Lead isotope evolution of the Central European upper mantle: Constraints from the Bohemian Massif

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dc.contributor.authorKrmíčková, Simonacs
dc.contributor.authorKrmíček, Lukášcs
dc.contributor.authorRomer, Rolf L.cs
dc.contributor.authorUlrych, Jaromírcs
dc.coverage.issue3cs
dc.coverage.volume11cs
dc.date.issued2020-05-15cs
dc.description.abstractThe Pb isotope composition of the upper mantle beneath Central Europe is heterogeneous due to the subduction of regionally contrasting material during the Variscan and Alpine orogenies. Late Variscan to Cenozoic mantle-derived melts allow mapping this heterogeneity on a regional scale for the last ca. 340 Myr. Late Cretaceous and Cenozoic anorogenic magmatic rocks of the Bohemian Massif (lamprophyres, volcanic rocks of basanite/tephrite and trachyte/phonolite series) concentrate mostly in the Eger Rift. Cretaceous ultramafic lamprophyres yielded the most radiogenic Pb isotope signatures reflecting a maximum contribution from metasomatised lithospheric mantle, whereas Tertiary alkaline lamprophyres originated from mantle with less radiogenic Pb-206/Pb-204 ratios suggesting a more substantial modification of lithospheric source by interaction with asthenospheric-derived melts. Cenozoic volcanic rocks of the basanite/tephrite and trachyte/phonolite series define a linear mixing trend between these components, indicating dilution of the initial lithospheric mantle signature by up-welling asthenosphere during rifting. The Pb isotope composition of Late Cretaceous and Cenozoic magmatic rocks of the Bohemian Massif follows the same Pb growth curve as Variscan orogenic lamprophyres and lamproites that formed during the collision between Laurussia, Gondwana, and associated terranes. This implies that the crustal Pb signature in the post-Variscan mantle is repeatedly sampled by younger anorogenic melts. Most Cenozoic mantle-derived rocks of Central Europe show similar Pb isotope ranges as the Bohemian Massif.en
dc.formattextcs
dc.format.extent925-942cs
dc.format.mimetypeapplication/pdfcs
dc.identifier.citationGeoscience Frontiers. 2020, vol. 11, issue 3, p. 925-942.en
dc.identifier.doi10.1016/j.gsf.2019.09.009cs
dc.identifier.issn1674-9871cs
dc.identifier.orcid0000-0003-0943-9776cs
dc.identifier.other164482cs
dc.identifier.scopus36617317200cs
dc.identifier.urihttp://hdl.handle.net/11012/193490
dc.language.isoencs
dc.publisherCHINA UNIV GEOSCIENCES, BEIJINGcs
dc.relation.ispartofGeoscience Frontierscs
dc.relation.urihttps://www.sciencedirect.com/science/article/pii/S1674987119301744cs
dc.rightsCreative Commons Attribution-NonCommercial-NoDerivatives 4.0 Internationalcs
dc.rights.accessopenAccesscs
dc.rights.sherpahttp://www.sherpa.ac.uk/romeo/issn/1674-9871/cs
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/cs
dc.subjectLead isotopesen
dc.subjectLamprophyresen
dc.subjectVolcanic rocksen
dc.subjectMantle componentsen
dc.subjectBohemian massifen
dc.subjectVariscan orogenyen
dc.titleLead isotope evolution of the Central European upper mantle: Constraints from the Bohemian Massifen
dc.type.driverarticleen
dc.type.statusPeer-revieweden
dc.type.versionpublishedVersionen
sync.item.dbidVAV-164482en
sync.item.dbtypeVAVen
sync.item.insts2025.02.03 15:44:35en
sync.item.modts2025.01.17 15:16:51en
thesis.grantorVysoké učení technické v Brně. Fakulta stavební. Ústav geotechnikycs
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