Department of Earth Science, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan.
Proc Natl Acad Sci U S A. 2011 Jan 11;108(2):463-6. doi: 10.1073/pnas.1009338108. Epub 2010 Dec 27.
Microcrystals of coesite and stishovite were discovered as inclusions in amorphous silica grains in shocked melt pockets of a lunar meteorite Asuka-881757 by micro-Raman spectrometry, scanning electron microscopy, electron back-scatter diffraction, and transmission electron microscopy. These high-pressure polymorphs of SiO(2) in amorphous silica indicate that the meteorite experienced an equilibrium shock-pressure of at least 8-30 GPa. Secondary quartz grains are also observed in separate amorphous silica grains in the meteorite. The estimated age reported by the (39)Ar/(40)Ar chronology indicates that the source basalt of this meteorite was impacted at 3,800 Ma ago, time of lunar cataclysm; i.e., the heavy bombardment in the lunar surface. Observation of coesite and stishovite formed in the lunar breccias suggests that high-pressure impact metamorphism and formation of high-pressure minerals are common phenomena in brecciated lunar surface altered by the heavy meteoritic bombardment.
微拉曼光谱、扫描电子显微镜、电子背散射衍射和透射电子显微镜分析表明,在一块月球陨石 Asuka-881757 的冲击熔体囊中,非晶态二氧化硅颗粒中发现了柯石英和斯石英的微晶。这些非晶态二氧化硅中的高压多晶型表明,陨石经历了至少 8-30 GPa 的平衡冲击压力。在陨石中也观察到了其他非晶态二氧化硅颗粒中的次生石英颗粒。(39)Ar/(40)Ar 年代学报告的估计年龄表明,该陨石的源玄武岩是在 3800 Ma 前受到撞击的,即月球灾变时期;也就是月球表面的大量陨石撞击。在月球角砾岩中观察到柯石英和斯石英的形成表明,在大量陨石撞击下改变的月球表面的角砾岩中,高压冲击变质作用和高压矿物的形成是常见现象。