Transgressive nature and chilled margins of the Upper Zone in the western Bushveld Complex, South Africa

S. Chistyakova, R. Latypov, F. Kruger, F. Zaccarini
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引用次数: 3

Abstract

The Upper Zone of the Bushveld Complex has long been known to have formed from a major influx of magma into the chamber that caused large-scale erosion of the chamber floor cumulates. The most dramatic manifestations of this process are two major gap areas (Northern and Southern) in the western Bushveld Complex in which the Upper Zone appears to have eroded away the underlying cumulates down to the very base of the Complex. However, due to almost complete lack of outcrops in the gap areas, no direct field observations have ever been reported to confirm the transgressive nature of the Upper Zone. Here, we present for the first time such observations from the Kameelhoek chromite mine located at the margin of the Northern Gap. In the open pit we have documented several transgressive depressions (up to 40 m in width) in the orthopyroxenite and chromitites of the Lower Critical Zone that are filled in with magnetite gabbro of the Upper Zone. The magnetite gabbro is chilled against the sidewalls of the depressions, forming glassy and fine-grained textured rocks with plagioclase laths arranged in radial clusters. Mineralogically and chemically, the magnetite gabbro correlates with cumulates from the lowermost part of the Upper Zone at its normal position in the complex. Three major points that have emerged from this study are: (1) the Critical Zone has been eroded away by magma that was parental to the Upper Zone, (2) this eroding magma was not the one that initiated formation of the Pyroxenite Marker, but rather the evolved melt that replenished the chamber at some later stage, and (3) the melt was phenocryst-free and likely derived from a deep-seated staging chamber. Our study thus supports a recent notion that even during the formation of the Upper Zone, the Bushveld chamber had still been operating as an open system that was replenished by melts from deeper magma sources.
南非Bushveld复合体西部上部带的海侵性质和冷缘
长期以来,人们一直认为布什维尔德复合体的上部区域是由岩浆大量涌入岩浆室形成的,岩浆涌入岩浆室造成了对岩浆室底部堆积物的大规模侵蚀。这一过程最引人注目的表现是布什维尔德综合体西部的两个主要缺口区(北部和南部),在那里,上部区域似乎已经侵蚀了底层的堆积物,一直到综合体的最底部。然而,由于缺口区几乎完全没有露头,没有直接的实地观察报告证实上带的海侵性质。在这里,我们首次介绍了位于北裂口边缘的Kameelhoek铬铁矿的观测结果。在露天矿中,我们在下临界带的直辉石岩和铬铁矿中记录了几个海侵凹陷(宽度达40米),这些凹陷被上临界带的磁铁矿辉长岩填满。磁铁矿辉长岩在凹陷的侧壁上被冷却,形成玻璃状、细粒的织构岩石,斜长石条呈放射状排列。在矿物学和化学上,该磁铁矿辉长岩在杂岩的正常位置与上带最下部的堆积相对应。本研究得出的三个主要观点是:(1)临界带已经被上带的岩浆侵蚀掉了;(2)这种侵蚀岩浆并不是开始形成辉石岩标志岩的岩浆,而是在后来的某个阶段补充了岩浆室的熔融物;(3)熔融物不含斑晶,可能来自一个深层的阶段室。因此,我们的研究支持了最近的一个观点,即即使在上带形成期间,布什维尔德室仍然作为一个开放的系统运行,由来自更深岩浆源的熔体补充。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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