Re-folded structure of syn-orogenic granitoids (Padrón dome, NW Iberia): Assessing rheological evolution of cooling continental crust in a collisional setting

dc.contributor.authorDíez Fernández, Rubén
dc.contributor.authorRubio Pascual, Francisco J.
dc.contributor.authorMartín Parra, Luis Miguel
dc.date.accessioned2023-06-17T13:21:11Z
dc.date.available2023-06-17T13:21:11Z
dc.date.issued2019-03
dc.description.abstractThis contribution discusses about the rheological, kinematic and dynamic frameworks necessary to produce recumbent and upright folds from syn-orogenic granitic massifs that were formed during an early stage of magma genesis related to the onset of a migmatitic dome. Syn-kinematic granitoids occurring within the high-grade infrastructure of the Padrón migmatitic dome (NW Iberia) are deformed into large-scale recumbent folds (D2) that are later affected by upright folds (D3). Petrostructural analysis of a selected area of this dome reveals that after a period of crustal thickening (D1), NNW-directed extensional flow gave way to recumbent folds and penetrative axial plane foliation (S2). Superimposed subhorizontal compression resulted in upright folds (D3). A closer view into the dynamics of the dome allows exploring the factors that may condition the nucleation of folds with contrasting geometries during progressive deformation of molten continental crust. The formation of folds affecting syn-kinematic granitoids suggests a cooling metamorphic path in migmatitic domes. Active and passive folding mechanisms require a crystallizing (cooling) magma to nucleate folds. A more competent metamorphic host inhibits fold nucleation from much less competent magmas. As it crystallizes, magma becomes more rigid (competent), and approaches viscosity values of its host. Passive folding is favored when no significant competence contrast exists between magma and host, so this folding mechanism is more likely shortly after magma genesis and emplacement. In such conditions, and under dominant subhorizontal flow accompanied by flattening (D2), passive folding would produce isoclinal recumbent geometries. Further magma cooling introduces a shift into the rheological behavior of partially molten crust. Thereon, crystallizing magma bodies would represent significant competence contrasts relative to their host. At this point, buckling is a more likely folding mechanism, and more regular, buckle folds re-fold previous structures after significant cooling. The geometry of resulting folds is upright due to dominant subhorizontal compression (D3) at this stage.
dc.description.departmentDepto. de Geodinámica, Estratigrafía y Paleontología
dc.description.facultyFac. de Ciencias Geológicas
dc.description.refereedTRUE
dc.description.sponsorshipMinisterio de Economía, Industria y Competitividad (MINECO)
dc.description.sponsorshipInstituto Geológico y Minero de España
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/54869
dc.identifier.doi10.1016/j.gsf.2018.03.007
dc.identifier.issn1674-9871
dc.identifier.officialurlhttps://www.sciencedirect.com/science/article/pii/S1674987118300860
dc.identifier.relatedurlhttps://www.sciencedirect.com/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/13202
dc.issue.number2
dc.journal.titleGeoscience Frontiers
dc.language.isoeng
dc.page.final669
dc.page.initial651
dc.publisherElsevier
dc.relation.projectIDCGL2016-76438-P
dc.relation.projectIDIGME 2281
dc.rights.accessRightsrestricted access
dc.subject.cdu551.24(460)
dc.subject.keywordRecumbent folds
dc.subject.keywordMigmatitic domes
dc.subject.keywordPartial melting
dc.subject.keywordCrustal-derived granitoids
dc.subject.keywordOrogenic collapse
dc.subject.keywordVariscan orogen
dc.subject.ucmGeodinámica
dc.subject.ucmPetrología
dc.subject.unesco2507 Geofísica
dc.titleRe-folded structure of syn-orogenic granitoids (Padrón dome, NW Iberia): Assessing rheological evolution of cooling continental crust in a collisional setting
dc.typejournal article
dc.volume.number10
dspace.entity.typePublication
relation.isAuthorOfPublication5a03ae3f-5399-488e-b3ba-546c9011caa8
relation.isAuthorOfPublication.latestForDiscovery5a03ae3f-5399-488e-b3ba-546c9011caa8

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