相关实验视频
Updated: Jul 11, 2026

08:46
Methane Hydrate Crystallization on Sessile Water Droplets
Published on: May 26, 2021
火星:Mariner 9 探测器对H2O冰云的光谱证据
概括
频谱分析显示火星上存在水冰云. 马里纳9号的数据显示,云由H(2) O冰颗粒组成,平均半径为2.0微米,质量为5×10(-5)粒/cm2.
科学领域:
- 行星科学 行星科学
- 频谱学是一种光谱学.
- 大气科学 大气科学
背景情况:
- 航天员9号任务为火星大气研究提供了关键数据.
- 了解火星云是解读火星气候和水循环的关键.
研究的目的:
- 用Mariner 9数据识别火星云的光谱特征.
- 为了确定H(2) O冰云在Tharsis山脊地区的物理性质.
主要方法:
- 分析来自Mariner 9干扰仪光谱仪的光谱数据.
- 观察到的光谱与冰云的理论辐射转移模型的比较.
- 模拟粒子大小分布和集成云质量的变化.
主要成果:
- 观察到的光谱特征被确定为水冰 (H2O冰).
- 塔西斯山脊H(2) O冰云由平均半径约为2.0微米的粒子组成.
- 综合云质量被确定为每平方厘米的5 x 10(-5) 粒.
结论:
- 火星上水冰云的存在和组成已经得到证实.
- 这些云的物理特征为火星大气过程提供了洞察力.
- 这项研究完善了我们对火星大气中的水分布的理解.
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