在太阳系内部第一代行星体中中等挥发性元素的丰富
Damanveer S Grewal1,2, Surjyendu Bhattacharjee3, Bidong Zhang4
1School of Molecular Sciences, Arizona State University, Tempe, AZ 85281, USA.
Science advances
|February 5, 2025
概括
早期的太阳系行星体富含中等挥发性元素 (MVE). 它们在碰撞期间的随后损失,而不是凝结或分化,解释了地球和火星等陆地行星的MVE耗尽.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 太阳系早期的进化过程
背景情况:
- 在陆地行星中中度挥发性元素 (MVE) 的耗尽尚未完全理解.
- 现有的理论涉及星云凝聚或MVE在行星小的形成和分化过程中的损失.
研究的目的:
- 重建MVE清单的早期内部[非碳 (NC) ]和外部[碳 (CC) ]太阳系行星体.
- 为了调查MVE枯竭在陆地行星的起源.
主要方法:
- 对岩铁石进行分析,以确定MVE的丰度.
- 在小行星天体中重建MVE库存.
主要成果:
- 几个NC和CC铁石母体 (IMPBs) 显示了类似石的MVE丰度,表明了早期的MVE丰富性.
- 第一代行星类物质对陆地行星MVE库存做出了重大贡献.
- 在IMPB中的MVE变化表明中级挥发性损失后的破坏.
结论:
- 地球行星MVE耗尽主要与在广泛的行星小碰撞期间的MVE损失有关.
- 这种碰撞驱动的损失是一个比不完整的凝结或差异化相关的损失更重要的因素.
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