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P. Schmoldt, PhD - MTNet - DIAS

P. Schmoldt, PhD - MTNet - DIAS

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7.1. Overview<br />

Geology of the Iberian Peninsula<br />

7<br />

The Iberian Peninsula is the westernmost extent of the Eurasian Continent, bordered by<br />

the Bay of Biscay to the north, the Atlantic Ocean to the west, the Mediterranean Sea<br />

to the south and southeast, and connected to the test of the Eurasian plate in the northeast<br />

(Fig. 7.1). Its most prominent topographic features are the Cantabrian Mountain<br />

Chain in the northwest, the Pyrenees in the northeast, the Betic Mountain Chain in the<br />

south, as well as the intraplate ranges Spanish Central System and Iberian Ranges. Thorough<br />

descriptions of the Iberian Peninsula geology are given for example in Gibbons and<br />

Moreno [2002b, and references within] and Moratti and Chalouan [2006, and references<br />

within]. A detailed overview about the geological evolution as well as past and presentday<br />

stress fields of the Iberian Peninsula are given in Andeweg [2002]; a compilation of<br />

figures therein, related to the PICASSO Phase I investigation, is given in Section A.1 in<br />

the appendix. A general summary of the events most relevant for the PICASSO Phase I<br />

investigation is given in the following paragraphs, focussing on the regions in the vicinity<br />

of the PICASSO Phase I profile. Therefore, this Chapter deals mostly with the tectonic<br />

settings of the Betic Cordillera and the Tajo Basin, including its subbasins and surrounding<br />

regions. But at first a general overview is given in the following paragraphs describing<br />

the main tectonic features of the Iberian Peninsula.<br />

Due to the distinct geological contrast between the eastern and western Iberian Peninsula<br />

these two parts are commonly referred to as Alpine Spain and Variscan Spain (sometimes<br />

also referred to as Hercynian Spain), respectively. The former is dominated by<br />

Mesozoic and Cenozoic sediments and young belts, whereas the latter comprises Precambrian<br />

and Palaeozoic rocks with minimal overprint by Alpine deformation [e.g. Gibbons<br />

and Moreno, 2002a]. The Variscan belt results from oblique collision and interaction between<br />

the Palaeozoic supercontinents Gondwana, Laurentia, and Baltica and a number<br />

of continental microplates taken place during Neoproterozoic through Palaeozoic times<br />

[Abalos et al., 2002]. The Iberian Massif, accounting for the majority of the Variscan<br />

133

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