Hydrothermal alteration at the Magdala gold deposit, Stawell, western Victoria

Abstract

The Magdala deposit in the Stawell goldfield in western Victoria was formed during the 440 Ma gold event of the Lachlan Orogeny and is hosted by Cambrian quartz-rich turbiditic sedimentary rocks (Albion Formation) that onlap a thick pile of tholeiitic basaltic lavas (Magdala Basalt). Detailed petrographic and geochemical analyses suggest that the host-rock (Stawell Facies) was originally a turbiditic sedimentary rock that was hydrothermally altered in response to seawater interaction with the hot basaltic pile. Subsequent regional greenschist metamorphism and ductile deformation that lasted at least 10 million years culminated in the formation of the Magdala mineralised system and produced a complex pattern of hydrothermal alteration. Evolution of this alteration occurred over six stages: Stage 1, Fe-enrichment of sedimentary rock adjacent to the basalt pre-D₁; Stage 2, chlorite (metamorphism), orbicular carbonate and pyrite, syn-D₂; Stage 3, muscovite, siderite, ankerite and pyrrhotite, syn-D₃ – D_4a – b; Stage 4, stilpnomelane, siderite, pyrrhotite, arsenopyrite and pyrite, syn-D_4c; Stage 5, silica, minnesotaite and magnetite, post-D_4c – pre-D₅; and Stage 6, Fe-rich chlorite, muscovite, calcite, arsenopyrite and pyrite, syn-D₅. Comparisons with other turbidite-hosted gold deposits in Victoria (e.g. Bendigo and Ballarat) highlight four major differences: (i) presence of a tholeiitic basaltic pile; (ii) ductile deformation (D_1 – 4) over at least 60 million years prior to gold mineralisation; (iii) highly evolved hydrothermal alteration; and (iv) source of sulfur. Of these differences the key element is the basaltic pile and its associated heat, which may have promoted the growth of micro-organisms in, and alteration of, the onlapping sedimentary rocks, thereby creating a basis from which an unusual turbidite-hosted orogenic-gold deposit was formed.

Key words:

• alteration
• Cambrian
• Lachlan Orogen
• orogenic gold
• Stawell

Acknowledgements

This project was funded through Australian Research Council Linkage Grant and Mining Project Investors Ltd (MPI). We wish to thank MPI for allowing the publication of this paper and for their technical support throughout this project. In particular, we thank J. Dugdale, G. McDermott, S. Melee, K. Hutchinson and B. Godsmark for all their help. Neil Phillips and Richard White are also thanked for making constructive comments on the manuscript.

Notes

*Appendices 1 –  3[indicated by an asterisk (*) in the text and listed at the end of the paper] are Supplementary Papers; copies may be obtained from the Geological Society of Australia's website (www.gsa.org.au) or from the National Library of Australia's Pandora archive (http://nla.gov.au/nla.arc-25194).