New insights from an emplacement model for the Santa Eulália Plutonic Complex (SW Iberian Peninsula)

dc.contributor.authorCruz, Claudia
dc.contributor.authorNogueira, Pedro
dc.contributor.authorMáximo, Jaime
dc.contributor.authorNoronha, Fernando
dc.contributor.authorSant'Ovaia, Helena
dc.date.accessioned2024-11-06T12:39:53Z
dc.date.available2024-11-06T12:39:53Z
dc.date.issued2023
dc.description.abstractThe Santa Eulália Plutonic Complex is formed by two main granites: G0 and G1. The G0 granite hosts metasedimentary carbonate and pelitic rocks (roof pendants) and elongated masses of mafic–intermediate rocks (the M-group). The host rocks form a diverse sequence of igneous, metasedimentary and metamorphic rocks. The study area is constrained by Variscan structures formed in a transpressional/transtensional sinistral tectonic regime (the Tomar–Badajoz–Córdoba sinistral shear zone) and is cut by the Alter do Chão and Assumar faults. The geological complexity of the area makes it difficult to determine the emplacement mechanism of the pluton. We propose a model for the ascent and emplacement of the pluton that can also be applied to similar post-collision Variscan granites. The gravity anomalies suggest that the pluton is slightly asymmetrical and extends to the SSE beneath the host rocks; its main root is >8 km thick in its deepest areas. The available radiometric data for an extended area embracing several regional plutons suggest a west–east magmatic alignment. The Variscan structures probably formed efficient crustal discontinuities enabling the generation and ascent of magma. Our model involves a west–east magmatic axis for magma spreading along extensional fractures (T-fractures) related to the Tomar–Badajoz–Córdoba shear zone. The opening movement along these fractures created divergent forces that allowed the ascent and emplacement of the plutonic rocks. The importance of these fractures is represented well by outcrops of porphyritic biotite granites (the Ervedal, Fronteira and G1 granites).por
dc.identifier.authoremailclaudiacruz@fc.up.pt
dc.identifier.authoremailpmn@uevora.pt
dc.identifier.authoremailjfmaximo@gmail.com
dc.identifier.authoremailfmpnoronha@gmail.com
dc.identifier.authoremailhsantov@fc.up.pt
dc.identifier.citationCruz, C., Nogueira, P., Máximo, J., Noronha, F., & Sant'Ovaia, H. (2023). New insights from an emplacement model for the Santa Eulália Plutonic Complex (SW Iberian Peninsula). Journal of the Geological Society, 180(4), jgs2022-131.por
dc.identifier.doihttps://doi.org/10.1144/jgs2022-131por
dc.identifier.scientificarea249por
dc.identifier.urihttps://www.lyellcollection.org/doi/abs/10.1144/jgs2022-131
dc.identifier.urihttp://hdl.handle.net/10174/37503
dc.language.isoporpor
dc.peerreviewedyespor
dc.publisherJournal of the Geological Societypor
dc.rightsrestrictedAccesspor
dc.subjectGranite emplacementpor
dc.subjectSanta Eulalia Plutonic Complexpor
dc.subjectgravimetrypor
dc.subjectRadiometrypor
dc.titleNew insights from an emplacement model for the Santa Eulália Plutonic Complex (SW Iberian Peninsula)por
dc.typearticlepor

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