原始小行星作为陆地挥发性物质的主要来源
Rayssa Martins1,2, Elin M Morton1, Sven Kuthning1
1Department of Earth Science & Engineering, Imperial College London, London, UK.
Science advances
|October 11, 2024
概括
地球 地球 地球 地球 地球 地球
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 同位素宇宙化学 同位素宇宙化学
背景情况:
- 地球的挥发性元素,如 (Zn) 的起源是一个重要的科学辩论.
- 关于同位素组成的先前研究表明石的起源来自外星,但往往排除了行星的关键构建块.
研究的目的:
- 为了研究从差异化行星的石的质量独立的同位素组成.
- 模拟不同类型的石对地球预算和同位素特征的贡献.
主要方法:
- 在石中的质量独立的同位素组合的分析.
- 开发和应用混合模型来模拟地球的挥发性元素积累.
主要成果:
- 来自差异化行星类的石,尽管形成了地球质量的70%左右,但只贡献了其的10%左右.
- 原始,未化的材料是地球和其他挥发性元素的主要来源.
结论:
- 不同化的行星类并不是地球的主要来源.
- 未融化的原始材料的积聚对于建立陆地行星的挥发性元素库存至关重要.
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