概括
小行星撞击在白纪-第三纪边界创造了玻璃球体. 氧同位素和主要元素分析显示,这些玻璃是融化碳酸盐和酸盐岩石的混合物,而不是火山或蒸发起源.
科学领域:
- 地质化学 地质化学
- 同位素分析的分析.
- 冲击石坑的形成
背景情况:
- 甲-第三纪 (K-T) 边界标志着一个重要的大规模灭绝事件.
- 了解K-T边界的地质特征对于重建过去的环境变化至关重要.
研究的目的:
- 为了分析在海地K-T边界发现的玻璃球体的组成.
- 为了确定这些撞击玻璃的起源和形成过程.
主要方法:
- 单个玻璃球体的激光提取氧气同位素分析.
- 玻璃球体的主要元素分析.
- 解释地质化学混合趋势.
主要成果:
- 玻璃球体表现出高 (重氧同位素) 和高 (轻氧同位素) 组成之间的混合趋势.
- 同位素和元素数据表明异质源岩的融化.
- 这些玻璃是碳酸盐和酸盐岩石的混合物.
结论:
- 观察到的混合线与大约6500万年前的小行星或彗星撞击事件一致.
- 撞击融化了碳酸盐和酸盐岩石的混合物.
- 火山过程或混合物涉及富含硫酸盐的蒸发物被排除在这些玻璃的来源之外.
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