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Article: Geochronology, petrogenesis and tectonic significance of peraluminous granites from the Chinese Altai, NW China
Title | Geochronology, petrogenesis and tectonic significance of peraluminous granites from the Chinese Altai, NW China | ||||||||||||||
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Authors | |||||||||||||||
Keywords | Crustal structure Emplacement Geochronology Granite Igneous geochemistry | ||||||||||||||
Issue Date | 2011 | ||||||||||||||
Publisher | Elsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/lithos | ||||||||||||||
Citation | Lithos, 2011, v. 127 n. 1-2, p. 261-281 How to Cite? | ||||||||||||||
Abstract | The Paleozoic granites in the Chinese Altai are important for the study of tectonic evolution and crustal growth in the Central Asian Orogenic Belt (CAOB). Four representative peraluminous granitic intrusions were selected for systematic studies of zircon U-Pb and Hf isotopic compositions and whole-rock geochemical and Nd-Sr isotopic analyses. These rocks have high ASI (Alumina Saturation Index, Al 2O 3/(CaO+Na 2O+K 2O)=1.01-1.46 molecular ratios), with 0.6-5.6wt.% of normative corundum, and are characterized by moderately negative Eu anomalies (Eu/Eu*=0.38-0.98) and strong depletion in Ba, Nb and Sr elements. Our data suggest that these intrusions were emplaced from 419 to 393Ma, consistent with a period of intensive magmatic activities and high temperature metamorphism in the Chinese Altai. While in situ zircon Hf isotopic analyses for these granites give predominantly positive ε Hf(t) values (+0.8 to +12.8), a few inherited zircons yield negative ε Hf(t) values from -12.5 to -1.53. The U-Pb age and Hf isotopic data of these inherited zircons are similar to that of the widespread metasediments. In addition, the peraluminous granitic rocks have near-zero or negative ε Nd(t) values (-3.3 to -0.5) and relatively high initial 87Sr/ 86Sr ratios (0.7079-0.7266), distinct from those of the I-type granites in the study region, but similar to the Early Paleozoic Habahe sediments. These isotopic compositions suggest that the newly accreted metasediments of Habahe Group may be the major source rock of the peraluminous granites. The geochemical compositions indicate that their precursor magmas were derived from a relatively shallow crustal level (P≤5kbar) and zircon saturation temperatures suggest that these granitic intrusions were emplaced at 672-861°C. The peraluminous granitic magmas were generated by dehydration melting of newly accreted materials, which were possibly brought to at least middle crustal depth by subduction-related processes in an active margin, and were subsequently molten by strikingly high ambient temperature probably caused by upwelling of the hot asthenosphere associated with ridge subduction in the Paleozoic. © 2011 Elsevier B.V. | ||||||||||||||
Persistent Identifier | http://hdl.handle.net/10722/151332 | ||||||||||||||
ISSN | 2023 Impact Factor: 2.9 2023 SCImago Journal Rankings: 1.491 | ||||||||||||||
ISI Accession Number ID |
Funding Information: This study was supported by the National Basic Research Program of China (2007CB411308), Hong Kong Research Grants Council (HKU704307P), the National Natural Science Foundation of China (40721063, 40772130 and 40803009), the HKU CRCG Research Grants and Hong Kong-Germany Joint Research Scheme. We thank Biao Song, Liewen Xie, Yueheng Yang, Jianfeng Gao, Ying Liu, Guangqian, Hu, Jinlong Ma, Xianglin Tu and Xirong hang for laboratory assistance. We are grateful to Nelson Eby and two anonymous reviewers for their critical reviews and comments that significantly improved this manuscript. A HKU postgraduate studentship to Keda CAI is gratefully acknowledged. | ||||||||||||||
References |
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Cai, K | en_US |
dc.contributor.author | Sun, M | en_US |
dc.contributor.author | Yuan, C | en_US |
dc.contributor.author | Zhao, G | en_US |
dc.contributor.author | Xiao, W | en_US |
dc.contributor.author | Long, X | en_US |
dc.contributor.author | Wu, FY | en_US |
dc.date.accessioned | 2012-06-26T06:20:45Z | - |
dc.date.available | 2012-06-26T06:20:45Z | - |
dc.date.issued | 2011 | en_US |
dc.identifier.citation | Lithos, 2011, v. 127 n. 1-2, p. 261-281 | en_US |
dc.identifier.issn | 0024-4937 | en_US |
dc.identifier.uri | http://hdl.handle.net/10722/151332 | - |
dc.description.abstract | The Paleozoic granites in the Chinese Altai are important for the study of tectonic evolution and crustal growth in the Central Asian Orogenic Belt (CAOB). Four representative peraluminous granitic intrusions were selected for systematic studies of zircon U-Pb and Hf isotopic compositions and whole-rock geochemical and Nd-Sr isotopic analyses. These rocks have high ASI (Alumina Saturation Index, Al 2O 3/(CaO+Na 2O+K 2O)=1.01-1.46 molecular ratios), with 0.6-5.6wt.% of normative corundum, and are characterized by moderately negative Eu anomalies (Eu/Eu*=0.38-0.98) and strong depletion in Ba, Nb and Sr elements. Our data suggest that these intrusions were emplaced from 419 to 393Ma, consistent with a period of intensive magmatic activities and high temperature metamorphism in the Chinese Altai. While in situ zircon Hf isotopic analyses for these granites give predominantly positive ε Hf(t) values (+0.8 to +12.8), a few inherited zircons yield negative ε Hf(t) values from -12.5 to -1.53. The U-Pb age and Hf isotopic data of these inherited zircons are similar to that of the widespread metasediments. In addition, the peraluminous granitic rocks have near-zero or negative ε Nd(t) values (-3.3 to -0.5) and relatively high initial 87Sr/ 86Sr ratios (0.7079-0.7266), distinct from those of the I-type granites in the study region, but similar to the Early Paleozoic Habahe sediments. These isotopic compositions suggest that the newly accreted metasediments of Habahe Group may be the major source rock of the peraluminous granites. The geochemical compositions indicate that their precursor magmas were derived from a relatively shallow crustal level (P≤5kbar) and zircon saturation temperatures suggest that these granitic intrusions were emplaced at 672-861°C. The peraluminous granitic magmas were generated by dehydration melting of newly accreted materials, which were possibly brought to at least middle crustal depth by subduction-related processes in an active margin, and were subsequently molten by strikingly high ambient temperature probably caused by upwelling of the hot asthenosphere associated with ridge subduction in the Paleozoic. © 2011 Elsevier B.V. | en_US |
dc.language | eng | en_US |
dc.publisher | Elsevier BV. The Journal's web site is located at http://www.elsevier.com/locate/lithos | en_US |
dc.relation.ispartof | Lithos | en_US |
dc.subject | Crustal structure | en_US |
dc.subject | Emplacement | en_US |
dc.subject | Geochronology | en_US |
dc.subject | Granite | en_US |
dc.subject | Igneous geochemistry | en_US |
dc.title | Geochronology, petrogenesis and tectonic significance of peraluminous granites from the Chinese Altai, NW China | en_US |
dc.type | Article | en_US |
dc.identifier.email | Cai, K: caikd@hku.hk | en_US |
dc.identifier.email | Sun, M: minsun@hku.hk | en_US |
dc.identifier.email | Zhao, G: gzhao@hkucc.hku.hk | - |
dc.identifier.authority | Sun, M=rp00780 | en_US |
dc.identifier.authority | Zhao, G=rp00842 | en_US |
dc.description.nature | link_to_subscribed_fulltext | en_US |
dc.identifier.doi | 10.1016/j.lithos.2011.09.001 | en_US |
dc.identifier.scopus | eid_2-s2.0-80053630397 | en_US |
dc.identifier.hkuros | 204301 | - |
dc.relation.references | http://www.scopus.com/mlt/select.url?eid=2-s2.0-80053630397&selection=ref&src=s&origin=recordpage | en_US |
dc.identifier.volume | 127 | en_US |
dc.identifier.issue | 1-2 | en_US |
dc.identifier.spage | 261 | en_US |
dc.identifier.epage | 281 | en_US |
dc.identifier.isi | WOS:000298070600017 | - |
dc.publisher.place | Netherlands | en_US |
dc.identifier.scopusauthorid | Wu, F=40561925600 | en_US |
dc.identifier.scopusauthorid | Long, X=14012199100 | en_US |
dc.identifier.scopusauthorid | Xiao, W=7202456615 | en_US |
dc.identifier.scopusauthorid | Zhao, G=7403296321 | en_US |
dc.identifier.scopusauthorid | Yuan, C=35241599200 | en_US |
dc.identifier.scopusauthorid | Sun, M=25932315800 | en_US |
dc.identifier.scopusauthorid | Cai, K=14011943800 | en_US |
dc.identifier.citeulike | 9824268 | - |
dc.identifier.issnl | 0024-4937 | - |