从白时期到三级时期的边界纳米钻石中获得的陆地碳和同位素比率
概括
在白-第三纪 (K-T) 边界的纳米尺寸钻石不是星际的. 同位素分析显示它们是撞击产生的,不同于已知的石钻石.
科学领域:
- 地质化学 地质化学
- 太空化学 太空化学
- 行星科学 行星科学
背景情况:
- 纳米尺寸的钻石在白纪-第三纪 (K-T) 边界发现.
- 一种假设表明,这些钻石是小行星撞击造成的星际颗粒遗迹.
研究的目的:
- 在K-T边界调查纳米尺寸钻石的起源.
- 为了确定这些钻石是否具有星际或撞击起源.
主要方法:
- 在北美和意大利的K-T边界钻石中分析碳 (13C/12C) 和 (15N/14N) 的同位素比.
- 同位素特征与已知的石和陆地钻石来源的比较.
主要成果:
- 来自北美地区的钻石显示出具有明显的碳和同位素组成和丰度的双成分混合物.
- 来自意大利遗址的钻石没有显示出这些组件的证据.
- K-T钻石的同位素特征与已知的石钻石不同,包括星际钻石.
结论:
- K-T边界纳米钻石的起源并不是星际的.
- 同位素数据强烈表明,钻石是在小行星撞击事件或与之相关的火球中形成的.
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