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6. PROVENANCE OF THE HP-HT UPPER ALLOCHTHON

125

conclusive about the origin of the subducted conti-

nental margin, as subduction of either the Gond-

wanan margin to the North or the Laurussian

margin to the South could explain this tectonic evolu-

tion. However, the new provenance data presented in

this paper is conclusive on the origin of the Banded

Gneiss formation, whose eclogite facies evolution can

only be explained as generated during subduction of

the Gondwana margin directed to the North.

CONCLUSIONS

The sedimentary protoliths of the eclogitic gneisses

of the Cabo Ortegal Complex (Banded Gneisses) has

a Gondwanan provenance. They were deposited in a

sedimentary basin located in the periphery of West

Africa. This implies that the margin of Gondwana,

which developed a Cambrian

Ediacaran continental

magmatic arc and a subsequent transition to a pas-

sive margin, subducted during the Devonian below

another continent located to the North, most proba-

bly Laurussia. This tectonothermal event represents

a first collision related to the final assembly of Pan-

gea, as has been recently proposed (Arenas

et al.

,

2014a).

Due to the strong bimodal character of the U

Pb

detrital populations and the high amount of ages

near to the sedimentation age (Max. Dep.

Age

=

c.

521 Ma, Min. Dep. Age

=

c.

506 Ma) the

basin where these sediments deposited was probably

a back-arc type basin. The Lu

Hf data shows that

at this time the Cambrian

Ediacaran population

was formed in a continental

magmatic arc and

strongly suggests, due to timing and due to its

WAC provenance, that the arc system was the

Cadomian arc. The igneous activity of the arc lasted

at least until Middle Cambrian in the Iberian sector

of the Gondwanan margin. Comparing this study

with a previous one on the Iberian IP Upper

Allochthon (Albert

et al.

, 2015), it seems reasonable

to propose that the siliciclastic series involved in the

HP

HT Upper Allochthon deposited first (due to its

isotopic heterogeneity between samples and high

amount of basic and acid intrusions). The sedimen-

tary protoliths of the IP Upper Allochthon depos-

ited shortly after than the HP

HT Upper

Allochthon (due to its homogeneity and scarce

igneous intrusions) in the same basin. The NW Ibe-

rian IP Upper Allochthon scarcely registers Edi-

acaran arc igneous activity, probably because when

erosion and sedimentation of the detrital series took

place the topographic relief of the Ediacaran part of

the arc was dismantled.

Considering the original linear character of the

Variscan belt and the presence of a rather continuous

equivalent HP

HT unit from the Iberian Massif to

the Bohemian Massif, we suggest that the conclusions

presented in this article can be extrapolated to the

entire Variscan realm.

ACKNOWLEDGMENTS

This work was supported by the Ministerio de Econ-

omıa y Competividad (Spanish project CGL2012

34618). R. Albert is thankful to the Universidad

Complutense de Madrid which provided him with a

pre-doctoral grant. The authors are grateful to A.P.

Willner and J. Payne who performed insightful

reviews of the manuscript and to M. Brown for excel-

lent editing work. The authors are also thankful for

the technical and laboratory support provided by

J.M. Fuenlabrada and J.A. Hernandez Jimenez

(TIMS Laboratory, UCM).

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©

2015 John Wiley & Sons Ltd

PROVENANCE OF THE HP

HT VARISCAN TERRANE

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