首页> 外文期刊>Journal of geophysical research. Solid earth: JGR >Geochemistry of the impact‐generated melt sheet at Manicouagan: Evidence for fractional crystallization
【24h】

Geochemistry of the impact‐generated melt sheet at Manicouagan: Evidence for fractional crystallization

机译:曼尼科阿根(Manicouagan)碰撞产生的熔体片的地球化学:分步结晶的证据

获取原文
获取原文并翻译 | 示例
           

摘要

Recent exploration drilling of the Manicouagan impact structure has revealed local developments of impact melt that are substantially thicker than the previously accepted average of ~300 m and a more complex melt sheet–basement interface showing considerable “topography.” The thickest section (1045 m of clast‐free to clast‐poor impact melt overlying 425 m of clast‐laden impact melt) is associated with a centrally located, fault‐bounded graben that was in place prior to melt crystallization. Here we report the results of a geochemical investigation of 115 samples obtained from nine drill holes and a set of field samples. The results reveal that most of the drill core comprises an undifferentiated unit, showing minimal geochemical variation. This is typically ~300 m thick and equates with previous studies performed on samples from exposed rock. In contrast, the deeper section exhibits differentiation and is divided into three layers based on chemical, mineralogical, and textural variations: a quartz monzonite to quartz monzodiorite upper zone (276 m), a quartz monzodioritic middle zone (244 m), and a mainly monzodioritic lower zone (525 m). The mineralogy is defined by plagioclase > orthoclase > clinopyroxene > orthopyroxene, with ubiquitous amphibole and biotite and olivine locally developed in the lower zone and below. Our results reveal that the thicker section of the impact melt sheet has undergone fractional crystallization. Differentiation of parts of the Manicouagan impact melt indicates that lunar impact melt samples possessing different chemistries, previously considered to be derived from distinct impact basins, may be related via the fractionation of common, much smaller diameter impact structures.
机译:最近对Manicouagan冲击结构的勘探钻探发现,冲击熔体的局部发育远厚于先前公认的约300 m的平均厚度,并且熔体-基底界面更为复杂,显示出相当大的“地形”。最厚的部分(覆盖425 m满载荷的1045 m无崩塌至不崩塌的冲击熔体)与熔体结晶之前就位的,位于断层边界的抓斗有关。在这里,我们报告了从9个钻孔和一组现场样品中获得的115个样品的地球化学调查结果。结果表明,大多数钻芯包含未分化的单元,显示出最小的地球化学变化。通常厚约300 m,与先前对裸露岩石样品进行的研究相当。相反,较深的部分表现出差异,并根据化学,矿物学和质地变化分为三层:石英蒙脱石至石英蒙脱闪石上部区(276 m),石英单闪闪岩中间区(244 m)和主要Monzodioritic下部带(525 m)。矿物学的定义为斜长石>正长石>斜向辉石>正辉石,普遍存在闪石和黑云母以及在下部和下部局部发育的橄榄石。我们的结果表明,冲击熔体板的较厚部分经历了分步结晶。 Manicouagan冲击熔体各部分的差异表明,具有不同化学性质的月球冲击熔体样品以前被认为源自不同的冲击盆地,可能与常见的直径较小的冲击结构分馏有关。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号