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Extremely negative and inhomogeneous sulfur isotope signatures in Cretaceous Chilean manto-type Cu–(Ag) deposits, Coastal Range of central Chile

Extremely negative and inhomogeneous sulfur isotope signatures in Cretaceous Chilean manto-type Cu–(Ag) deposits, Coastal Range of central Chile
Extremely negative and inhomogeneous sulfur isotope signatures in Cretaceous Chilean manto-type Cu–(Ag) deposits, Coastal Range of central Chile
Chilean manto-type (CMT) Cu(–Ag) hydrothermal deposits share a characteristic association of volcano-sedimentary Jurassic to Lower Cretaceous host rocks, style of mineralization, ore and associated mineralogy and geochemistry, with ore grades typically > 1%Cu, that make this family of deposits significant and interesting, both academically and economically. Although often stratabound, geological evidence supports an epigenetic origin for these deposits. We present a detailed stable isotope study of La Serena and Melipilla–Naltahua Lower Cretaceous deposits, central Chile, which reveals extremely negative ?34S values, to ? 50‰, which are among the lowest values found in any ore deposit. In addition, the range of ?34S values from sulfides in the two areas is very wide: ? 38.3 to ? 6.9‰ in La Serena, and ? 50.4 to ? 0.6‰ in Melipilla–Naltahua. These new data significantly extended the reported range of ?34S data for CMT deposits. Co-existing sulfates range from 7.9 to 14.3‰, and are exclusive to La Serena deposit. The wide sulfide isotopic range occurs at deposit and hand specimen scale, and suggests a polygenic sulfur source for these deposits, where bacteriogenic sulfide dominates. While sulfur isotope data for the bulk of Jurassic CMT deposits, northern Chile, suggests a predominant magmatic source in their origin (mean = ? 2.7 ± 1.9‰, 1?), contributions of a magmatic component is only likely to be involved at Melipilla–Naltahua deposit.

The ?13C values obtained for calcites associated with the mineralization range from ? 20.1 to 0.2‰ also suggesting polygenic carbon sources, with the likely strong involvement of degradation of organic matter and leaching of limestone.

Two different genetic models, with involvement of hydrocarbon, are proposed for both areas. For Melipilla–Naltahua, a two-step model can be developed as follows: 1) Framboidal pyrite growth, with very low ?34S, formed by bacterial sulfate reduction in an open system, and with diagenetic degradation of oil-related brines, leaving pyrobitumen. 2) Cu-bearing stage, replacing of framboidal pyrite, inheriting depleted sulfur as low as ? 50.4‰, together with sulfides directly precipitated from a hydrothermal fluid with ?34S close to 0‰. For La Serena, a single step model fits best, without framboidal pyrite generation. Cu-bearing sulfides were precipitated mainly in veins where Cu plus base metal-bearing hydrothermal fluids mixed with H2S generated by bacterial sulfate reduction in the host rocks. Isotopic evidence clearly illustrates that bacterial activity, perhaps enhanced by hydrothermal activity, was fed by hydrocarbon brines and sulfate remobilized from continental evaporites. It is possible that variable ecological conditions led to different extents of isotopic fractionation, adding to the typical sulfur isotopic heterogeneity of such bacterial systems. For both areas, the Cu-bearing stage occurred during the peak to waning stages of the very low-grade metamorphism that affected the Lower Cretaceous sequence.
0169-1368
13-24
Carrillo-Rosúa, Javier
48d97ee6-8bb3-4438-ab82-3f6848f62f64
Boyce, Adrian J.
e21e60d3-a9ab-4cad-9bd8-f6680f3dbd7f
Morales-Ruano, Salvador
a9abf360-3323-43c7-9e6f-113013d984e5
Morata, Diego
0df55169-f581-4227-8b1e-9cad03047e46
Roberts, Stephen
f095c7ab-a37b-4064-8a41-ae4820832856
Munizaga, Francisco
a3b12436-5bb0-4780-ac86-10a01eaaa323
Moreno-Rodríguez, Verónica
c5be940e-3826-4a61-8306-115ec656cc82
Carrillo-Rosúa, Javier
48d97ee6-8bb3-4438-ab82-3f6848f62f64
Boyce, Adrian J.
e21e60d3-a9ab-4cad-9bd8-f6680f3dbd7f
Morales-Ruano, Salvador
a9abf360-3323-43c7-9e6f-113013d984e5
Morata, Diego
0df55169-f581-4227-8b1e-9cad03047e46
Roberts, Stephen
f095c7ab-a37b-4064-8a41-ae4820832856
Munizaga, Francisco
a3b12436-5bb0-4780-ac86-10a01eaaa323
Moreno-Rodríguez, Verónica
c5be940e-3826-4a61-8306-115ec656cc82

Carrillo-Rosúa, Javier, Boyce, Adrian J., Morales-Ruano, Salvador, Morata, Diego, Roberts, Stephen, Munizaga, Francisco and Moreno-Rodríguez, Verónica (2014) Extremely negative and inhomogeneous sulfur isotope signatures in Cretaceous Chilean manto-type Cu–(Ag) deposits, Coastal Range of central Chile. Ore Geology Reviews, 56, 13-24. (doi:10.1016/j.oregeorev.2013.06.013).

Record type: Article

Abstract

Chilean manto-type (CMT) Cu(–Ag) hydrothermal deposits share a characteristic association of volcano-sedimentary Jurassic to Lower Cretaceous host rocks, style of mineralization, ore and associated mineralogy and geochemistry, with ore grades typically > 1%Cu, that make this family of deposits significant and interesting, both academically and economically. Although often stratabound, geological evidence supports an epigenetic origin for these deposits. We present a detailed stable isotope study of La Serena and Melipilla–Naltahua Lower Cretaceous deposits, central Chile, which reveals extremely negative ?34S values, to ? 50‰, which are among the lowest values found in any ore deposit. In addition, the range of ?34S values from sulfides in the two areas is very wide: ? 38.3 to ? 6.9‰ in La Serena, and ? 50.4 to ? 0.6‰ in Melipilla–Naltahua. These new data significantly extended the reported range of ?34S data for CMT deposits. Co-existing sulfates range from 7.9 to 14.3‰, and are exclusive to La Serena deposit. The wide sulfide isotopic range occurs at deposit and hand specimen scale, and suggests a polygenic sulfur source for these deposits, where bacteriogenic sulfide dominates. While sulfur isotope data for the bulk of Jurassic CMT deposits, northern Chile, suggests a predominant magmatic source in their origin (mean = ? 2.7 ± 1.9‰, 1?), contributions of a magmatic component is only likely to be involved at Melipilla–Naltahua deposit.

The ?13C values obtained for calcites associated with the mineralization range from ? 20.1 to 0.2‰ also suggesting polygenic carbon sources, with the likely strong involvement of degradation of organic matter and leaching of limestone.

Two different genetic models, with involvement of hydrocarbon, are proposed for both areas. For Melipilla–Naltahua, a two-step model can be developed as follows: 1) Framboidal pyrite growth, with very low ?34S, formed by bacterial sulfate reduction in an open system, and with diagenetic degradation of oil-related brines, leaving pyrobitumen. 2) Cu-bearing stage, replacing of framboidal pyrite, inheriting depleted sulfur as low as ? 50.4‰, together with sulfides directly precipitated from a hydrothermal fluid with ?34S close to 0‰. For La Serena, a single step model fits best, without framboidal pyrite generation. Cu-bearing sulfides were precipitated mainly in veins where Cu plus base metal-bearing hydrothermal fluids mixed with H2S generated by bacterial sulfate reduction in the host rocks. Isotopic evidence clearly illustrates that bacterial activity, perhaps enhanced by hydrothermal activity, was fed by hydrocarbon brines and sulfate remobilized from continental evaporites. It is possible that variable ecological conditions led to different extents of isotopic fractionation, adding to the typical sulfur isotopic heterogeneity of such bacterial systems. For both areas, the Cu-bearing stage occurred during the peak to waning stages of the very low-grade metamorphism that affected the Lower Cretaceous sequence.

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Published date: January 2014
Organisations: Geochemistry

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Local EPrints ID: 361810
URI: http://eprints.soton.ac.uk/id/eprint/361810
ISSN: 0169-1368
PURE UUID: 26faae9e-166b-4ba7-bd3d-9e8b1a79a64e
ORCID for Stephen Roberts: ORCID iD orcid.org/0000-0003-4755-6703

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Date deposited: 03 Feb 2014 14:57
Last modified: 15 Mar 2024 02:39

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Contributors

Author: Javier Carrillo-Rosúa
Author: Adrian J. Boyce
Author: Salvador Morales-Ruano
Author: Diego Morata
Author: Stephen Roberts ORCID iD
Author: Francisco Munizaga
Author: Verónica Moreno-Rodríguez

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