概括
月球岩石的冲击变形显示了高压变形和融化. 两个撞击源和不同的融化化学成分表明,不同的月球地形受到影响.
科学领域:
- 地质地质地质地质地质地
- 行星科学 行星科学
- 冲击石坑的形成
背景情况:
- 冲击变形是对行星体撞击事件的关键指标.
- 月球上的水晶岩石和岩保存了极端压力和温度的证据.
研究的目的:
- 为了研究冲击变形对月球晶体岩石和石的影响.
- 要区分初级和二级冲击冲击源.
- 分析冲击诱导化的化学变化.
主要方法:
- 用显微镜检查岩石样本的变形结构.
- 对于冲击特征,对塑酸盐和烟氧的分析.
- 冲击诱导融化玻璃的化学分析.
主要成果:
- 冲击变形明显在精细的材料和破裂,很少在粗碎片.
- 观测到的变形结构在Plagioclase和Pyroxene,透视玻璃,和冲击化.
- 确定了两个主要冲击源:石撞击和石坑喷射物撞击.
- 区分了两种主要的冲击诱导化的化学类型.
结论:
- 月球岩石在高压事件中表现出显著的冲击变形.
- 冲击冲击波源于初级和二级冲击事件.
- 融化的化学差异与海和高地地区的撞击地点相关.
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