利略探测器质谱仪:木星大气层的组成
H B Niemann1, S K Atreya, G R Carignan
1Goddard Space Flight Center, Greenbelt, MD 20771, USA.
概括
利略探测器的数据显示了木星的木星数据.
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:
- 木星的大气组成为我们提供了关于太阳系早期的洞察力.
- 以前对木星贵重气体和同位素的测量是有限的.
研究的目的:
- 为了确定木星大气层的详细组成.
- 为了将木星的元素和同位素丰度与太阳和星际值进行比较.
- 为了调查木星大气成分的起源.
主要方法:
- 使用利略探测器上的四极质谱仪对木星大气层进行现场分析.
- 测量气体混合比率和同位素比率从0.5到21bar.
主要成果:
- 与的比率接近太阳.
- 碳,硫和氧的丰度与太阳值有很大的差异.
- 虹灯的丰富程度比太阳能低一个数量级.
- 碳和贵气的同位素比例与太阳相似.
- 与的比率和3与4的比率为原太阳的组成和太阳的进化提供了新的约束.
结论:
- 木星的大气层反映了复杂的形成历史,具有明显的元素丰富.
- 同位素测量支持太阳系进化模型,包括转化为-3.
- 利略探测器的数据为木星大气研究提供了一个基准.
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