从Hf-W计时器从小行星和陆地行星的快速积累和早期核心形成
1Institut für Mineralogie, Universität Münster, Corrensstrasse 24, D-48149 Münster, Germany. tkleine@nwz.uni-muenster.de
Nature
|August 29, 2002
概括
使用 hafnium-182 到-182 (Hf-W) 衰变的放射性约会揭示了快速的行星积累. 陆地行星和月球的核心形成发生在太阳系最初的3000万年内.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 地质时间学 (Geochronology)
背景情况:
- 短寿命同位素的放射性衰变,特别是-182到-182 (Hf-W),有助于行星形成和分化的年代.
- 之前的研究表明,太阳系开始后的晚期核心形成 (太阳系开始后的6000万年) 和基于地球地幔W同位素组成的长期积累.
研究的目的:
- 用更新的Hf-W数据重新评估行星形成和核心形成时间表.
- 为了研究行星大小和核心形成持续时间之间的关系.
主要方法:
- 在碳化和H地石石中分析Hf-W同位素数据.
- 使用Hf-W衰变系统作为核形成的计时器.
主要成果:
- 经过修订的Hf-W数据显示,与之前的估计相比,增积和核心形成的时间表显著不同.
- 维斯塔,火星和地球的新年龄确定表明了快速的积累过程.
- 观察到的相关性是,较小的行星体表现出较短的核心形成时间尺度.
结论:
- 陆地行星和月球的核心形成发生在太阳系历史的早期,在最初的3000万年内.
- 这些发现挑战了先前的模型,这些模型表明长时间的积累和晚期的核心形成.
- 行星的大小是影响核心形成持续时间的关键因素.
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