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Article: U-Pb and Hf isotopic study of detrital zircons from the Wulashan khondalites: Constraints on the evolution of the Ordos Terrane, Western Block of the North China Craton

TitleU-Pb and Hf isotopic study of detrital zircons from the Wulashan khondalites: Constraints on the evolution of the Ordos Terrane, Western Block of the North China Craton
Authors
KeywordsDetrital zircon
Khondalite
LA-ICPMS
North China Craton
U-Pb age, Hf isotope
Issue Date2006
PublisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/epsl
Citation
Earth And Planetary Science Letters, 2006, v. 241 n. 3-4, p. 581-593 How to Cite?
AbstractDetrital zircons from the Wulashan khondalites in the Ordos Terrane, western block of the North China Craton, give U-Pb ages between 1.84 and 2.32 Ga, showing that their provenance was dominated by Paleoproterozoic rocks, much younger than those exposed in the Eastern Block. These zircons have oscillatory growth zoning and possess ε Hf values between -8 and +9, suggesting derivation of their precursor magmas from old crust and juvenile materials from the mantle. The lowest ε Hf values of zircons with different ages give a line that intersects the depleted mantle line at about 2.6 Ga in a ε Hf vs. time diagram. This may imply that the precursor magma source in the deep level of the crust was largely separated from the mantle ∼2.6 Ga ago and therefore 2.6 Ga may be an important crustal formation period for the terrane. One khondalite sample has detrital zircons with a single age population at ∼2.0 Ga and positive ε Hf values from +1 to +9, clearly recording the significant addition of juvenile materials at ∼2.0 Ga in the source region. This may inspire us to seek whether there was a connection between a mantle superevent and the formation of Columbia supercontinent. Data of this study exclusively demonstrate that the Ordos Terrane was developed independently from the Eastern Block until assembly of the Columbia supercontinent. Therefore, tectonic models involving that the whole North China Craton was cratonized 2.5 Ga ago should be dismissed. © 2005 Elsevier B.V. All rights reserved.
Persistent Identifierhttp://hdl.handle.net/10722/48578
ISSN
2022 Impact Factor: 5.3
2020 SCImago Journal Rankings: 2.829
ISI Accession Number ID
References

 

DC FieldValueLanguage
dc.contributor.authorXia, Xen_HK
dc.contributor.authorSun, Men_HK
dc.contributor.authorZhao, Gen_HK
dc.contributor.authorWu, Fen_HK
dc.contributor.authorXu, Pen_HK
dc.contributor.authorZhang, Jen_HK
dc.contributor.authorLuo, Yen_HK
dc.date.accessioned2008-05-22T04:17:44Z-
dc.date.available2008-05-22T04:17:44Z-
dc.date.issued2006en_HK
dc.identifier.citationEarth And Planetary Science Letters, 2006, v. 241 n. 3-4, p. 581-593en_HK
dc.identifier.issn0012-821Xen_HK
dc.identifier.urihttp://hdl.handle.net/10722/48578-
dc.description.abstractDetrital zircons from the Wulashan khondalites in the Ordos Terrane, western block of the North China Craton, give U-Pb ages between 1.84 and 2.32 Ga, showing that their provenance was dominated by Paleoproterozoic rocks, much younger than those exposed in the Eastern Block. These zircons have oscillatory growth zoning and possess ε Hf values between -8 and +9, suggesting derivation of their precursor magmas from old crust and juvenile materials from the mantle. The lowest ε Hf values of zircons with different ages give a line that intersects the depleted mantle line at about 2.6 Ga in a ε Hf vs. time diagram. This may imply that the precursor magma source in the deep level of the crust was largely separated from the mantle ∼2.6 Ga ago and therefore 2.6 Ga may be an important crustal formation period for the terrane. One khondalite sample has detrital zircons with a single age population at ∼2.0 Ga and positive ε Hf values from +1 to +9, clearly recording the significant addition of juvenile materials at ∼2.0 Ga in the source region. This may inspire us to seek whether there was a connection between a mantle superevent and the formation of Columbia supercontinent. Data of this study exclusively demonstrate that the Ordos Terrane was developed independently from the Eastern Block until assembly of the Columbia supercontinent. Therefore, tectonic models involving that the whole North China Craton was cratonized 2.5 Ga ago should be dismissed. © 2005 Elsevier B.V. All rights reserved.en_HK
dc.format.extent192137 bytes-
dc.format.extent26624 bytes-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/msword-
dc.languageengen_HK
dc.publisherElsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/epslen_HK
dc.relation.ispartofEarth and Planetary Science Lettersen_HK
dc.rightsEarth and Planetary Science Letters. Copyright © Elsevier BV.en_HK
dc.rightsThis work is licensed under a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.-
dc.subjectDetrital zirconen_HK
dc.subjectKhondaliteen_HK
dc.subjectLA-ICPMSen_HK
dc.subjectNorth China Cratonen_HK
dc.subjectU-Pb age, Hf isotopeen_HK
dc.titleU-Pb and Hf isotopic study of detrital zircons from the Wulashan khondalites: Constraints on the evolution of the Ordos Terrane, Western Block of the North China Cratonen_HK
dc.typeArticleen_HK
dc.identifier.openurlhttp://library.hku.hk:4550/resserv?sid=HKU:IR&issn=0012-821X&volume=241&issue=3-4&spage=581&epage=593&date=2006&atitle=U–Pb+and+Hf+isotopic+study+of+detrital+zircons+from+the+Wulashan+khondalites:+Constraints+on+the+evolution+of+the+Ordos+Terrane,+Western+Block+of+the+North+China+Cratonen_HK
dc.identifier.emailXia, X: xpxia@hotmail.comen_HK
dc.identifier.emailSun, M: minsun@hku.hken_HK
dc.identifier.emailZhao, G: gzhao@hkucc.hku.hken_HK
dc.identifier.authorityXia, X=rp00815en_HK
dc.identifier.authoritySun, M=rp00780en_HK
dc.identifier.authorityZhao, G=rp00842en_HK
dc.description.naturepostprinten_HK
dc.identifier.doi10.1016/j.epsl.2005.11.024en_HK
dc.identifier.scopuseid_2-s2.0-30744457893en_HK
dc.identifier.hkuros120015en_HK
dc.relation.referenceshttp://www.scopus.com/mlt/select.url?eid=2-s2.0-30744457893&selection=ref&src=s&origin=recordpageen_HK
dc.identifier.volume241en_HK
dc.identifier.issue3-4en_HK
dc.identifier.spage581en_HK
dc.identifier.epage593en_HK
dc.identifier.isiWOS:000235289000019-
dc.publisher.placeNetherlandsen_HK
dc.identifier.scopusauthoridXia, X=35241486400en_HK
dc.identifier.scopusauthoridSun, M=25932315800en_HK
dc.identifier.scopusauthoridZhao, G=7403296321en_HK
dc.identifier.scopusauthoridWu, F=40561925600en_HK
dc.identifier.scopusauthoridXu, P=49161291100en_HK
dc.identifier.scopusauthoridZhang, J=9940975100en_HK
dc.identifier.scopusauthoridLuo, Y=49161174100en_HK
dc.identifier.issnl0012-821X-

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