2012
DOI: 10.1007/s00126-012-0402-y
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A unified model for gold mineralisation in accretionary orogens and implications for regional-scale exploration targeting methods

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Cited by 272 publications
(96 citation statements)
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References 112 publications
(141 reference statements)
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“…This relationship is due to a number of factors: (1) The addition of juvenile material into the crust before the initiation of a gold-forming event is critical to developing gold fertility Bateman & Bierlein 2007, Hronsky et al 2012. This can happen at anytime before gold mineralization, and suggests that the fertility of the Southern Cross and Murchison gold sources developed 350 -150 myr before the gold mineralizing event at c. 2650-2630 Ma, as this is when juvenile material was added to the crust, creating a fertile source.…”
Section: Orogenic Goldmentioning
confidence: 99%
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“…This relationship is due to a number of factors: (1) The addition of juvenile material into the crust before the initiation of a gold-forming event is critical to developing gold fertility Bateman & Bierlein 2007, Hronsky et al 2012. This can happen at anytime before gold mineralization, and suggests that the fertility of the Southern Cross and Murchison gold sources developed 350 -150 myr before the gold mineralizing event at c. 2650-2630 Ma, as this is when juvenile material was added to the crust, creating a fertile source.…”
Section: Orogenic Goldmentioning
confidence: 99%
“…(3) The 'Mafic' group of granites (sanukitoids; Cassidy et al 2002) are associated with juvenile crust and appear to be an important factor in gold mineralization (Cassidy et al 1998(Cassidy et al , 2002. These granites are relatively high in Ni, Cr and Mg# as well as large ion lithophile elements (Ba, Sr, light REE; Champion & Sheraton 1997) and such alkalic mafic magmas may have represented an important gold source (Wyman & Kerrich 1988;Müller 2002;Hronsky et al 2012;Duuring et al 2007). The Mafic granites utilized the same structures as gold and were emplaced at the start of the gold event at c. 2650 Ma (Cassidy et al 2002).…”
Section: Orogenic Goldmentioning
confidence: 99%
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“…The most favoured candidate fluid sources are: 1) metamorphic devolatilisation (Kerrich and Wyman, 1990;Goldfarb et al, 1991;Phillips, 1993;McCuaig and Kerrich, 1998;Yardley and Cleverly, 2013); and 2) hydrothermal fluids exsolved from crystallising magmas (de Ronde et al, 2000;Lawrence et al, 2013a;Lawrence et al, 2013b;Treloar et al, 2014). However, alternate sources have been suggested, including, deeply convecting meteoric water (Hagemann et al, 1994;Jenkin et al, 1994), mantlesourced fluids (Cameron, 1988;Hronsky et al, 2012), or fluids expelled from subducting oceanic crust (Breeding and Ague, 2002). In general, candidate sources of Au share similarities with those of fluids.…”
Section: Introductionmentioning
confidence: 99%
“…Such timeframes are linked to the very localised nature, both spatially and temporally, of the controlling mechanisms involved. Fluids and mineralisation processes have been conceptionally pictured as "inverted lightning rods" from depth (Hronsky, et al, 2012) . Episodic fault slip events (Cox, 2016) involving highly-pressurized fluids (Sibson, et al, 1988) have been invoked.…”
Section: Introductionmentioning
confidence: 99%