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Updated: Jun 18, 2026

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Conducting Miller-Urey Experiments
Published on: January 21, 2014
彗星尘埃作为白纪/第三纪边界的氨基酸来源
1NASA Ames Research Center, Moffett Field, California 94035, USA.
Nature
|November 8, 1990
概括
在白纪/三级纪 (K/T) 边界附近发现的外星氨基酸表明来自彗星尘埃的沉积,而不是撞击. 这个理论解释了它们在边界层上方和下方的存在,以及在撞击粘土本身的缺席.
科学领域:
- 天体生物学 天体生物学
- 地质化学 地质化学
- 古生物学的古生物学
背景情况:
- 在丹麦Stevns Klint的白纪/三级纪 (K/T) 边界检测到的外星氨基酸.
- 在边界粘土上方和下方的层中发现的氨基酸,但不在其中.
研究的目的:
- 在K/T边界调查外星氨基酸的起源和沉积机制.
- 为了使氨基酸的存在与K/T撞击事件相协调.
主要方法:
- 来自K/T边界的岩石样本的地化学分析.
- 氨基酸分布与撞击和彗星尘埃沉积模型的比较.
主要成果:
- 在K/T边界粘土中缺少氨基酸,这使得冲击传递具有挑战性.
- 边界的两侧层中氨基酸的存在表明沉积独立于主要撞击事件.
结论:
- 在K/T边界的外星氨基酸可能起源于彗星尘埃.
- 彗星尘埃,而不是撞击器本身,在撞击事件之前和之后将这些益生菌分子送到地球.
相关概念视频
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