Behaviour of gold during partial melting of supra subduction zone mantle wedge

Gold-rich magmatic-hydrothermal deposits form in atypical convergent plate-margin tectonic settings conducive to melting lithospheric mantle. Deposits tend to be associated with K 2 O-enriched arc magmas, but ultrapotassic magmas are almost never gold-fertile. Our global compilations of chemical compositions of peridotite xenoliths and of near-primary mafic melts reveal that, during mantle-wedge melting, Au typically has a melt/restite partition coefficient like Yb and Na, much higher than Cu and PGEs. Redox-sensitive element ratios in primitive mafic melts in gold provinces typically indicate ƒO 2 conditions like ordinary arc magmas. Lithophile-element ratios in primitive mafic melts reveal that Au-fertile melts form from garnet-undersaturated, hornblende(±phlogopite)-bearing sources within spinel lherzolite facies, constraining most melting to pressures ≲1.8 GPa and temperatures ≲1100°C, below the solidus of monosulphide solid solution (MSS) of typical mantle composition. Therefore, silicate melts acquire metallogenic fertility primarily by selectively dissolving Au in crystalline MSS. We highlight Au enrichment in lithospheric mantle due to zone refining during orogenic thickening of lithospheric mantle, wherein incompatible-element-rich partial melts are generated by hornblende breakdown at its depth limit and migrate into overlying cooler lithospheric mantle. Fractional crystallisation during ascent of these low-degree melts as hornblende + MSS ± phlogopite-bearing metasomatic veins generates enriched domains within the lithospheric mantle. These low-temperature veins selectively re-melt later upon hydration, decompression, or heating, producing Au-fertile melts in extensional and contractional tectonic settings. Our case studies of gold provinces in rift and orogenic stress settings indicate similar mantle melt compositions but magmatic differentiation trends that diverge according to tectonic stress regime. • Source of Au-fertile melts has ƒO 2 conditions similar to ordinary arc magmas. • Gold behaves as moderately incompatible during mantle-wedge melting. • Gold-fertile magmas derive from hornblende(±phlogopite)-bearing sources. • Silicate melt acquires Au fertility by dissolving crystalline MSS.

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Publication Details

Journal
Earth-Science Reviews
Published
2025-03-27
DOI
https://doi.org/10.1016/j.earscirev.2025.105111
Citations
1
Primary Topic
Geological and Geochemical Analysis
Type
article
Field-Weighted Citation Impact
1.87
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article

Behaviour of gold during partial melting of supra subduction zone mantle wedge

Marco L. Fiorentini, Robert R. Loucks, Carolina Mafra
1 citations
Earth-Science Reviews
Geological and Geochemical Analysis
1.87
article

Behaviour of gold during partial melting of supra subduction zone mantle wedge

Marco L. Fiorentini, Robert R. Loucks, Carolina Mafra
article en
1 citations

Abstract

Gold-rich magmatic-hydrothermal deposits form in atypical convergent plate-margin tectonic settings conducive to melting lithospheric mantle. Deposits tend to be associated with K 2 O-enriched arc magmas, but ultrapotassic magmas are almost never gold-fertile. Our global compilations of chemical compositions of peridotite xenoliths and of near-primary mafic melts reveal that, during mantle-wedge melting, Au typically has a melt/restite partition coefficient like Yb and Na, much higher than Cu and PGEs. Redox-sensitive element ratios in primitive mafic melts in gold provinces typically indicate ƒO 2 conditions like ordinary arc magmas. Lithophile-element ratios in primitive mafic melts reveal that Au-fertile melts form from garnet-undersaturated, hornblende(±phlogopite)-bearing sources within spinel lherzolite facies, constraining most melting to pressures ≲1.8 GPa and temperatures ≲1100°C, below the solidus of monosulphide solid solution (MSS) of typical mantle composition. Therefore, silicate melts acquire metallogenic fertility primarily by selectively dissolving Au in crystalline MSS. We highlight Au enrichment in lithospheric mantle due to zone refining during orogenic thickening of lithospheric mantle, wherein incompatible-element-rich partial melts are generated by hornblende breakdown at its depth limit and migrate into overlying cooler lithospheric mantle. Fractional crystallisation during ascent of these low-degree melts as hornblende + MSS ± phlogopite-bearing metasomatic veins generates enriched domains within the lithospheric mantle. These low-temperature veins selectively re-melt later upon hydration, decompression, or heating, producing Au-fertile melts in extensional and contractional tectonic settings. Our case studies of gold provinces in rift and orogenic stress settings indicate similar mantle melt compositions but magmatic differentiation trends that diverge according to tectonic stress regime. • Source of Au-fertile melts has ƒO 2 conditions similar to ordinary arc magmas. • Gold behaves as moderately incompatible during mantle-wedge melting. • Gold-fertile magmas derive from hornblende(±phlogopite)-bearing sources. • Silicate melt acquires Au fertility by dissolving crystalline MSS.

Earth-Science ReviewsVol. 266
The University of Western Australia (AU), ARC Centre of Excellence in Plant Energy Biology (AU)
Climate action
Openalex Percentile: Top 20%
Geological and Geochemical Analysis
1.87
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