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Trace inheritance—Clarifying the zircon O-Hf isotopic fingerprint of I-type granite sources: Implications for the restite model

dc.contributor.authorJeon, Heejin
dc.contributor.authorWilliams, Ian S.
dc.date.accessioned2018-01-04T23:52:50Z
dc.date.issued2018-01-05
dc.description.abstractEarly to mid Carboniferous I-type granites distributed in a broad meridional belt west of Sydney, southeastern Australia, represent the last phase of granite magmatism in the southern Lachlan Fold Belt. Rare inherited zircon in the granites, in combination with zircon precipitated from the melt phase of the magmas, provides direct evidence of the nature and age of the source rocks from which the granites were derived, and the isotopic compositions of those rocks. Most granites from the north and central parts of the belt, represented by the Wuuluman, Home Rule, Oberon and Lett plutons (334 ± 3, 328 ± 4, 339 ± 2 and 328 ± 2 Ma, respectively), are characterized by scarce inherited zircon dominantly of Siluro-Devonian age, consistent with all being derived from a common zircon-poor source rock of mid to late Devonian age. Based on the isotopic compositions of the igneous zircon rims, that source was relatively homogeneous and immature (δ18Ozrn 6–7‰, εHf(t) 0–+4). Two samples of the Tarana pluton (331 ± 2 Ma), near the centre of the belt, show evidence for heterogeneity in that source and the presence of a more evolved component that is also more zircon rich. Together with the Lett pluton from the same geochemical suite, their zircon rim compositions define a mixing array between more and less evolved end members (δ¹⁸Ozrn 5.5–9.5‰, εHf(t) -4–+4). Only in the southern Chapmans Creek pluton (327 ± 3 Ma) is there clear evidence that the source of the granite also contained a minor component with a similar older protolith to the LFB early Palaeozoic sediments that host most of the LFB pre-Carboniferous granites. Presence of that component, which overwhelmingly dominates the inheritance in the pre-Carboniferous granites, is also reflected in a slightly elevated whole rock initial ⁸⁷Sr/⁸⁶Sr (> 0.7050) and igneous δ¹⁸Ozrn (ca. 7.5‰), but not in the igneous zircon εHf(t) (ca. +2). The amount of restitic zircon in granite is determined by not only the proportion of restite present but also the zircon contents of the various source rock components. The process of restite unmixing does not necessarily mean that more mafic, restite-rich granites will contain more inherited zircon.en_AU
dc.description.sponsorshipThis work was funded by ARC grant DP0559604 to ISW. HJ also received support from an ANU PhD scholarship.en_AU
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn0009-2541en_AU
dc.identifier.urihttp://hdl.handle.net/1885/139067
dc.publisherElsevieren_AU
dc.relationhttp://purl.org/au-research/grants/arc/DP0559604en_AU
dc.rights© 2017 Elsevier B.V. http://www.sherpa.ac.uk/romeo/issn/0009-2541/..."Author's post-print on open access repository after an embargo period of between 12 months and 48 months" from SHERPA/RoMEO site (as at 4/01/18).en_AU
dc.sourceChemical Geologyen_AU
dc.subjectI-type granitesen_AU
dc.subjectLachlan Fold Belten_AU
dc.subjectO isotopesen_AU
dc.subjectHf isotopesen_AU
dc.subjectRestite modelen_AU
dc.subjectZircon inheritanceen_AU
dc.titleTrace inheritance—Clarifying the zircon O-Hf isotopic fingerprint of I-type granite sources: Implications for the restite modelen_AU
dc.typeJournal articleen_AU
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage468en_AU
local.bibliographicCitation.startpage456en_AU
local.contributor.affiliationJeon, H., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.affiliationWilliams, I. S., Research School of Earth Sciences, The Australian National Universityen_AU
local.contributor.authoruidu4472561en_AU
local.identifier.ariespublicationa383154xPUB9212
local.identifier.citationvolume476en_AU
local.identifier.doi10.1016/j.chemgeo.2017.11.041en_AU
local.publisher.urlhttps://www.elsevier.com/en_AU
local.type.statusAccepted Versionen_AU

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