早期的行星微小分化和晚期的积累形成了地球的预算
Wenzhong Wang1,2,3,4, Michael J Walter5, John P Brodholt6,7
1Deep Space Exploration Lab/School of Earth and Space Sciences, University of Science and Technology of China, Hefei, Anhui, 230026, China. wwz@ustc.edu.cn.
在地球形成期间的同位素分离揭示了核心分离丰富了重同位素,而早期的蒸发有利于更轻的同位素. 这表明晚期积累对地球的气预算产生了重大影响.
科学领域:
- 地质化学 地质化学
- 行星科学 行星科学
- 同位素地球化学 同位素地球化学
背景情况:
- 地球挥发性元素的起源是有争议的,原行星分化和晚期积聚的作用尚不清楚.
- (N) 对生命至关重要,使其库存的形成成为行星科学的关键问题.
研究的目的:
- 在地球的积累和分化过程中调查同位素分离.
- 确定早期过程与晚期增加对地球挥发性库存的相对贡献.
主要方法:
- 使用第一原理计算来建模同位素分离.
- 模拟过程包括核心分离和星云气体蒸发.
主要成果:
- 核心分离使剩余的酸盐富含重同位素.
- 富含气的星云气体的蒸发使行星物以轻同位素丰富.
- 结合的效应有利于在大量的酸盐地球中的轻同位素.
结论:
- 如果地球的气预算是由恩斯泰特-地铁类材料形成的,那么碳状地铁类材料的晚期积累是必要的.
- 同位素约束表明,晚期层对其他挥发性元素 (如H,S和C) 的贡献有限.
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