概括
火星上的因选择性大气逃逸而富含同位素 (15) N. 早期火星的气压力可能高达30毫巴.
科学领域:
- 行星科学 行星科学
- 大气化学 大气化学
- 同位素地球化学 同位素地球化学
背景情况:
- 维京人的测量显示,火星大气中同位素 (15) N 的丰富程度显著.
- 这种丰富表明火星上有大气损失过程的历史.
研究的目的:
- 为了模拟火星上的过去历史.
- 为了解释火星大气中观察到的15N的丰富.
主要方法:
- 利用维京号任务数据来分析大气组成.
- 开发大气逃逸模型,特别关注选择性过程.
- 研究电子冲击解离N(2) 和解离性重组N(2) ((+) 在大气损失中的作用.
主要成果:
- (15) N的丰富与选择性大气逃生机制相一致.
- 在外层形成的快速原子有助于这种选择性损失.
- 最初的 (N(2)) 部分压力可能是几毫巴.
结论:
- 同位素的选择性逃逸在塑造目前的火星大气层方面发挥了至关重要的作用.
- 如果表面过程作为大气HNO2和HNO3的重要沉积点,则最初的气压力可能达到30毫巴.
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