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5. PROVENANCE OF THE UPPER ALLOCHTHON

89

Provenance of the Variscan Upper Allochthon (Cabo Ortegal Complex,

NW Iberian Massif)

R. Albert

a

,

, R. Arenas

a

, A. Gerdes

b

,

c

, S. Sánchez Martínez

a

, J. Fernández-Suárez

a

, J.M. Fuenlabrada

d

a

Departamento de Petrología y Geoquímica and Instituto de Geociencias (UCM-CSIC), Universidad Complutense de Madrid, Spain

b

Institut für Geowissenschaften, Petrologie und Geochemie, J.W. Goethe Universität, Frankfurt am Main, Germany

c

Department of Earth Sciences, Stellenbosch University, Private Bag X1, Matieland, South Africa

d

CAI de Geocronología y Geoquímica Isotópica, Universidad Complutense de Madrid, Spain

a b s t r a c t

a r t i c l e i n f o

Article history:

Received 28 May 2014

Received in revised form 17 October 2014

Accepted 20 October 2014

Available online 15 November 2014

Handling Editor: I. Safonova

Keywords:

Detrital zircons

Provenance

Isotope geochemistry

Variscan Upper Allochthon

Cabo Ortegal Complex

This study focuses on the provenance of the uppermost unit of the Upper Allochthon of the Variscan belt with

combined U

Pb and Lu

Hf zircon (LA-ICPMS) and Sm

Nd whole-rock analyses. This unit is represented in the

Cabo Ortegal Complex (NW Iberia) by the metasiliciclastic Cariño Gneisses which overlap ophiolitic units that

represent perigondwanan oceanic domains. The data set indicates a maximum depositional age of c. 510 Ma

and a c. 1.73 Ga Sm

Nd model age, typifying a late or post Pan-African (or Cadomian) and Eburnean events,

which entailed abundant input of juvenile material involving broad mixing with older crustal sources. The

Mesoproterozoic activity is scarce and scattered and therefore unlikely to represent a major crust generation

pulse in the source area of the siliciclastic unit. The data set also records an Archean orogenic pulse in its source

area followed by a long lasting crust reworking process, where the Eburnean juvenile materials intruded. These

dataareinterpretedasindicativeofaWestAfricaCratonprovenance,wherethesiliciclasticseriesfromwhichthe

CariñoGneissesarederivedwereprobablydepositedinaback-arctypebasinwheredetrituswasmostlysourced

by the continent rather than the magmatic arc.

© 2014 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

1. Introduction

The Variscan

Appalachian

Alleghenian orogeny was formed when

the Pangea supercontinent assembled during Carboniferous and Early

Permian. Part of the European branch of this orogen, the Variscan belt,

is well preserved in the Iberian Massif. This Massif exhibits an almost

complete section of the southern part (present day coordinates) of the

orogen from the most external zones (Autochthon) to the internal

sectionswhicharerepresentedbytheParautochthonandtheallochtho-

nous complexes.

Our understanding of the sources and provenance of the rock series

involved in the Variscan Orogeny has signi

fi

cantly increased in the last

few years mostly driven by U

Pb and Lu

Hf zircon (LA-ICPMS) and

Sm

Nd whole rock studies. In the NW Iberian Massif most of the prov-

enance studies have been focussed on sedimentary series located below

the ophiolitic units, either in the autochthonous domain (Cantabrian

zone, CZ, West-Asturian

Leonese zone, WALZ, and Central Iberian

zone, CIZ,

Fig. 1

a,

Fernández-Suárez et al., 1999; Gutiérrez-Alonso

et al., 2003; Martínez Catalán et al., 2004; Fernández-Suárez et al.,

2013; Shaw et al., 2014

), the Parautochthon (

Díez Fernández et al.,

2012b

) or the basal units (

Díez Fernández et al., 2010

). These studies

suggest as a main conclusion that the rock series were formed at the pe-

riphery of the Gondwanan margin, between the Nubian platform and

the periphery of West African Craton (WAC), although their exact

location is still a matter of debate. The key for paleogeographic recon-

structions is usually focussed on the presence or absence of a Stenian

Tonian zircon population in Ediacaran and post-Ediacaran rock series.

Rocks containing this population are usually placed in front of the

Sahara Craton or the Nubian Shield (

Díez Fernández et al., 2010;

Fernández-Suárez et al., 2013; Shaw et al., 2014

), whereas those lacking

or having an extremely low quantity of it are considered to have a

proximal WAC provenance (

Abati et al., 2010a, 2012

). Nevertheless,

the real importance of the isotopic sources has not been completely

evaluated in NW Iberia as there are almost no previous studies integrat-

ing U

Pb/Lu

Hf (zircon) and Sm

Nd (whole rock) data systematics.

This kind of studies is absent in metasedimentary rock series and only

very few works have presented some of these combined results for

metaigneous rocks (i.e.

Sánchez Martínez et al., 2011

).

The Upper Allochthon or upper units is located above the ophiolitic

units, which are considered to represent the Variscan suture in the

NW Iberian Massif. This issue poses

fi

rst order questions, not only

about tectonic settings but also about provenance and sources of the in-

volved rockseries. In the Upper Allochthon, two works were carried out

separately publishing U

Pb detrital zircon and Sm

Nd whole rock data

on metagreywackes (

Fernández-Suárez et al., 2003; Fuenlabrada et al.,

Gondwana Research 28 (2015) 1434

1448

Corresponding author.

E-mail address:

r.albert@geo.ucm.es

(R. Albert).

http://dx.doi.org/10.1016/j.gr.2014.10.016

1342-937X/© 2014 International Association for Gondwana Research. Published by Elsevier B.V. All rights reserved.

Contents lists available at

ScienceDirect

Gondwana Research

journal homepage:

www.elsevier.com/locate/gr