在火星大气层中检测到分子
V A Krasnopolsky1, P D Feldman
1Department of Physics, Catholic University of America, Washington, DC 20064, USA. vkrasn@altavista.com
概括
科学家在火星大气层中检测到气 (H2),这揭示了自火星早期历史以来水的大量流失. 这一发现表明,火星可能曾经拥有比地球更多的水.
科学领域:
- 行星科学 行星科学
- 大气化学 大气化学
- 天体生物学 天体生物学
背景情况:
- 了解火星上水的历史对于评估其过去的可居住性至关重要.
- 以前的研究表明,火星经历了显著的气候变化,导致水的流失.
研究的目的:
- 量化火星大气中的分子 (H2) 的丰富程度.
- 为了调查H2和 (D) 分割对火星水的历史的影响.
主要方法:
- 使用远紫外光谱探测器 (FUVSE) 观测火星光谱中的四条 (H2) 线.
- 对线路强度的分析,以确定140公里以上的柱子H2丰度.
- 应用光化学模型来模拟H2的丰度和估计混合比率.
主要成果:
- 检测到四条H2线,其中三条被太阳莱曼β光子激发.
- 在140公里以上,估计列H2的丰度为1.17 x 10^13分子/厘米^2.
- 在下层大气中计算的H2混合比为15 +/- 5 ppm,与光化学分化相符.
结论:
- 火星H2和HD的混合比率支持水蒸气和分子之间的的光化学分化.
- 分析表明,自从水力动力逃逸结束以来,全球海洋的深度超过30米.
- 火星最初可能拥有比地球更多的水份,大气逃逸后只剩下4%的水.
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