Polymetallic Te-rich melts contribute to efficient enrichment and precipitation of Au in hydrothermal ore deposits

IF 4.5 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Gao-Hua Fan , Jian-Wei Li , Ri-Chen Zhong , Sarah A. Gleeson , Zhuo-Sen Yao , Daniel E. Harlov , Xiao-Dong Deng , Hao Cui , Chang Yu , Wen-Sheng Gao
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Abstract

Tellurides are abundant in a large variety of hydrothermal Au deposits. Previous studies have proposed that these phases crystallize from polymetallic Te-rich melts that may act as scavengers for Au to form high grade deposits. However, the conditions under which Te-rich melts form and whether such melts can act as agents to concentrate Au have not been directly assessed. Here, we present an experimental study using natural ore samples from a giant Te-rich Au deposit (Dongping, China) to show that tellurides in Au ores crystallized from polymetallic melts and these melts behaved as a critical agent for Au enrichment and precipitation. The samples investigated contain abundant polymetallic inclusions, which consist of various telluride-gold mineral assemblages as well as minor chalcopyrite. Individual inclusions typically comprise one micron-sized gold grain. Annealing experiments of these inclusions were carried out at 300, 350, 400, and 450 °C. The polymetallic inclusions had relatively subtle changes in morphology and texture at 300 and 350 °C, but changed markedly at 400 and 450 °C, accompanying with the formation of abundant droplet-like and/or vermiculate gold grains randomly dispersed in the telluride matrix. Three in-situ scanning electron microscopy heating–cooling experiments with different heating rates and durations revealed a eutectic temperature of 243 to 270 °C for polymetallic tellurides, at which native gold began to dissolve into molten tellurides. During the heating processes of the three experimental runs, changes in topographic contrast occurred, with the formation of transient holes in the tellurides and the appearance of tellurides on the surface of chalcopyrite. These observations are indicative of localized migration of the molten tellurides. Upon cooling in run #1 and #2, native gold recrystallized at ∼ 340 °C from the molten tellurides and subsequently regrew in a gradual manner. After these two runs, many newly-formed telluride-gold globules were observed occurring as fracture- and/or cavity-infillings within the host pyrite, further confirming molten state of the polymetallic minerals. Collectively, our new data demonstrate that polymetallic Te-rich melts with a complete melting temperature of ∼ 340 to 400 °C are responsible for the formation of telluride-gold mineral assemblages in natural Te-rich Au ores. Such melts can act as an important Au scavenger and facilitate Au precipitation. Our findings highlight the significance of polymetallic Te-rich melts as a key agent for concentrating Au to form high-grade Au ores worldwide.
多金属富te熔体有助于热液矿床中金的高效富集和沉淀
碲化物在种类繁多的热液型金矿床中含量丰富。以前的研究已经提出,这些相从多金属富te熔体中结晶,可能作为Au的清除剂形成高品位矿床。然而,富te熔体形成的条件以及这些熔体是否可以作为富集Au的助剂还没有得到直接的评估。在此,我们提出了一项实验研究,利用来自中国东平一个巨型富te金矿床的天然矿石样本,表明金矿中的碲化物是从多金属熔体中结晶出来的,这些熔体是Au富集和沉淀的关键因素。样品中含有丰富的多金属包裹体,由多种碲金矿组合和少量黄铜矿组成。单个内含物通常包含一微米大小的金颗粒。分别在300、350、400和450℃下对这些夹杂物进行了退火实验。在300和350℃时,多金属夹杂物的形貌和织构变化相对较小,而在400和450℃时变化明显,并伴有大量的液滴状和(或)蛭状金颗粒随机分散在碲化物基体中。三次不同加热速率和加热时间的原位扫描电镜加热-冷却实验表明,多金属碲化物的共晶温度为243 ~ 270℃,此时天然金开始溶解于熔融碲化物中。在三次实验的加热过程中,地形对比发生了变化,碲化物中形成了瞬态孔洞,黄铜矿表面出现了碲化物。这些观测结果表明熔融碲化物的局部迁移。在运行#1和#2冷却后,天然金在~ 340°C从熔融碲化物中再结晶,随后以逐渐的方式重新生长。在这两次运行后,观察到许多新形成的碲金球状体在宿主黄铁矿中以裂隙和/或空腔充填的形式出现,进一步证实了多金属矿物的熔融状态。总的来说,我们的新数据表明,在完全熔融温度为~ 340至400°C的多金属富te熔体是在天然富te金矿中形成碲-金矿矿物组合的原因。这种熔体可以作为重要的金清除剂,促进金的析出。我们的发现突出了多金属富te熔体作为富集Au形成高品位金矿的关键因素的重要性。
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来源期刊
Geochimica et Cosmochimica Acta
Geochimica et Cosmochimica Acta 地学-地球化学与地球物理
CiteScore
9.60
自引率
14.00%
发文量
437
审稿时长
6 months
期刊介绍: Geochimica et Cosmochimica Acta publishes research papers in a wide range of subjects in terrestrial geochemistry, meteoritics, and planetary geochemistry. The scope of the journal includes: 1). Physical chemistry of gases, aqueous solutions, glasses, and crystalline solids 2). Igneous and metamorphic petrology 3). Chemical processes in the atmosphere, hydrosphere, biosphere, and lithosphere of the Earth 4). Organic geochemistry 5). Isotope geochemistry 6). Meteoritics and meteorite impacts 7). Lunar science; and 8). Planetary geochemistry.
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