南非巴伯顿绿岩带北部Fairview金矿早期太古代撞击球粒层的地球和地外化学成分

G. J. Oliveira, W. Reimold, A. Crósta, N. Hauser, C. Koeberl, D. Mader, R. Schmitt, T. Mohr‐Westheide
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引用次数: 1

摘要

从南非巴伯顿绿岩带的几个地层水平上描述了被广泛接受的代表地球早期大规模撞击事件的远端喷出物沉积物的早期太古代球体层。最近,在带北域Fairview金矿(25°43′53″S, 31°5′59″E)的勘探钻探中,发现了一组新的球粒层相交。BH5901、BH5907、BH5911和BH5949岩心中的Fairview球粒层在Onverwacht组向Fig Tree组过渡的同一地层位置相交,间距仅为几米。Fairview的球粒层在岩石学和化学上至少与其他三个著名的Barberton球粒层(S2-S4)相似,并且在钻芯BARB5和CT3中有多个球粒层床相交,它们都来自大致相同的地层位置。它们的组成不均匀,特别是在高亲铁元素的丰度方面。中等(Cr, Co, Ni)和高亲铁性(Ir)元素的最高浓度在球粒陨石的浓度范围内,因此,加强了Fairview球粒层形成的撞击假设。钻芯BH5907、BH5911和BH5949球粒层样品的铱峰值浓度和Cr/Ir元素间比值表明,球粒物质的掺量为50% ~ 60%,而BH5901球粒层样品的掺量仅为1%。我们讨论了这四个Fairview球体层是否代表相同的撞击事件,以及它们是否可以与任何S2-S4, CT3和BARB5交叉点相关。
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Terrestrial and extraterrestrial chemical components of early Archean impact spherule layers from Fairview Gold Mine, northern Barberton greenstone belt, South Africa
Early Archean spherule layers, widely accepted to represent distal ejecta deposits from large-scale impact events onto the early Earth, have been described from several stratigraphic levels of the Barberton greenstone belt in South Africa. Recently, exploration drilling at the Fairview Gold Mine (25°43′53″S, 31°5′59″E) in the northern domain of the belt resulted in the discovery of a new set of spherule layer intersections. The Fairview spherule layers in drill cores BH5901, BH5907, BH5911, and BH5949 were intersected just a few meters apart, at about the same stratigraphic position within the transition from the Onverwacht Group to the Fig Tree Group. The Fairview spherule layers have petrographic and chemical similarities to at least three other well-known Barberton spherule layers (S2–S4), and multiple spherule layer bed intersections in drill cores BARB5 and CT3, all from about the same stratigraphic position. They are not uniform in composition, in particular with respect to abundances of highly siderophile elements. The highest concentrations of moderately (Cr, Co, Ni) and highly siderophile (Ir) elements are within the range of concentrations for chondrites and, thus, reinforce the impact hypothesis for the generation of the Fairview spherule layers. Iridium peak concentrations and Cr/Ir interelement ratios for spherule layer samples from drill cores BH5907, BH5911, and BH5949 suggest admixtures of 50%–60% chondritic material, whereas for the BH5901 spherule layer, only an admixture of 1% chondritic material is indicated. We discuss whether these four Fairview spherule layers represent the same impact event, and whether they can be correlated to any of the S2–S4, CT3, and BARB5 intersections.
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