相关实验视频
Updated: Aug 17, 2026

14:22
Activating Molecules, Ions, and Solid Particles with Acoustic Cavitation
Published on: April 11, 2014
在地球地幔中发现的裂异
1J. Kunz, Institut de Physique du Globe de Paris, Laboratoire de Geochimie et Cosmochimie, Centre National de la Recherche Scientifique URA 1758, 4 place Jussieu, F-75252 Paris Cedex 05, France. T. Staudacher, Institut de Physique du.
概括
-244的裂变解释了地球30%的裂变.
科学领域:
- 地质化学 地质化学
- 宇宙化学 宇宙化学
- 行星科学 行星科学
背景情况:
- 地球内部的同位素为早期太阳系过程提供了洞察力.
- 放射性贵气是行星形成和进化的关键标志物.
研究的目的:
- 量化-244裂变对地球裂变性的贡献.
- 为了精确地球积聚和大气形成的时间.
主要方法:
- 分析了中海的玄武岩玻璃.
- 射线测年技术. 射线测年技术.
- 对和其他贵重气体的同位素分析.
主要成果:
- -244 (Pu-244) 裂变约占裂变性异过量的30%.
- -238 (U-238) 的自发裂变解释了剩余的裂变性异.
- -129 (Xe-129) 过量表明地球的积累结束了50-70亿年后的太阳系形成.
结论:
- 早期的太阳系放射性核,如Pu-244,显著影响了地球的同位素组成.
- 地球的大气层可能是通过地幔脱气形成的.
- 地球积聚的时间受到灭绝的放射性核酸数据的限制.
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