同位素证据反对一个恩斯塔提特地地
Caroline Fitoussi1, Bernard Bourdon
1Laboratoire de Géologie de Lyon, ENS Lyon, CNRS and Université Claude Bernard de Lyon, Lyon, France. caroline.fitoussi@ens-lyon.fr
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
- 宇宙化学 宇宙化学
- 地质化学 地质化学
背景情况:
- 地球的大体组成类似于恩斯塔提特地铁.
- 对于地球的恩斯塔提特石石石积聚模型缺乏明确的证据.
- (Si) 同位素为行星形成提供了一个独特的标志物.
研究的目的:
- 为了测试使用Si同位素对地球的静态合石积累模型.
- 研究核心形成和月球形成对地球Si同位素特征的影响.
- 为了调和恩斯塔提特混和陆地Si同位素数据之间的差异.
主要方法:
- 在陆地样本 (大批酸盐地球,月球) 中分析Si同位素特征.
- 陆地Si同位素与各种外星物质的比较,包括恩斯塔提特地质.
- 核心形成和冲击后过程的建模,以解释观察到的Si同位素变化.
主要成果:
- 地球的Si同位素组成不能通过简单的恩斯塔合金积和核心形成来解释.
- 大量酸盐地球和月球之间的Si同位素相似性排除了隐藏的下层地幔储库.
- 一个三端成员的混凝土混合模型成功地协调了地球和恩斯泰特混凝土的Si同位素数据.
结论:
- 对于地球的积累,静态地模型需要进行重大修订.
- 月球形成撞击和随后的平衡在塑造地球Si同位素签名方面发挥了关键作用.
- 一个更复杂的混凝土混合模型是必要的,以充分解释地球的元素和同位素组成.
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