Abstract
Introduction: The winding Variscan belt in Iberia, featuring the Cantabrian orocline (NW Iberia) and the Central Iberian curve, is a foremost expression of the late Carboniferous amalgamation of Pangea, which produced remagnetizations spanning almost the entire globe. Geological settings: Also in Iberia, late Carboniferous remagnetizations are widespread often hindering paleomagnetic interpretations in terms of pre-Pangean geologic history. In contrast, such remagnetizations facilitated the kinematic study of the Cantabrian orocline. Immediately to its south is located the Central Iberian curve whose geometry and kinematics are under debate. Recent studies suggest that this putative structure cannot have formed in the same process as the Cantabrian orocline. Results: Here we present a paleomagnetic and rock magnetic study from Extremadura, a region in the utmost west of the southern limb of the Central Iberian curve. Our new results show two distinct remagnetization events in Paleozoic rocks in Extremadura: (1) Mesozoic or Cenozoic remagnetization occurring in dolomitized limestones and (2) late Carboniferous remagnetization in limestones, characterized by consistent shallow inclinations, but largely scattered declinations indicating a counter clockwise (CCW) vertical axis rotation. Pyrrhotite is documented as magnetic carrier in the limestones which testifies a remagnetization under anchimetamorphic conditions, i.e. during the Variscan orogeny. Interpretation: We interpret the declination scattering as a remagnetization coeval to the vertical axis rotation. The described CCW rotations are those expected for the southern limb of the Cantabrian orocline and are in disagreement with a late Carboniferous secondary origin for the Central Iberian bend, extending the Cantabrian orocline to at least most of the Iberian peninsula.
| Original language | English |
|---|---|
| Pages (from-to) | 583-600 |
| Number of pages | 18 |
| Journal | Journal of Iberian Geology |
| Volume | 43 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - Dec 2017 |
Funding
Acknowledgements We thank Alicia López-Carmona, Piedad Franco and Eva Manchado for their assistance with thin sections. M. Suárez provided X-Ray diffraction analysis for some of the studied samples. Daniël Brouwer helped to collect and analyze the DB samples. We thank two anonymous reviewers their insights and help to improve this paper. DPG is funded by a Japan Society for Promotion of Science (JSPS) fellowship for overseas researchers (P16329) and a MEXT/JSPS KAKENHI Grant (JP16F16329). GGA is funded by the Spanish Ministry of Economy and Competitiveness under the project ODRE III-Oroclines and Delamination: Relations and Effects (CGL2013-46061-P) and project Origin, metallogeny, climatic effects and cyclicity of Large Igneous Provinces (LIPs)(§ 14.Y26.31.0012) funded by the Russian Federation. DPG wants to acknowledge Billy Shears on its 50th anniversary for this 20 years of raising my smile. This paper is part of UNESCO IGCP Projects 574: Buckling and Bent Orogens, and Continental Ribbons; 597: Amalgamation and breakup of Pangaea: The Type Example of the Supercontinent Cycle; and 648: Supercontinent Cycles and Global Geodynamics.
Keywords
- Cantabrian orocline
- Carboniferous tectonics
- Central Iberian zone
- Paleomagnetism
- Remagnetization