在火星上层大气层中检测到原子
V A Krasnopolsky1, M J Mumma, G R Gladstone
1Department of Physics, Catholic University of America, Washington, DC 20064, USA. VKras@lepvx3.gsfc.nasa.gov
概括
火星 火星 火星 火星 火星
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 天体化学是天体化学.
背景情况:
- 了解火星的大气组成和演变是它可居住性的关键.
- 火星水和大气气体中的 (重) 与的比率提供了对水损失和大气过程的见解.
研究的目的:
- 测量火星大气中的莱曼α线强度.
- 确定结分子 (HD) 与分子 (H2) 的比率.
- 为了比较HD/H2的分化与水 (HDO/H2O) 的分化,并了解火星大气过程.
主要方法:
- 使用哈勃太空望远镜的高分辨率光谱学.
- 测量了火星大气中的莱曼α线的强度.
主要成果:
- 在23 +/- 6 rayleighs检测到莱曼α线.
- 计算的HD/H2比为1.5 +/- 0.6 x 10(-4).
- 发现HD/H2比HDO/H2O小11倍,这表明分离的热力学控制.
结论:
- 火星HD/H2分离是通过热力学控制的,而不是动力学.
- 分子 (H2) 与水相比,在中显著耗尽,这是由于其在大气中的寿命长.
- 观察到的同位素分离表明,地球上存在大约5米厚的可交换水冰储备.
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