【24h】

Paleomagnetism of impact breccias from the Chicxulub crater - Implications for ejecta emplacement and hydrothermal processes

机译:Chicxulub陨石坑的撞击角砾岩的古磁性-对射出安置和热液过程的影响

获取原文
获取原文并翻译 | 示例
           

摘要

Results of a paleomagnetic study of 89 samples from impact breccias from the Chicxulub crater are presented and used to investigate on ejecta emplacement, hydrothermal and alteration processes. The impactite sequence sampled in cores from Yaxcopoil-1 borehole is ~100. m thick and formed by six subunits characterized by petrographic, scan images, geochemical and textural analyses, which point to different emplacement modes. Impact occurred within reverse polarity chron C29r; therefore, magnetization acquired at crater formation and shortly thereafter will present reverse polarity, which is supported by paleomagnetic measurements on melt samples from Yucatan-6 borehole. Results after step-wise thermal and alternating field demagnetization document a pattern of 23 upward and 29 downward inclinations at Yaxcopoil-1 around -33° and 38°, respectively. Measurements of magnetic hysteresis and variation of low-field susceptibility with temperature suggest low-Ti titanomagnetites and magnetite as main magnetic carriers. Petrographic observations indicate the presence of fine-grained magnetite, hematite and Fe-oxyhydroxides, related to hydrothermal alteration processes. Curie points are in the range of 520-580 °C. The wide range of unblocking temperature spectra points to variable grain sizes of a magnetic phase that unblocks around 580 °C. Hysteresis ratio plots indicate most samples fall in the pseudo-single domain field. In some samples, wasp-waist constrained hysteresis loops suggest magnetite and hematite. Analyses of vector plots and coercivity and unblocking temperature spectra do not show apparent differences within and between subunits. Subunits are characterized by distinct textural and compositional differences in size, type and relative abundance of clasts and melt-rich or carbonate-rich matrix types. Bulk properties vary with composition and clast contents, particularly within the Middle Suevite and Brecciated Melt Rock subunits that show higher values, while low values characterize the Lower Suevite carbonate-rich with rare basement clasts subunit. Magnetization acquisition mechanisms are discussed, with reference to impactite characteristics, and may relate to remagnetization from hydrothermal and post-impact alteration processes.
机译:提出了对来自Chicxulub火山口撞击角砾岩的89个样品的古磁研究结果,并将其用于调查射流安置,水热和蚀变过程。从Yaxcopoil-1井筒的岩心中采样的冲蚀岩层序为〜100。它由6个亚单位组成,厚度为m厚,由岩石学,扫描图像,地球化学和质地分析等特征组成,这些特征指向不同的沉积模式。 C29r极性接反。因此,在火山口形成时以及随后不久获得的磁化强度将呈现相反的极性,这是通过对尤卡坦6井眼熔融样品进行古磁测量得到支持的。逐步进行热和交变磁场消磁后的结果表明,Yaxcopoil-1分别在-33°和38°处分别有23个向上和29个向下倾斜的模式。磁滞现象和低场磁化率随温度的变化表明,低钛的钛磁铁矿和磁铁矿是主要的磁性载体。岩相学观察表明,存在与水热蚀变过程有关的细粒磁铁矿,赤铁矿和羟基氧化铁。居里点在520-580°C的范围内。宽范围的无阻塞温度谱表明,磁性相的晶粒尺寸在580°C左右无阻塞。磁滞比图表明大多数样本属于伪单域字段。在某些样品中,黄蜂腰部约束的磁滞回线表明磁铁矿和赤铁矿。向量图分析,矫顽力和畅通的温度谱分析未显示亚基内部和亚基之间的明显差异。亚基的特征在于碎屑和富含熔体或富含碳酸盐的基质类型在大小,类型和相对丰度方面存在明显的质地和组成差异。松散性质随组成和碎屑含量的不同而变化,特别是在中苏韦石和角砾状熔岩亚基中显示出较高的值,而低值则表示富含下部苏维特碳酸盐岩的稀有基底碎屑亚基。讨论了磁化强度的获取机制,并参考了撞击矿的特征,并且可能涉及热液和撞击后蚀变过程的磁化作用。

相似文献

  • 外文文献
  • 中文文献
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