EGU26-9932, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-9932
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Thursday, 07 May, 16:15–18:00 (CEST), Display time Thursday, 07 May, 14:00–18:00
 
Hall X2, X2.43
What do Re-Os ages of sulfide minerals at amphibolite facies mean: resolving syngenetic vs metamorphic ages in an Archean VMS deposit
Cendi Dana1, Steven Hollis1, Lorenzo Tavazzani2, Cyril Chelle-Michou2, Stijn Glorie3, Yusuke Kuwahara4, Kazuhide Mimura4, Moei Yano4, Junichiro Ohta4, David Selby5, Yasuhiro Kato4, Vanessa Pashley6, Megan James7, and Darryl Podmore7
Cendi Dana et al.
  • 1University of Edinburgh, Earth and Planetary Institute, School of Geosciences, Edinburgh, United Kingdom of Great Britain – England, Scotland, Wales (c.d.p.dana@sms.ed.ac.uk)
  • 2Department of Earth and Planetary Sciences, ETH Zurich, Zurich 8092, Switzerland
  • 3Department of Earth Sciences, University of Adelaide, South Australia 5005, Australia
  • 4Ocean Resources Research Center for Next Generation, Chiba Institute of Technology, Chiba 275-0016, Japan
  • 5Department of Earth Sciences, University of Durham, Durham DH1 3LE, United Kingdom
  • 6Geochronology and Tracers Facility, British Geological Survey, Nottingham NG12 5GG, United Kingdom
  • 7Black Raven Mining, PO Box 261, North Perth, Western Australia 6872, Australia

Establishing the age of mineral deposits and their host rock sequences is fundamental to mineral exploration, as it constrains the temporal evolution of prospective geological environments and the geodynamic processes responsible for ore formation. This is particularly critical for syn-genetic stratiform systems such as volcanogenic massive sulfide (VMS) deposits, which are typically localized along favorable stratigraphic horizons within volcanic belts and linked to episodes of regional extension and magmatism. In Archean cratons, however, VMS deposits commonly experience multiple post-ore deformation, metamorphic, and hydrothermal events that may obscure primary isotopic signatures and result in metal remobilization, complicating efforts to constrain the timing of syn-genetic mineralization.

In this study, we apply an integrated geochronological approach including U–Pb zircon and titanite, Lu–Hf garnet, Re–Os sulfide and molybdenite, and Pb–Pb galena dating to constrain the age of syn-genetic mineralization in an Archean VMS deposit metamorphosed to amphibolite facies. Our results demonstrate that the Re–Os isotopic system in syn-genetic pyrite can be preserved through high-grade metamorphism and yields ages consistent with U–Pb zircon ages of the felsic host rocks, providing a robust means to directly date VMS mineralization in highly metamorphosed Archean terranes. In contrast, Re–Os ages obtained from pyrrhotite record prograde metamorphism and align with Lu–Hf garnet ages, indicating their utility for constraining metamorphic overprinting and metal remobilization events.

We further show that Re–Os dating of bulk massive sulfide ore dominated by both pyrite and pyrrhotite produces mixed, geologically meaningless ages, rendering this approach unreliable where extensive pyrrhotite formation has occurred via pyrite desulfidation. Although molybdenite within the footwall stratigraphy yields robust Re–Os ages despite amphibolite-facies metamorphism, these ages reflect late granitoid emplacement and regional metamorphism rather than syn-genetic VMS mineralization. Collectively, our findings provide new constraints on the timing of metamorphosed VMS deposits and have significant implications for regional exploration strategies, particularly within the Yilgarn Craton.

How to cite: Dana, C., Hollis, S., Tavazzani, L., Chelle-Michou, C., Glorie, S., Kuwahara, Y., Mimura, K., Yano, M., Ohta, J., Selby, D., Kato, Y., Pashley, V., James, M., and Podmore, D.: What do Re-Os ages of sulfide minerals at amphibolite facies mean: resolving syngenetic vs metamorphic ages in an Archean VMS deposit, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-9932, https://doi.org/10.5194/egusphere-egu26-9932, 2026.