原始行星体的积聚:从静态地铁体的Hf-W同位素证据
1Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109-1063, USA. Institute for Isotope Geology and Mineral Resources, Department of Earth Sciences, ETH Zurich, CH-8092, Zurich, Switzerland.
概括
曾经被认为是地球的构建块的恩斯塔提特,显示出不同的同位素数据. 这表明大量的重新分布,可能来自行星小碰撞,而不是内部过程.
科学领域:
- 宇宙化学 宇宙化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 恩斯塔提特石是石,通常与地球的积累物质有关.
- 之前的研究表明,静态地铁和陆地行星体之间存在密切的关系.
研究的目的:
- 通过使用同位素,研究恩斯泰特和地球的增积物质之间的关系.
- 为了确定恩斯塔提特地石是否与其他早期太阳系材料同时形成.
主要方法:
- 分析 (W) 的同位素组合物在恩斯塔提特混凝土中的分析.
- 测量初始的哈夫 (Hf) 同位素比率 ((182) Hf / ((180) Hf) 在酸盐和金属部分.
- 使用Hf-W系统进行放射测年.
主要成果:
- 的同位素数据揭示了恩斯塔提特混凝土和假定的地球增积物质之间的显著差异.
- 在酸盐和金属部分中观察到明显的初始 (182) Hf / 180) Hf 比率.
- 据计算,明显的年龄差异为138 +/- 5.3万年,与简单的积累模型不一致.
结论:
- 恩斯塔提特地石可能不是从与地球相同的同质水库中形成的.
- 内部再平衡不能完全解释观察到的同位素差异.
- 大规模的再分配,可能是通过小行星碰撞,是对观察到的数据更合理的解释.
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