在巨大的撞击后,地球的冷却和核心形成
Bernard J Wood1, Alex N Halliday
1Department of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK. bwood@els.mq.edu.au
Nature
|October 28, 2005
概括
地球 地球 地球 地球 地球 地球
科学领域:
- 地质物理学 地质物理学
- 行星科学 行星科学
- 地质化学 地质化学
背景情况:
- 凯尔文爵根据导电冷却计算地球的年龄为2400万年.
- 月球形成的巨大撞击显著改变了地球的热状态和组成.
- 在U-Pb和Hf-W同位素系统之间存在关于地球积累和核心分离时间尺度的不一致.
研究的目的:
- 解释来自U-Pb和Hf-W同位素系统的不同时间尺度.
- 为了使早期地球冷却模型与地质和同位素证据相协调.
- 为晚期核心分离和其对地球年龄的影响提出一种机制.
主要方法:
- 对同位素系统 (U-Pb和Hf-W) 的分析以确定时间尺度.
- 地球冷却和核心分离过程的建模.
- 研究巨型撞击和地幔结晶的作用.
主要成果:
- Hf-W时间表反映了月球形成撞击之前的核心形成.
- 巨大的撞击过程中的氧化导致了富含硫的金属核心的晚期分离.
- 这种晚期分离,发生在月球形成撞击后的30 +/- 10 Myr,解释了地球的U-Pb约会.
- 在此期间,地球冷却了大约4000K,符合凯尔文的冷却估计.
结论:
- 一个两阶段的核心形成过程调和了不同的同位素时间尺度.
- 氧化和晚期金属分离显著影响了地球早期的热进化.
- 拟议的模型提供了对早期地球历史和冷却的更全面的理解.
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