概括
火星石 (SNCs) 很可能起源于大约2亿年前的100多公里宽的大型撞击坑. 它们接触到宇宙射线的时间要晚得多,在太空碎片化之后.
科学领域:
- 行星科学 行星科学
- 宇宙化学 宇宙化学
- 冲击石坑的形成
背景情况:
- 谢尔戈蒂特,纳克莱特和查西尼 (SNC) 石被强烈认为是火星起源的.
- 以前的火星岩石喷射机制缺乏完全的满足.
研究的目的:
- 为了调查SNC石的可信喷射和宇宙射线暴露历史.
- 为了确定这些火星石最可能的起源场景.
主要方法:
- 利用梅洛什缩模型估计了石坑的大小和弹射速度.
- 分析了火星火山口产量,以评估大型火山口形成的概率.
- 根据碎片事件检查了宇宙射线暴露历史.
主要成果:
- SNC石很可能在2亿年前从一个大石坑 (>100公里直径) 喷射出来.
- 宇宙射线暴露始于0.5-10百万年前,在射出物体的空间碎片化之后.
结论:
- 撞击喷射模型为SNC石的起源提供了一个合理的解释.
- 弹射的时间和随后的宇宙射线暴露是不同的事件.
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