6. PROVENANCE OF THE HP-HT UPPER ALLOCHTHON
109
Provenance of the HP
–
HT subducted margin in the Variscan
belt (Cabo Ortegal Complex, NW Iberian Massif)
R. ALBERT,
1
R. ARENAS,
1
A. GERDES,
2,3
S. SANCHEZ MARTINEZ
1
AND L. MARKO
2
1
Departamento de Petrologıa y Geoquımica & Instituto de Geociencias (UCM, CSIC), Universidad Complutense, 28040,
Madrid, Spain
(r.albert@geo.ucm.es)
2
Institut f
€
ur Geowissenschaften, Goethe
–
University Frankfurt, 60438, Frankfurt, Germany
3
Department of Earth Sciences, Stellenbosch University, Private Bag X1, Matieland, South Africa
ABSTRACT
The Variscan Upper Allochthon is a continental-affinity terrane that recorded a Cambrian
–
Ediacaran
magmatic arc generation, a subsequent transition to a passive margin, and a collision-related high-
P
metamorphism during the Devonian
–
Carboniferous amalgamation of Pangea. The objective of this
article is to decipher which continental margin subducted in the Devonian high-
P
–
high-
T
(HP
–
HT)
event. To do so, a provenance study is presented using combined U
–
Pb (
n
=
613) and Lu
–
Hf
(
n
=
463) isotopic LA
–
ICP
–
MS zircon analyses and Sm
–
Nd whole
–
rock (
n
=
5) determinations.
These analyses have been performed on five samples of the Banded Gneisses (Cabo Ortegal Complex,
NW Iberia), which forms a part of the HP
–
HT bottom member of the Upper Allochthon. Palaeozoic
–
Neoproterozoic zircon ages (34.7%) have a maximum abundance at 522
–
512 Ma, peaks at 575, 561,
545 Ma and minor abundance peaks between 780 and 590 Ma, and show from their Lu
–
Hf composi-
tions a volcanic arc mixing pattern. This arc was probably related to the Cadomian arc system. The
Mesoproterozoic population is scarce and scattered (2.8%), and due to its Lu
–
Hf pattern, it is pro-
posed that this population is also West Africa Craton derived. The Paleoproterozoic population
(39.6%) is concentrated at 2.07 Ga and it is linked to the Eburnean Orogeny, where depleted mantle
derived magmas intruded an Archean craton margin. This craton is represented by the Archean pop-
ulation (22.8%), which is grouped at 3.0, 2.68-2.61 and 2.52-2.48 Ga, and shows long-term reworking
processes and at least two juvenile magma intrusions. These data show that the Variscan Upper
Allochthon has a West African provenance and therefore, it strongly suggests that the NW Iberian
allochthonous complexes and their correlative European terranes are also West Africa derived. These
results allow us to finally clarify that the first high-
P
event, recorded during the eo-Variscan amalga-
mation of Pangea, was attained by the subduction of the margin of Gondwana under Laurussia.
Key words:
Cabo Ortegal; LAICPMS; Lu
–
Hf; U
–
Pb; Variscan Allochthon.
INTRODUCTION
The Variscan belt is a long orogen developed during
the main stages of the Pangea assembly as a result of
the collision of two large continents, Gondwana to
the South and Laurussia to the North (Matte, 1991,
2001; Winchester
et al.
, 2002; Martınez Catalan
et al.
, 2009; Arenas
et al.
, 2014a). It is considered
that the final assemblage of Pangea took place
between Devonian and Early Permian, and that the
continental collision followed the closure of the main
Palaeozoic ocean, the Rheic Ocean. This ocean was
generated after the Late Cambrian
–
Early Ordovician,
after rifting and progressive north drift of Avalonia
and other peri-Gondwanan terranes (Stampfli &
Borel, 2002; Murphy
et al.
, 2006; Arenas
et al.
, 2007;
Murphy & Nance, 2008; Nance
et al.
, 2010). The
Variscan belt can be followed from Iberia, across
Brittany and the French Massif Central, to the Bohe-
mian Massif, extending towards the basement of the
Alps, Corsica and Sardinia (Fig. 1a). The orogen was
linear in origin, but it was affected by several late- to
post-orogenic oroclinal bends that hinder correlations
across the belt (Matte, 2001; Martınez Catalan, 2011;
Weil
et al.
, 2013). The Variscan orogen has continu-
ity in eastern North America in the Appalachian
–
Al-
leghanian Belt.
The Variscan orogen contains a long suture zone
outlined by several allochthonous terranes with ophi-
olites and high-
P
units (Fig. 1a). They preserve the
most significant information in relation to the oldest
orogenic events and the evolution of the oceanic
domains that preceded the collision. Therefore, a
clear understanding of the origin and tectonothermal
evolution of these terranes is a key issue to improve
the knowledge about the initial interaction between
Gondwana and Laurussia. The orogen is character-
ized by the development of two high-
P
events with
©
2015 John Wiley & Sons Ltd
959
J. metamorphic Geol.,
2015,
33,
959–979
doi:10.1111/jmg.12155




