俄罗斯雅库特乌达奇纳亚管道中橄榄石巨晶镍铜铁硫化物的纳米和微米级PGM

J. González-Jiménez, I. Tretiakova, M. Fiorentini, V. Malkovets, L. Martin, Júlia Farré-de-Pablo
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引用次数: 1

摘要

本文主要研究了一种纳米级和微米级的富含os的矿物颗粒,这些矿物颗粒存在于来自乌达奇纳亚管道(雅库特,俄罗斯)的橄榄石巨晶中发现的Ni-Fe-Cu硫化球中。利用场发射枪电子探针微量分析仪、场发射扫描电镜、聚焦离子束和高分辨率透射电镜等综合技术对这些铂族元素矿物颗粒及其宿主硫化物基质进行了研究。硫化物球是地幔起源的,因为它位于原始橄榄石中(Fo90-93),很可能来自于镍铁铜硫化物熔体的结晶,这些熔体是由枯竭的次大陆岩石圈地幔中玄武岩熔体中的液体不混溶分离出来的。通过场发射扫描电镜和场发射枪电子探针显微分析仪的单点分析和测图发现,硫化物球的核心为磁黄铁矿,其火焰状析出体(通常为1100℃)在<600℃冷却后分解为磁黄铁矿和镍黄铁矿的火焰状析出体。一旦凝固,固态的单硫化物固溶体与非平衡态的富cu和富ni硫化物熔体反应,产生颗粒状的镍黄铁矿,与黄铜矿处于平衡态,形成硫化物球体的边缘。与此同时,纳米到微米级的铁长石晶体在硫化物熔体中直接或稍早于单硫化物固溶体结晶。因此,在高温下形成纳米颗粒而不是低温下从Ni-Fe-Cu固体硫化物中析出,Os以及较小程度上的Ir和Ru被优先吸收而被物理分割。本文提供的新数据表明,为了更好地了解岩浆系统中铂族元素分馏机制,有必要利用纳米级结构特征的分析技术研究Ni-Fe-Cu硫化物中铂族元素矿物颗粒。这些过程可能在控制大范围幔源岩浆中亲铁和亲铜元素的背景地球化学收支中起关键作用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Nano- and Micrometer-Sized PGM in Ni-Cu-Fe Sulfides from an Olivine Megacryst in the Udachnaya Pipe, Yakutia, Russia
This paper focuses on a nanoscale study of nano- and micrometer-size Os-rich mineral particles hosted in a Ni-Fe-Cu sulfide globule found in an olivine megacryst from the Udachnaya pipe (Yakutia, Russia). These platinum-group element mineral particles and their host sulfide matrices were investigated using a combination of techniques, including field emission gun electron probe microanalyzer, field emission scanning electron microscopy, and focused ion beam and high-resolution transmission electron microscopy. The sulfide globule is of mantle origin, as it is hosted in primitive olivine (Fo90–93), very likely derived from the crystallization of Ni-Fe-Cu sulfide melt droplets segregated by liquid immiscibility from a basaltic melt in a volume of depleted subcontinental lithospheric mantle. Microscopic observations by means of field emission scanning electron microscopy and single-spot analysis and mapping by field emission gun electron probe microanalyzer reveal that the sulfide globule comprises a core of pyrrhotite with flame-like exsolutions (usually <10 μm thickness) of pentlandite, which is irregularly surrounded by a rim of granular pentlandite and chalcopyrite. Elemental mapping by energy dispersive spectroscopy (acquired using the high-resolution transmission electron microscopy) of the pyrrhotite (+ pentlandite) core reveals that pentlandite exsolution in pyrrhotite is still observable at the nanoscale as fringes of 100 to 500 nm thicknesses. The sulfide matrices of pyrrhotite, pentlandite, and chalcopyrite contain abundant nano- and micrometer-size platinum group element mineral particles. A careful inspection of eight of these platinum group element particles under focused ion beam and high-resolution transmission electron microscopy showed that they are crystalline erlichmanite (OsS2) with well-developed crystal faces that are distinctively oriented relative to their sulfide host matrices. We propose that the core of the Ni-Fe-Cu sulfide globule studied here was derived from a precursor monosulfide solid solution originally crystallized from a sulfide melt at >1100 °C, which later decomposed into pyrrhotite and the pentlandite flame-like exsolutions upon cooling at <600 °C. Once solidified, the solid monosulfide solid solution reacted with non-equilibrium Cu-and Ni-rich sulfide melt(s), giving rise to the granular pentlandite in equilibrium with chalcopyrite now forming the rim of the sulfide globule. Meanwhile, nano- to micron-sized crystals of erlichmanite crystallized directly from or slightly before monosulfide solid solution from the sulfide melt. Thus, Os, and to a lesser extent Ir and Ru, were physically partitioned by preferential uptake via early formation of nanoparticles at high temperature instead of low-temperature exsolution from solid Ni-Fe-Cu sulfides. The new data provided in this paper highlight the necessity of studying platinum group element mineral particles in Ni-Fe-Cu sulfides using analytical techniques that can image nanoscale textural features in order to better understand the mechanisms of platinum group element fractionation in magmatic systems. These processes may play a crucial role in controlling the background geochemical budgets for siderophile and chalcophile elements in a wide range of mantle-derived magmas.
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