PGE distribution in Merensky wide-reef facies of the Bushveld Complex, South Africa: Evidence for localized hydromagmatic control

S. Prevec, Savvas Anthony Largatzis, W. Brownscombe, T. Salge
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Abstract

The wide-reef facies of the Merensky Reef in the eastern part of the western lobe of the Bushveld Complex was sampled in order to better resolve otherwise spatially constrained variation in highly siderophile elements across this geological unit. The platinum group element mineralogy and whole-rock highly siderophile element concentrations were measured across two vertical sections in close proximity. In one section, the Merensky Reef unit was bound by top and bottom platinum group elements-enriched horizons (reefs) with a well-developed pegmatoidal phase in the top third of the intrareef pyroxenite, but with neither a top nor a bottom chromitite present. The other drill core section featured a thin (<1 cm thick) chromitite layer associated with the highest platinum group element concentrations of any rock in this study as the bottom reef, but with a chromitite-absent top reef, and very poor development of the pegmatoid. Primitive mantle-normalized profiles of the main lithological units show relatively flat, primitive mantle-like highly siderophile element abundances (Cr, V, Co, Ni, platinum group elements, Au and Cu) in the Merensky pyroxenite, with modest depletion in Ir-affiliated platinum group elements. The platinum group element-rich top and bottom reefs, and the pegmatoidal upper pyroxenites, display characteristic enrichment in the Pt-affiliated platinum group elements and undepleted Ir-affiliated platinum group elements. The leuconoritic hanging wall and footwall rocks show comparable highly siderophile element profiles, distinguished from one another by relative depletion in the Pt-affiliated platinum group elements of the footwall samples. The vertical variation in highly siderophile element abundances through both sections is characterized by low platinum group element abundances through the lower reef pyroxenite, with platinum group element, Au, and Cu ± Ni concentrations increasing through the upper pegmatoidal pyroxenite, and main enrichment peaks at the top and bottom reefs. Significant localized (centimeter-scale) zones of chalcophile metal depletion are present immediately above the top reef and below the bottom reef. In addition, a wider zone of Pt-affiliated platinum group elements (with Pd more depleted than Pt)-depletion was identified within the pegmatoidal pyroxenite around one meter below the top reef. The platinum group element mineralogy of the bottom reef consists mainly of platinum group element sulfides, with minor arsenides and antimonides. In contrast, the platinum group element mineralogy of the top reef, and the small amount of data from the intrareef pyroxenite, mainly consist of Pt-affiliated platinum group elements-Bi-tellurides. The Pt-sulfides are mainly equant, relatively coarse crystals (many grains between 50 to 100 μm2 area), contrasting with the Pt-affiliated platinum group elements-Sb-As and -Bi-Te minerals that tend be high aspect-ratio grains, occurring in veinlets or as rims on earlier-forming platinum group element phases. These Te-As-Bi-Sb compounds are closely associated with chlorite, actinolite, quartz, and chalcopyrite, consistent with secondary deposition at lower temperatures and association with aqueous fluids. A model is proposed involving the emplacement of the Merensky unit as a magma pulse into at least semi-crystallized host rock, followed by aqueous fluid saturation and local migration, combined with concentration of late magmatic fluids around the top and bottom contacts of the magma pulse. Late remobilization of Pt-affiliated platinum group elements from the zones immediately (centimeter-scale) above the top reef, and from the underlying meter or two of pyroxenite, and from the centimeters underlying the bottom reef, have added additional platinum group elements to the reefs as late platinum group elements-Te-As-Bi-Sb minerals, independent of whether or not chromite is present in the reef initially.
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南非Bushveld杂岩Merensky宽礁相PGE分布:局部岩浆流体控制的证据
对Bushveld杂岩西叶东部的Merensky礁的宽礁相进行了采样,以便更好地解决该地质单元中高亲铁元素的空间限制变化。铂族元素矿物学和全岩高亲铁元素浓度在两个接近的垂直剖面上进行了测量。在一个剖面上,梅伦斯基礁单元被顶部和底部富铂族元素的层位(礁)所约束,在礁内辉石岩的顶部三分之一处有发育良好的伟晶岩相,但顶部和底部都没有铬铁矿。另一钻孔岩心剖面的底礁为薄(<1 cm厚)的铬铁矿层,其铂族元素浓度是本研究中所有岩石中最高的,但顶礁没有铬铁矿,类伟晶岩发育非常差。主要岩性单元的原始地幔归一化剖面显示,梅伦斯基辉石岩中亲铁元素(Cr、V、Co、Ni、铂族元素、Au和Cu)丰度相对平坦,呈原始地幔状,与ir相关的铂族元素有一定的亏缺。富铂族元素的顶、底礁和伟晶状上辉石岩均具有铂族元素富集和未亏缺铂族元素富集的特征。上盘和下盘白斑岩均表现出相当高的亲铁元素特征,其区别在于下盘样品中铂族元素的相对贫化。高亲铁元素丰度的垂直变化特征为:铂族元素丰度在礁体下部辉石岩中呈低丰度,铂族元素、Au和Cu±Ni浓度在礁体上部辉石岩中呈上升趋势,富集峰主要在礁体顶部和底部。显著的局部(厘米尺度)亲铜金属耗损区出现在顶部礁的正上方和底部礁的下方。此外,在顶部礁体下方约一米的伟晶状辉石岩中发现了一个更广泛的铂族元素(Pd比Pt更贫)耗损区。底礁铂族元素矿物学以铂族元素硫化物为主,含少量砷化物和锑化物。顶部礁体的铂族元素矿物学特征,以及礁内辉石岩的少量资料,主要由铂族元素-铋碲化物组成。与铂族元素sb - as和-Bi-Te等矿物相比,铂族元素硫化物主要为均匀、较粗的晶体(许多颗粒面积在50 ~ 100 μm2之间),而铂族元素的铂族元素sb - as和bi - te矿物则倾向于高纵横比的颗粒,在早期形成的铂族元素相中呈细脉状或呈边缘状。这些Te-As-Bi-Sb化合物与绿泥石、放线石、石英和黄铜矿密切相关,与低温下的二次沉积和与水相结合一致。提出了Merensky单元作为岩浆脉冲侵入至少半结晶的寄主岩石的模型,随后是含水流体饱和和局部迁移,并结合岩浆脉冲顶部和底部接触处晚期岩浆流体的浓度。铂系铂族元素从顶部礁上方(厘米尺度)、从下垫1 - 2米的辉石岩以及从底部礁下垫数厘米的铂族元素晚期再活化,为礁体添加了额外的铂族元素,即晚期铂族元素- te - as - bi - sb矿物,而与最初礁体中是否存在铬铁矿无关。
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