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- W2017265938 abstract "The Shilu Fe-Co-Cu ore district is situated in the western Hainan Province of south China. This district consists of the upper Fe-rich layers and the lower Co-Cu ores, which are mainly hosted within the Neoproterozoic Shilu Group, a dominantly submarine siliciclastic and carbonate sedimentary succession that generally has been metamorphosed to greenschist facies. Three facies of metamorphosed BIFs, the oxide, the silicate-oxide and the sulfide-carbonate-silicate, have been identified within the Shilu Group. The oxide banded iron formation (BIF) fades (quartz itabirites or Fe-rich ores) consists of alternating hematite-rich and quartz-rich microbands. The silicate-oxide BIF facies (amphibolitic itabirites or Fe-poor ores) comprises alternating millimeter to tens of meter scale, magnetite-hematite-rich bands with calc-silicate-rich macro- to microbands. The sulfide-carbonate-silicate BIF facies (Co-Cu ores) contain alternating cobaltiferous pyrite, cobaltiferous pyrrhotite and chalcopyrite macrobands to microbands mainly with dolomite-calcite, but also with minor sericite-quartz bands. Blasto-oolitic, pelletoidal, colloidal, psammitic, and ayptoaystalline to microaystalline textures, and blasto-bedding structures, which likely represent primary sedimentation, are often observed in the Shilu BIF facies. The Shilu BIFs and interbedded host rocks are generally characterized by relatively low but variable Sigma REE concentrations, LREE depletion and/or MREE enrichment relative to HREE, and no Ce, Gd and Eu anomalies to strongly positive Ce, Gd and Eu anomalies in the upward-convex PAAS-normalized REY patterns, except for both the banded or impure dolostones with nil Ce anomaly to negative Ce anomalies and negative La anomalies, and the minor sulfide-carbonate-silicate BIF facies with moderately negative Eu anomalies. They also contain relatively low but variable HFSE abundances as Zr, Nb, Hf, Th and Ti, and relatively high but variable abundances of Cu, Co, Ni, Pb, As, Mn and Ba. The consistently negative epsilon(Nd)(t) values range from -4.8 to -8.5, with a T-DM age of ca. 2.0 Ga. In line with the covariations between Al2O3 and TiO2, Fe2O3 + FeO and SiO2, Mn and Fe, Zr and Y/Ho and REE, and Sc and LREE, the geochemical and Sm-Nd isotopic features suggest that the precursors to the Shilu BIFs formed from a source dominated by seafloor-derived, high- to low temperature, acidic and reducing hydrothermal fluids but with variable input of detrital components in a seawater environment. Moreover, the involved detrital materials were sourced dominantly from an unknown, Paleoproterozoic or older crust, with lesser involvement from the Paleo- to Mesoproterozoic Baoban Group underlying the Shilu Group. The Shilu BIFs of various fades are interpreted to have formed in a shallow marine, restricted or sheltered basin near the rifted continental margin most likely associated with the break-up of Rodinia as the result of mantle superplume activity in South China. The seafloor-derived, periodically upwelling metalliferous hydrothermal plume/vent fluids under anoxic but sulfidic to anoxic but Fe2+-rich conditions were removed from the plume/ vent and accumulated in the basin, and then variably mixed with terrigenous detrital components, which finally led to rhythmic deposition of the Shilu BIFs. (C) 2013 Elsevier B.V. All rights reserved." @default.
- W2017265938 created "2016-06-24" @default.
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- W2017265938 date "2014-03-01" @default.
- W2017265938 modified "2023-10-02" @default.
- W2017265938 title "Petrography and geochemistry of the Shilu Fe–Co–Cu ore district, South China: Implications for the origin of a Neoproterozoic BIF system" @default.
- W2017265938 cites W1520801330 @default.
- W2017265938 cites W1595389031 @default.
- W2017265938 cites W1631820701 @default.
- W2017265938 cites W1965047767 @default.
- W2017265938 cites W1965536973 @default.
- W2017265938 cites W1968486409 @default.
- W2017265938 cites W1969248880 @default.
- W2017265938 cites W1970798863 @default.
- W2017265938 cites W1972758675 @default.
- W2017265938 cites W1973767361 @default.
- W2017265938 cites W1974416540 @default.
- W2017265938 cites W1975042776 @default.
- W2017265938 cites W1978466946 @default.
- W2017265938 cites W1979315982 @default.
- W2017265938 cites W1980763523 @default.
- W2017265938 cites W1981189009 @default.
- W2017265938 cites W1982560803 @default.
- W2017265938 cites W1982858374 @default.
- W2017265938 cites W1984910394 @default.
- W2017265938 cites W1985765917 @default.
- W2017265938 cites W1987180280 @default.
- W2017265938 cites W1989010177 @default.
- W2017265938 cites W1989239982 @default.
- W2017265938 cites W1991103499 @default.
- W2017265938 cites W1999348580 @default.
- W2017265938 cites W2000177754 @default.
- W2017265938 cites W2001674813 @default.
- W2017265938 cites W2004169846 @default.
- W2017265938 cites W2005432195 @default.
- W2017265938 cites W2008591861 @default.
- W2017265938 cites W2010211198 @default.
- W2017265938 cites W2010211832 @default.
- W2017265938 cites W2011801766 @default.
- W2017265938 cites W2017288756 @default.
- W2017265938 cites W2017907787 @default.
- W2017265938 cites W2018326531 @default.
- W2017265938 cites W2020980625 @default.
- W2017265938 cites W2021531271 @default.
- W2017265938 cites W2023532632 @default.
- W2017265938 cites W2026979881 @default.
- W2017265938 cites W2027228820 @default.
- W2017265938 cites W2027522276 @default.
- W2017265938 cites W2029180739 @default.
- W2017265938 cites W2030818891 @default.
- W2017265938 cites W2030900564 @default.
- W2017265938 cites W2030996811 @default.
- W2017265938 cites W2031100729 @default.
- W2017265938 cites W2034245229 @default.
- W2017265938 cites W2039422591 @default.
- W2017265938 cites W2040326828 @default.
- W2017265938 cites W2042043581 @default.
- W2017265938 cites W2043916827 @default.
- W2017265938 cites W2047957045 @default.
- W2017265938 cites W2052551486 @default.
- W2017265938 cites W2052581430 @default.
- W2017265938 cites W2052895954 @default.
- W2017265938 cites W2056607398 @default.
- W2017265938 cites W2060003735 @default.
- W2017265938 cites W2064111162 @default.
- W2017265938 cites W2064972995 @default.
- W2017265938 cites W2065862430 @default.
- W2017265938 cites W2066086830 @default.
- W2017265938 cites W2066836395 @default.
- W2017265938 cites W2066933832 @default.
- W2017265938 cites W2068136474 @default.
- W2017265938 cites W2068156942 @default.
- W2017265938 cites W2070220772 @default.
- W2017265938 cites W2070693846 @default.
- W2017265938 cites W2071172756 @default.
- W2017265938 cites W2075585431 @default.
- W2017265938 cites W2076169172 @default.
- W2017265938 cites W2077125391 @default.
- W2017265938 cites W2078585263 @default.
- W2017265938 cites W2078602930 @default.
- W2017265938 cites W2078893670 @default.
- W2017265938 cites W2079758306 @default.
- W2017265938 cites W2082388721 @default.
- W2017265938 cites W2082421959 @default.
- W2017265938 cites W2083558141 @default.
- W2017265938 cites W2086551038 @default.
- W2017265938 cites W2090249305 @default.
- W2017265938 cites W2091031232 @default.
- W2017265938 cites W2091453268 @default.
- W2017265938 cites W2095683741 @default.
- W2017265938 cites W2100634462 @default.
- W2017265938 cites W2100880591 @default.