Detailed Occurrence of Feather Features in Quartz in Experimentally Shocked Granite

IF 3.9 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Toshihiro Tada, Kosuke Kurosawa, Naotaka Tomioka, Takayoshi Nagaya, Junko Isa, Christopher Hamann, Haruka Ono, Takafumi Niihara, Takaya Okamoto, Takafumi Matsui
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Abstract

Feather features (FFs) in quartz consist of a planar fracture (PF) and associated fine lamellae (FF lamellae; FFL) and have been observed in various natural impact structures. However, the mechanisms and conditions of FF formation are poorly understood. We conducted shock recovery experiments on granite using decaying compressive pulses to investigate the formation conditions of FFs. We characterized the recovered samples using an optical microscope equipped with a universal stage, a scanning electron microscope combined with an electron back-scattered diffraction detector, and a transmission electron microscope. We found that FFs are formed over a wide range of peak pressures (2–18 GPa) and that FFs can be divided into at least three types (I–III) based on the crystallographic orientation of the PFs and FFL, the angle between the orientation of the FFL and the propagation direction of the compression wave, and the presence/absence of amorphous silica in the FFL. The peak pressures that produce type I–III FFs are estimated to be <12, 12–14, and >16 GPa, respectively. We propose that FFs can be used as a shock barometer for quartz-bearing rocks.

Abstract Image

实验冲击花岗岩中石英羽状特征的详细出现情况
石英中的羽状特征(FFs)由平面断裂(PF)和相关细薄片(FF lamellae; FFL)组成,在各种天然撞击结构中都曾观察到。然而,人们对 FF 的形成机制和条件知之甚少。我们利用衰减压缩脉冲对花岗岩进行了冲击恢复实验,以研究 FF 的形成条件。我们使用配备通用平台的光学显微镜、结合电子背散射衍射探测器的扫描电子显微镜和透射电子显微镜对复原样品进行了表征。我们发现,FFs 是在很宽的峰值压力(2-18 GPa)范围内形成的,根据 PFs 和 FFL 的晶体学取向、FFL 取向与压缩波传播方向的夹角以及 FFL 中是否存在无定形二氧化硅,FFs 至少可分为三种类型(I-III)。据估计,产生 I-III 型 FF 的峰值压力分别为 12、12-14 和 16 GPa。我们建议将FFs用作含石英岩石的冲击气压计。
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来源期刊
Journal of Geophysical Research: Planets
Journal of Geophysical Research: Planets Earth and Planetary Sciences-Earth and Planetary Sciences (miscellaneous)
CiteScore
8.00
自引率
27.10%
发文量
254
期刊介绍: The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.
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