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dc.contributor.authorJacobs, Joachim
dc.contributor.authorPaoli, Gabriele
dc.contributor.authorRocchi, Sergio
dc.contributor.authorKsienzyk, Anna Katharina
dc.contributor.authorSirevaag, Hallgeir
dc.contributor.authorElburg, Marlina
dc.date.accessioned2020-05-12T12:30:58Z
dc.date.available2020-05-12T12:30:58Z
dc.date.issued2018-02-09
dc.identifier.citationJacobs J, Paoli G, Rocchi S, Ksienzyk AK, Sirevaag H, Elburg M. Alps to Apennines zircon roller coaster along the Adria microplate margin. Scientific Reports. 2018;8:2704.eng
dc.identifier.urihttp://hdl.handle.net/1956/22204
dc.description.abstractWe have traced the particle path of high-pressure metasedimentary rocks on Elba Island, Northern Apennines, with the help of a U-Pb-Hf detrital zircon study. One quarter of the analysed zircons are surprisingly young, 41-30 Ma, with a main age peak at ca. 32 Ma, indicating an unexpected early Oligocene maximum deposition age. These Oligocene ages with negative εHf indicate a volcanic source region in the central-southern Alps. Though young by geological means, these zircons record an extraordinary geodynamic history. They originated in a volcanic arc, during the convergence/collision of the the Adria microplate with Europe from ca. 65 to 30 Ma. Thereafter, the Oligocene zircons travelled ca. 400 km southward along the Adria margin and the accretionary prism to present-day Tuscany, where they were subducted to depths of at least 40 km. Shortly thereafter, they were brought to the surface again in the wake of hinge roll back of the Apennine subduction zone and the resulting rapid extensional exhumation. Such a zircon roller coaster requires a microplate that has back-to-back subduction zones with opposing polarities on two sides.eng
dc.language.isoengeng
dc.publisherNature Researcheng
dc.rightsAttribution CC BYeng
dc.rights.urihttp://creativecommons.org/licenses/by/4.0eng
dc.titleAlps to Apennines zircon roller coaster along the Adria microplate margineng
dc.typeJournal articleeng
dc.date.updated2020-02-17T09:41:39Z
dc.rights.holderCopyright 2018 The Author(s)eng
dc.type.versionpublishedVersioneng
bora.peerreviewedPeer reviewedeng
dc.type.documentJournal article
dc.identifier.cristinID1619432
dc.identifier.doi10.1038/s41598-018-20979-weng
dc.source.issn2045-2322eng
dc.relation.journalScientific Reports


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