P. Schmoldt, PhD - MTNet - DIAS
P. Schmoldt, PhD - MTNet - DIAS P. Schmoldt, PhD - MTNet - DIAS
7. Geology of the Iberian Peninsula Fig. 7.12.: Main morphostructural units of the south submeseta and their location in the Iberian Peninsula; modified after Gutierrez- Elorza et al. [2002] (note: Cuenca = Basin, Montes = Mountains, Sierra = Mountain range, Llanura = Plain, Rio = River); the location of map B is indicated by the red area in map A in the top-right of this figure. Iberian Range experienced intense deformation during the Middle Miocene, initiated by the Iberian – Internal Betics collision [e.g. Andeweg, 2002]. To the west of the Iberian Range, bordering the Tajo Basin to the northwest, the Spanish Central System (SCS; also referred to as Central Range or in Spanish as Sistema Central) forms a NE-SW trending mountain range branch. Outcrops of Variscan basement, associated with the Iberian Massif, contain mainly metamorphic and igneous rocks with granitic rocks dominating in the west and metamorphic rocks in the east [Tejero and Ruiz, 2002]. Details of the SCS formation process are not known at present, but several models have been proposed, describing the SCS as pop-up structure [Warburton and Alvarez, 1989; de Vicente et al., 1996; Tejero et al., 1996; Andeweg, 2002; Alonso-Zarza et al., 2002; Tejero and Ruiz, 2002, and references within], or as a flower structure [Portero and Aznar, 1984; Tejero et al., 1996] and attributing it to simultaneous strike-slip faulting and block rotation [Vegas et al., 1990]. The start of the SCS configuration is dated at the Eocene – Oligocene boundary, with sedimentation in the Loranca and Madrid Basin (Cuenca de Loranca and Cuenca de Madrid in Fig. 7.12) as well as in the Iberian Range evidencing that at least the northeastern region of the SCS was constructed at that time [Andeweg, 2002]. The Moho deepens beneath the SCS, reaching a depth of 34 km, primarily due to thickening of the lower crust [ILIHA DSS Group, 1993], which was attributed by Surinach and Vegas [1998] to Cretaceous – Miocene shear zone activity of the SCS comprising rotation of brittle upper crust segments, together with ductile deformation and thickening of 146
7.3. Tajo Basin and central Spain Fig. 7.13.: Geologic timescale with most relevant geologic events of the Tajo Basin the deeper crust, resulting in elevated topography. The contact between the SCS and the sediments of the Tajo Basin to the south is a NE-SW trending reverse fault with a throw of more than 2 km, active from Palaeogene into Middle Miocene times [Alonso-Zarza et al., 2002]. To the west of the Tajo Basin, accounting for the majority of the western region of the Iberian Peninsula, the Iberian Massif crops out, constituting the oldest part of the European Variscan orogeny formed during the Middle Devonian – Early Permian times as consequence of the collision between Laurentia and Gondwana [e.g Colmenero et al., 2002; Gibbons and Moreno, 2002a]. The Iberian Massif was above sea level during pre- Cenozoic times and had a planar and low relief [Stapel, 1999], but was subsequently deformed by various Cenozoic tectonic events resulting in an arcuate geometry [e.g. Andeweg, 2002; Colmenero et al., 2002; Gibbons and Moreno, 2002a, and references within]. The Iberian Massif consists mainly of igneous and metamorphic rocks and has commonly been divided into six zones or domains with the Precambrian outcrops of the Central-Iberian zone bordering the Tajo Basin to the west and south-west as well as to the north-west as part of the SCS [Colmenero et al., 2002; Tejero and Ruiz, 2002; Valladares et al., 2002] (Fig. 7.1). Location and shape of the interface between the Jurassic – Triassic rocks forming the Iberian Range and the Variscan rocks of the Iberian Massif below the Tajo is presently unclear, but since the Altomira Range is part of the Iberian Range the interface is most likely to be found to its west, below the Madrid Basin. Hence, crustal materials beneath the northern part of the PICASSO Phase I profile, located in the Loranca Basin and the Manchega Plain are presumably of Mesozoic times. Investigations of neotectonic stress tensors in the SCS and Madrid Basin [de Vicente 147
- Page 132 and 133: 5. Earth’s properties observable
- Page 134 and 135: 5. Earth’s properties observable
- Page 136 and 137: 5. Earth’s properties observable
- Page 138 and 139: 5. Earth’s properties observable
- Page 140 and 141: 5. Earth’s properties observable
- Page 142 and 143: 6. Using magnetotellurics to gain i
- Page 144 and 145: 6. Using magnetotellurics to gain i
- Page 146 and 147: 6. Using magnetotellurics to gain i
- Page 148 and 149: 6. Using magnetotellurics to gain i
- Page 150 and 151: 6. Using magnetotellurics to gain i
- Page 152 and 153: 6. Using magnetotellurics to gain i
- Page 154 and 155: 6. Using magnetotellurics to gain i
- Page 156 and 157: 6. Using magnetotellurics to gain i
- Page 158 and 159: 6. Using magnetotellurics to gain i
- Page 160 and 161: 6. Using magnetotellurics to gain i
- Page 162 and 163: 6. Using magnetotellurics to gain i
- Page 164 and 165: 6. Using magnetotellurics to gain i
- Page 168 and 169: Part II Geology of the study area I
- Page 170 and 171: 7. Geology of the Iberian Peninsula
- Page 172 and 173: 7. Geology of the Iberian Peninsula
- Page 174 and 175: 7. Geology of the Iberian Peninsula
- Page 176 and 177: 7. Geology of the Iberian Peninsula
- Page 178 and 179: 7. Geology of the Iberian Peninsula
- Page 180 and 181: 7. Geology of the Iberian Peninsula
- Page 184 and 185: 7. Geology of the Iberian Peninsula
- Page 186 and 187: 7. Geology of the Iberian Peninsula
- Page 188 and 189: 7. Geology of the Iberian Peninsula
- Page 190 and 191: 7. Geology of the Iberian Peninsula
- Page 192 and 193: 7. Geology of the Iberian Peninsula
- Page 194 and 195: 7. Geology of the Iberian Peninsula
- Page 196 and 197: 7. Geology of the Iberian Peninsula
- Page 198 and 199: 7. Geology of the Iberian Peninsula
- Page 200 and 201: 7. Geology of the Iberian Peninsula
- Page 202 and 203: 7. Geology of the Iberian Peninsula
- Page 205 and 206: Recovering a synthetic 3D subsurfac
- Page 207 and 208: direction direction Depth: 12 - 30
- Page 209 and 210: 8.2. Generating synthetic 3D model
- Page 211 and 212: Distance from the centre of the mes
- Page 213 and 214: 3D N45W 3D-crust TE Rho TE Phi Peri
- Page 215 and 216: 8.3. Inversion of 3D model data sch
- Page 217 and 218: Model variation RMS misfit Optimal
- Page 219 and 220: Profile: 3D-crust (TM-only) Depth (
- Page 221 and 222: Parameter Value 8.3. Inversion of 3
- Page 223 and 224: Depth (km) 10 -2 10 -1 10 0 10 1 10
- Page 225 and 226: Depth (km) 10 -2 10 -1 10 0 10 1 10
- Page 227 and 228: Step 1: Isotropic 2D inversion Step
- Page 229 and 230: 8.3. Inversion of 3D model data par
- Page 231 and 232: 8.4. Summary and conclusions bution
7.3. Tajo Basin and central Spain<br />
Fig. 7.13.: Geologic timescale with most relevant geologic events of the Tajo Basin<br />
the deeper crust, resulting in elevated topography. The contact between the SCS and the<br />
sediments of the Tajo Basin to the south is a NE-SW trending reverse fault with a throw of<br />
more than 2 km, active from Palaeogene into Middle Miocene times [Alonso-Zarza et al.,<br />
2002].<br />
To the west of the Tajo Basin, accounting for the majority of the western region of<br />
the Iberian Peninsula, the Iberian Massif crops out, constituting the oldest part of the<br />
European Variscan orogeny formed during the Middle Devonian – Early Permian times<br />
as consequence of the collision between Laurentia and Gondwana [e.g Colmenero et al.,<br />
2002; Gibbons and Moreno, 2002a]. The Iberian Massif was above sea level during pre-<br />
Cenozoic times and had a planar and low relief [Stapel, 1999], but was subsequently<br />
deformed by various Cenozoic tectonic events resulting in an arcuate geometry [e.g.<br />
Andeweg, 2002; Colmenero et al., 2002; Gibbons and Moreno, 2002a, and references<br />
within]. The Iberian Massif consists mainly of igneous and metamorphic rocks and has<br />
commonly been divided into six zones or domains with the Precambrian outcrops of the<br />
Central-Iberian zone bordering the Tajo Basin to the west and south-west as well as to the<br />
north-west as part of the SCS [Colmenero et al., 2002; Tejero and Ruiz, 2002; Valladares<br />
et al., 2002] (Fig. 7.1).<br />
Location and shape of the interface between the Jurassic – Triassic rocks forming the<br />
Iberian Range and the Variscan rocks of the Iberian Massif below the Tajo is presently<br />
unclear, but since the Altomira Range is part of the Iberian Range the interface is most<br />
likely to be found to its west, below the Madrid Basin. Hence, crustal materials beneath<br />
the northern part of the PICASSO Phase I profile, located in the Loranca Basin and the<br />
Manchega Plain are presumably of Mesozoic times.<br />
Investigations of neotectonic stress tensors in the SCS and Madrid Basin [de Vicente<br />
147