地球的挥发性枯竭趋势与高能量的月球形成撞击相一致
Natalia V Solomatova1, Razvan Caracas2,3
1CNRS, Ecole Normale Supérieure de Lyon, Laboratoire de Géologie de Lyon LGLTPE UMR5276, Centre Blaise Pascal, 46 allée d'Italie, Lyon, 69364 France.
概括
月球形成的撞击可能已经显著耗尽了地球的挥发性元素,包括. 模拟显示,并不过剩,这表明冲击在挥发性损失中扮演的角色比以前想象的要大.
科学领域:
- 行星科学 行星科学
- 地质化学 地质化学
- 宇宙化学 宇宙化学
背景情况:
- 地球的挥发性元素的丰富度相对于地铁,限制了行星的热化学进化.
- 与相似的星云凝结温度元素相比,的明显过剩是有争议的.
研究的目的:
- 在早期的岩海洋条件下,研究火石融中的蒸发.
- 将的行为与月球形成后的其他小元素进行比较.
主要方法:
- 使用了初始分子动力学模拟.
- 模拟的印蒸发从火矿化物.
- 模拟了早期岩海洋的条件.
主要成果:
- 在没有太阳星云气体的情况下从岩海洋蒸发时不会表现出过剩.
- 观察到印度丰度略有不足.
- 印的行为与其适度的 siderophile性质保持一致.
结论:
- 高能量的月球形成冲击可能对挥发性物质耗尽作出了重大贡献.
- 以前关于过剩的假设可能是不正确的.
- 冲击是地球挥发性元素库存的一个关键因素.
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