在火星核心上存在液态酸盐层的证据
1Institute of Geochemistry and Petrology, ETH Zürich, Zurich, Switzerland. amir.khan@erdw.ethz.ch.
Nature
|October 25, 2023
概括
火星
科学领域:
- 星球科学
- 地震学
- 地质学
背景情况:
- 据InSight任务的地震数据显示,火星的核心比纯铁轻27%.
- 地震和地质模型表明,比宇宙化学上可用的元素更易挥发 (H,C,S).
- 核心组成模型与行星形成约束之间的差异.
研究的目的:
- 通过地震数据研究火星的核心组成和结构.
- 为了协调火星内部的地震,地质和宇宙化学模型之间的差异.
- 确定核心-地幔边界和覆盖层的特性.
主要方法:
- 来自InSight地震记录的多重衍射P波的分析.
- 液体铁合金的热弹性性能的第一原理计算.
- 对核心-地幔边界敏感的差异体波旅行时间数据的反转.
主要成果:
- 证据表明一个有层次的核心-地幔边界与化层.
- 核心半径减小 (1.675 ± 30 公里),核心密度增加 (6.65 ± 0.1 g/cm3).
- 化层厚度 (150 ± 15 公里) 和密度 (4.05 ± 0.05 g/cm3).
- 核心组成:85-91%的铁,9-15%的轻元素 (S,C,O,H).
结论:
- 推断的核心特性解决了地质物理和宇宙化学要求之间的差异.
- 在较小,更密集的核心上方的一层化与地震数据一致.
- 火星的岩石产物可能会显示出这种酸盐层的化学特征.
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