纪-第三纪边界的位置来自Chicxulub火山口的冲击石英
概括
在白-第三纪 (K-T) 边界沉积物中的冲击石英存在分布问题. 新的研究表明,受冲击的湿碳酸盐的冲击脱氧化解释了这些异常,包括温暖的火球效应.
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:
- 在白-第三纪 (K-T) 边界沉积物中的冲击石英与奇克苏鲁布撞击事件有关.
- 观察到的冲击石英的分布模式对现有的冲击模型构成挑战.
- 具体来说,它在喷射层上方的发生,西面的更多丰富性和高速影响是有问题的.
研究的目的:
- 解决在K-T边界的冲击石英分布和特征上的差异.
- 提出一种解释与奇克苏鲁布撞击有关的观察到的异常的机制.
主要方法:
- 在K-T边界沉积物中对冲击石英发生的分析.
- 对冲动力学和冲击波传播的建模.
- 研究目标岩石组成 (湿碳酸盐) 在冲击过程中的作用.
主要成果:
- 冲击石英在北美的主要喷射层上方发现.
- 冲击石英的分布是不对称的,更多的石英在奇克苏鲁布火山口以西.
- 观察到的冲击板块表明中等压力,与解释距离所需的高速冲击不一致.
结论:
- 受到冲击的湿碳酸盐的冲击脱化为观察到的冲击石英分布提供了统一的解释.
- 二氧化碳和二氧化的膨胀产生了二次的,温暖的加速火球,使中等冲击压与观察到的现象相协调.
- 这种机制解决了与奇克苏鲁布撞击有关的空间分布和冲击强度悖论.
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