Pyrite-walled tube structures in a Mesoproterozoic sediment-hosted metal sulfide deposit
Abstract
Unusual decimeter-scale structures occur in the sediment-hosted Black Butte Copper Mine Project deposit within lower Mesoproterozoic strata of the Belt Supergroup, Montana. These low domal and stratiform lenses are made up of millimeter-scale, hollow or mineral-filled tubes bounded by pyrite walls. X-ray micro−computed tomography (micro-CT) shows that the tube structures are similar to the porous fabric of modern diffuse hydrothermal vents, and they do not resemble textures associated with the mineralization of known microbial communities. We determined the sulfur isotopic composition of sulfide minerals with in situ secondary ion mass spectrometry (SIMS) and of texture-specific sulfate phases with multicollector−inductively coupled plasma−mass spectrometry (MC-ICP-MS). The sedimentological setting, ore paragenesis, sulfur isotope systematics, and porosity structure of these porous precipitates constrain the site of their formation to above the sediment-water interface where metalliferous hydrothermal fluids vented into the overlying water column. These data constrain the geochemistry of the Mesoproterozoic sediment-water interface and the site of deposition for copper-cobalt-silver mineralization. Metals in the hydrothermal fluids titrated sulfide in seawater to create tortuous fluid-flow conduits. Pyrite that precipitated at the vent sites exhibits large sulfur isotope fractionation (>50‰), which indicates a close association between the vents and sulfate-reducing microbiota. In the subsurface, base metal sulfides precipitated from sulfide formed during the reduction of early diagenetic barite, also ultimately derived from seawater. This model suggests dynamic bottom-water redox conditions at the vent site driven by the interplay between sulfate-reducing organisms and metalliferous fluid effluence.
Additional Information
© 2017 Geological Society of America. Manuscript Received 31 January 2016; Revised Manuscript Received 27 April 2017; Manuscript Accepted 12 July 2017. This project originated during the Agouron Institute Advanced Field Course during July 2013. Funding was provided by the Agouron Institute and the National Aeronautics and Space Administration (NASA) Astrobiology Institute (NAI). We thank Tintina Resources, Inc., especially Chance Matthews, for access to drill core and outcrop associated with the Black Butte Copper Project. We also thank Tyler Mackey, James Wray, Ross Williams, Ken Williford, and Doug Archer for thoughtful discussion and field assistance, and especially Kirsten Siebach for excellent photos. We thank Peter Girguis and Roger Summons for samples of modern hydrothermal vents used in the micro–computed tomography analyses; Jess Adkins, Nathan Dalleska, Yunbin Guan, Jena Johnson, Guillaume Paris, and Jason Price for analytical support; and Michael Russell for help interpreting our data. We thank Peter McGoldrick, Garth Graham, and an additional anonymous reviewer for helpful and thoughtful reviews that greatly improved this submission. We thank the Editors Aaron Cavosie and Fernando Corfu for their help managing and preparing this manuscript.Attached Files
Supplemental Material - 2017303.pdf
Supplemental Material - 2017303_appendix1.xlsx
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Supplemental Material - 2017303_movie-b3.mov
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Supplemental Material - 2017303_movie-m1.mpeg
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Additional details
- Eprint ID
- 82822
- DOI
- 10.1130/B31504.1
- Resolver ID
- CaltechAUTHORS:20171031-151355294
- Agouron Institute
- NASA
- Created
-
2017-10-31Created from EPrint's datestamp field
- Updated
-
2021-11-15Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)