 Mexico D.F. México
6 IGME, c/Ríos Rosas 23, 28003, Madrid, Spain
7 Department of Geology, St. Mary's University, Halifax, Nova Scotia, B3H 3C3 Canada

* Corresponding author (e-mail: bmurphy{at}stfx.ca)

The Rheic Ocean formed during the Late Cambrian–Early Ordovician when peri-Gondwanan terranes (e.g. Avalonia) drifted from the northern margin of Gondwana, and was consumed during the collision between Laurussia and Gondwana and the amalgamation of Pangaea. Several mafic complexes, from the Acatlán Complex in Mexico to the Bohemian Massif in eastern Europe, have been interpreted to represent vestiges of the Rheic Ocean. Most of these complexes are either Late Cambrian–Early Ordovician or Late Palaeozoic in age. Late Cambrian–Early Ordovician complexes are predominantly rift-related continental tholeiites, derived from an enriched c. 1.0 Ga subcontinental lithospheric mantle, and are associated with crustally-derived felsic volcanic rocks. These complexes are widespread and virtually coeval along the length of the Gondwanan margin. They reflect magmatism that accompanied the early stages of rifting and the formation of the Rheic Ocean, and they remained along the Gondwanan margin to form part of a passive margin succession as Avalonia and other peri-Gondwanan terranes drifted northward. True ophiolitic complexes of this age are rare, a notable exception occurring in NW Iberia where they display ensimatic arc geochemical affinities. These complexes were thrust over, or extruded into, the Gondwanan margin during the Late Devonian–Carboniferous collision between Gondwana and Laurussia (Variscan orogeny). The Late Palaeozoic mafic complexes (Devonian and Carboniferous) preserve many of the lithotectonic and/or chemical characteristics of ophiolites. They are characterized by derivation from an anomalous mantle which displays time-integrated depletion in Nd relative to Sm. Devonian ophiolites pre-date closure of the Rheic Ocean. Although their tectonic setting is controversial, there is a consensus that most of them reflect narrow tracts of oceanic crust that originated along the Laurussian margin, but were thrust over Gondwana during Variscan orogenesis. The relationship of the Carboniferous ophiolites to the Rheic Ocean sensu stricto is unclear, but some of them apparently formed in a strike-slip regimes within a collisional setting directly related to the final stages of the closure of the Rheic Ocean.