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dc.contributor.authorUysal, Ibrahim
dc.contributor.authorDokuz, Abdurrahman
dc.contributor.authorKapsiotis, Argyrios
dc.contributor.authorSaka, Samet
dc.contributor.authorKarsli, Orhan
dc.contributor.authorKaliwoda, Melanie
dc.contributor.authorMueller, Dirk
dc.date.accessioned2021-11-09T19:50:12Z
dc.date.available2021-11-09T19:50:12Z
dc.date.issued2017
dc.identifier.issn1367-9120
dc.identifier.issn1878-5786
dc.identifier.urihttps://doi.org/10.1016/j.jseaes.2017.08.012
dc.identifier.urihttps://hdl.handle.net/20.500.12440/4213
dc.description.abstractThe eastern Orhaneli ophiolite in NW Anatolia (Turkey) consists of voluminous dunite and minor harzburgite intruded by clinopyroxenite veins. Harzburgite contains spinel of low Cr# [100 x Cr/(Cr + Al) = 40-45] and diopside of low Al2O3 and TiO2 contents, whereas dunite contains spinel of higher Cr# (62-82) and diopside (blebs) (even more) depleted in Al2O3 and TiO2 (than harzburgite). The concentrations of Heavy Rare Earth Elements (HREE) in harzburgite are consistent with derivation of this type of peridotite from 19% dry melting of a fertile mantle protolith at a MOR regime. Dunites have lower concentrations of HREE than harzburgite implying that dunites were generated by higher degrees (> 30%) of (cumulative) melting of the same protolith. Furthermore, the characteristic U-shapes of the chondrite-normalized REE-patterns of dunites indicate the involvement of hydrous melt-peridotite interaction processes in their genesis. Nevertheless, a set of mosaic-in texture dunite samples contain olivine that has lower Fo# [100 x Mg/(Mg + Fe2+)] and NiO contents than olivine in harzburgite. These dunites are probably of cumulate origin as it is also indicated by their enrichment in Pt and Pd (<= 17.92 ppb). Micro-textural and Re-Os isotopic data support that clinopyroxenite intrusions do not have a pure magmatic origin and their formation was partly controlled by metasomatic processes. Overall data indicate that the eastern Orhaneli ultramafic rocks have a complex petrological history including various stages of partial melting, metasomatism and magmatism in an evolving from MOR to SSZ geotectonic setting.en_US
dc.description.sponsorshipScientific Research Foundation of Karadeniz Technical University [2008.112.005.17]; National Natural Science Foundation of China (NNSFC)National Natural Science Foundation of China (NSFC) [41402065]en_US
dc.description.sponsorshipThis study was financially supported by the Scientific Research Foundation of Karadeniz Technical University (Project# 2008.112.005.17) and the National Natural Science Foundation of China (NNSFC; Youth Science Fund Project# 41402065). We would like to express our sincere thanks to P. Stutz for his help in the preparation of the polished-thin sections. Editor Dr. Derek Wyman and an anonymous reviewer are thanked for their critical and constructive comments.en_US
dc.language.isoengen_US
dc.publisherPergamon-Elsevier Science Ltden_US
dc.relation.ispartofJournal of Asian Earth Sciencesen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.subjectPartial meltingen_US
dc.subjectMetasomatismen_US
dc.subjectPeridotitesen_US
dc.subjectOphiolitesen_US
dc.subjectTurkeyen_US
dc.titlePetrogenesis of ultramafic rocks from the eastern Orhaneli ophiolite, NW Turkey: Hints on the initiation and evolution of melt-peridotite interaction processes within a heterogeneously depleted mantle sectionen_US
dc.typearticleen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.description.wospublicationidWOS:000413384800004en_US
dc.description.scopuspublicationid2-s2.0-85028970979en_US
dc.departmentGümüşhane Üniversitesien_US
dc.authoridUysal, Ibrahim / 0000-0001-7607-2893
dc.identifier.volume148en_US
dc.identifier.startpage51en_US
dc.identifier.doi10.1016/j.jseaes.2017.08.012
dc.identifier.endpage64en_US
dc.authorwosidUysal, Ibrahim / AAE-3044-2019
dc.authorwosidSaka, Samet / AAN-7212-2021
dc.authorscopusid50062274000
dc.authorscopusid13406528500
dc.authorscopusid14826727100
dc.authorscopusid55619008100
dc.authorscopusid6506159221
dc.authorscopusid16203011000
dc.authorscopusid57199771951


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