来自MESSENGER的水星表面的放射性元素:对这个星球的形成和演变的影响
Patrick N Peplowski1, Larry G Evans, Steven A Hauck
1The Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723, USA. patrick.peplowski@jhuapl.edu
概括
传奇世界 传奇世界 传奇世界
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 核天体物理学 核天体物理学
背景情况:
- 水星的表面成分为它的形成和演变提供了线索.
- (K), (Th) 和 (U) 等放射性元素是行星过程的关键指标.
研究的目的:
- 为了确定K,Th和U在水星北半球的表面丰度.
- 利用这些丰度来限制水星的形成和热史模型.
主要方法:
- 使用了来自MESSENGER马射线光谱仪的数据.
- 在水星北半球测量了K,Th和U的平均表面丰度.
主要成果:
- 平均表面丰度:K (1150±220ppm),Th (220±60ppb),U (90±20ppb) 在表面均:K (1150±220ppm),Th (220±60ppb),U (90±20ppb).
- 该K/Th和K/U比率表明形成从挥发性丰富的材料,而不是极端加热.
- 丰富度表明,自形成以来,内部热量生产有显著的下降.
结论:
- 水星很可能是由类似于体石的挥发性物质形成的.
- 在水星历史早期发生了广泛的火山活动,随后活动减少.
- 这些发现挑战了在形成过程中需要极端行星升温的模型.
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