在氧化行星体中透硫化物核心的形成
Samuel D Crossley1,2,3, Jacob B Setera4, Brendan A Anzures5
1NASA Johnson Space Center, 2101 NASA Parkway, Houston, TX, 77058, USA. crossley@arizona.edu.
Nature communications
|April 4, 2025
概括
行星核心的形成可能涉及硫化物化物在岩石融化之前迁移,特别是在氧化物体中. 这个过程解释了石中的贵金属分布,并表明火星等行星的硫化物核心.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 矿物物理 矿物物理
背景情况:
- 星球核心形成模型通常假定酸盐化后会发生金属酸盐分离.
- 氧化条件和丰富的硫比金属更有利于铁硫化物的稳定性.
- 这对于在外太阳系中形成的天体尤为重要.
研究的目的:
- 调查原始的,氧化矿物质组合中的化硫化物融迁移.
- 确定硫化物分离在贵金属分布中的作用.
- 评估对氧化行星体核心组成的影响.
主要方法:
- 使用石样本进行部分融化实验.
- 用部分化合成硫化物进行实验.
- 对贵金属 (Os,Ru,Ir,Pd,Pt) 微量元素比例的分析.
主要成果:
- 在酸盐化之前,在原始的氧化矿物质组合中观察到的透硫化物化迁移.
- 从固体残留物中分化液体硫化物,可以产生明显的贵金属比例.
- 这些比例与氧化石残留物 (brachinites) 和它们的补充融化物中发现的比例相匹配.
结论:
- 提供了强有力的证据,证明石中的硫化物融分离.
- 这表明氧化行星体中预计会有硫化物主导的核心.
- 这种机制为行星核心形成提供了新的视角,包括火星.
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