由剪切变形产生的核心形成化的相互连接网络
1Department of Geology & Geophysics, University of Minnesota, Minneapolis 55455, USA. bruhn@olivine.geology.umn.edu
Nature
|March 8, 2000
概括
星球核心的形成可能不需要岩海洋. 实验表明剪切变形可以使金属融通过固体地幔透,为核心发展提供了一个新的机制.
科学领域:
- * 星球科学 星球科学
- * * 地质物理学
- * 实验性岩石学研究
背景情况:
- * 驱动陆地行星核心形成的精确机制在很大程度上是未知的.
- *当前的模型经常提出岩海洋或化金属的重力沉没.
- * 由于水静态实验结果,通过固体矩阵的透已经被扣除.
研究的目的:
- * 调查行星核心形成的替代机制.
- * 在非水静态条件下测试融透在固体地幔中的可行性.
- * 挑战目前盛行的岩海洋假设.
主要方法:
- *高压实验模拟行星内部条件.
- * 在金属/金属硫化物融的固体多晶橄中应用剪切变形.
- *分析融的相互连接性和透途径.
主要成果:
- *剪切变形成大株成功地相互连接的金属和金属硫化物融化的隔离口袋在固体橄基质中融化.
- * 这表明,在动态的非水静态环境中,透是可能的.
- * 结果与之前基于水静态实验的假设相矛盾.
结论:
- *行星核心的形成可以通过融物通过固体酸盐地幔的透而发生,即使没有完整的岩海洋.
- * 涉及剪切变形的动态过程对于使融迁移至关重要.
- * 这提供了一种可行的替代机制,用于在陆地行星上分离核心材料.
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