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Updated: Jul 11, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
金星上层大气中性组成:来自先驱金星轨道器的初步结果
概括
先金星轨道卫星的测量显示,原子氧是155公里以上的主要热层成分,温度根据太阳角度大大变化. 同位素的比率与地球的值保持一致.
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 空间物理 空间物理
背景情况:
- 金星的热层是理解大气动力学和化学的关键区域.
- 以前对金星上层大气组成和温度概况的了解是有限的.
研究的目的:
- 对金星热层中性成分和温度进行现场测量.
- 为了确定主要气体的相对丰度及其随高度和太阳光照明的变化.
主要方法:
- 在"先金星轨道探测器"上使用了四极质谱仪.
- 在现场测量中性粒子,并从尺度高度推导温度.
主要成果:
- 证实了主要成分的存在:二氧化碳 (CO2),一氧化碳 (CO), (N2),原子氧 (O) 和 (He).
- 在终点区域155公里以下,CO2被确定为最丰富的气体.
- 发现原子氧是155公里以上的主要成分,O/CO2比率高于预期.
- 观测到的热层温度范围从大约400 K在69度的太阳顶角到230 K在90度的太阳顶角.
- 确定氧和碳的同位素比值与地球上的值可比.
结论:
- 原子氧在金星上层热层中扮演的角色比以前认为的更为重要.
- 热层温度表现出强烈的依赖于太阳顶点角度,表明动态过程.
- 同位素组成表明金星和地球的共同起源或类似的进化过程.
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