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dc.contributor.author
Liu, Sheng-Ao
dc.contributor.author
Li, Shuguang
dc.contributor.author
He, Yongsheng
dc.contributor.author
Huang, Fang
dc.date.accessioned
2024-08-19T09:45:47Z
dc.date.available
2024-08-19T09:43:06Z
dc.date.available
2024-08-19T09:45:47Z
dc.date.issued
2010-12-15
dc.identifier.issn
0016-7037
dc.identifier.issn
1872-9533
dc.identifier.other
10.1016/j.gca.2010.09.003
en_US
dc.identifier.uri
http://hdl.handle.net/20.500.11850/689454
dc.description.abstract
Adakites are commonly associated with porphyry Cu–Au ore deposits worldwide. Two groups of early Cretaceous adakites occur widely in central-eastern China but their association with mineralization contrasts sharply: adakites from the Lower Yangtze River Belt (LYRB) host one of the largest porphyry Cu–Au deposit belts in China, whereas those from the South Tan-Lu Fault (STLF), which is adjacent to the LYRB, are all ore-barren. These adakites, thus, provide a rare opportunity to explore the main factor that controls the genetic links between adakites and Cu–Au mineralization. Here we report new chronological, elemental and Sr–Nd–Pb isotopic data and present a comprehensive geochemical comparison for these two groups of adakites. At a given SiO2, the STLF adakites show lower Al2O3 and higher K2O, K2O/Na2O, MgO, Cr, Ni and Mg# than the LYRB adakites. These systematic differences may indicate a dry basaltic source for the STLF adakites and a water-enriched basaltic source for the LYRB adakites. The STLF adakites have high Sr/Y and (La/Yb)N, which are positively correlated, and low Sr/La and Ce/Pb, while the LYRB adakites show lower (La/Yb)N but higher Sr/Y, Sr/La and Ce/Pb than the STLF adakites. Furthermore, the LYRB adakites are characterized by highly radiogenic Pb isotopic compositions with 206Pb/204Pb(t) up to 18.8, which are clearly distinct from the STLF adakites with low radiogenic Pb (206Pb/204Pb(t) = 15.8–16.4). Although the high Mg# of the two groups of adakites suggest reaction with mantle peridotites during magma ascent, the geochemical comparisons indicate that the STLF adakites were derived from partial melting of the delaminated eclogitic lower continental crust, while the LYRB adakites were derived from partial melting of the seawater-altered oceanic crust that was being subducted towards the LYRB during the early Cretaceous. The petrogenetic contrasts between these two groups of high-Mg adakites, therefore, indicate that the large-scale Cu–Au mineralization is associated with oceanic slab melting, not delamination or recycling of the ancient lower continental crust, as previously proposed.
en_US
dc.language.iso
en
en_US
dc.publisher
Elsevier
en_US
dc.title
Geochemical contrasts between early Cretaceous ore-bearing and ore-barren high-Mg adakites in central-eastern China: Implications for petrogenesis and Cu–Au mineralization
en_US
dc.type
Journal Article
dc.date.published
2010-09-07
ethz.journal.title
Geochimica et Cosmochimica Acta
ethz.journal.volume
74
en_US
ethz.journal.issue
24
ethz.journal.abbreviated
Geochim. Cosmochim. Acta
ethz.pages.start
7160
en_US
ethz.pages.end
7178
en_US
ethz.identifier.wos
ethz.publication.place
New York, NY
ethz.publication.status
published
en_US
ethz.leitzahl
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02330 - Dep. Erd- und Planetenwissenschaften / Dep. of Earth and Planetary Sciences::02725 - Institut für Geochemie und Petrologie / Institute of Geochemistry and Petrology::03592 - Schmidt, Max / Schmidt, Max
en_US
ethz.leitzahl.certified
ETH Zürich::00002 - ETH Zürich::00012 - Lehre und Forschung::00007 - Departemente::02330 - Dep. Erd- und Planetenwissenschaften / Dep. of Earth and Planetary Sciences::02725 - Institut für Geochemie und Petrologie / Institute of Geochemistry and Petrology::03592 - Schmidt, Max / Schmidt, Max
ethz.date.deposited
2017-06-09T06:53:49Z
ethz.source
ECIT
ethz.identifier.importid
imp59364d3cd65a210087
ethz.identifier.importid
imp59364d7d6bc7836136
ethz.ecitpid
pub:41539
ethz.ecitpid
pub:46533
ethz.eth
yes
en_US
ethz.availability
Metadata only
en_US
ethz.rosetta.installDate
2024-08-19T09:43:08Z
ethz.rosetta.lastUpdated
2024-08-19T09:43:08Z
ethz.rosetta.exportRequired
true
ethz.rosetta.versionExported
true
dc.identifier.olduri
http://hdl.handle.net/20.500.11850/25696
dc.identifier.olduri
http://hdl.handle.net/20.500.11850/162510
ethz.COinS
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