欧罗巴内部的缓慢演变:变态海洋起源,延迟的金属核心形成,以及有限的海底火山活动
Kevin T Trinh1, Carver J Bierson1, Joseph G O'Rourke1
1School of Earth and Space Exploration, Arizona State University, AZ 85287, USA.
Science advances
|June 16, 2023
概括
欧洲欧洲欧洲欧洲欧洲欧洲
科学领域:
- 行星科学 行星科学
- 天体生物学 天体生物学
- 地质物理学 地质物理学
背景情况:
- 讨论了欧洲的内部组成和差异化.
- 以前的模型假设早期的分化类似于地球.
- 欧洲可能在低温下与水冰或水合酸盐一起积累.
研究的目的:
- 为了模拟欧洲从低初始温度的热演变.
- 研究欧罗巴的海洋和冰的外的起源.
- 评估核心形成和内部加热的时间.
主要方法:
- 热演变的数值建模.
- 模拟酸盐脱水过程.
- 基于低温积累的内部结构分析.
主要成果:
- 酸盐脱水是一种可行的机制,可以产生欧洲的海洋和外.
- 海底岩石可能仍然很冷和水合.
- 核心形成可能发生在积聚后数十亿年.
- 海洋化学可能反映了长期的内部加热.
结论:
- 欧罗巴的海洋和外可以在没有早期分化的情况下从内部过程中形成.
- 月球的内部结构和演变可能与地球的内部结构和演变有很大不同.
- 未来的研究应该考虑在海洋世界模型中长期加热和水合.
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