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贝皮科伦博任务的第二次金星飞越显示了几十年来稳定的大气层
Jörn Helbert1, Rainer Haus2, Gabriele Arnold2,3
1German Aerospace Center (DLR), Institute of Planetary Research, Rutherfordstrasse 2, 12489, Berlin, Germany. joern.helbert@dlr.de.
Nature communications
|December 12, 2023
概括
新的测量显示,金星的中层层仍然稳定,与1983年的数据一致. 水星射线仪和热红外光谱仪 (MERTIS) 提供了关键的温度和云数据,有助于比较行星学.
科学领域:
- 行星科学 行星科学
- 大气科学 大气科学
- 金星科学 金星科学
背景情况:
- 金星中层是理解大气动力学和与地球的比较行星学的关键.
- 以前的来自金星的中层层层数据可以追溯到1983年Venera-15任务.
- 了解金星的大气对于洞察行星进化至关重要.
研究的目的:
- 为呈现金星大气层的新中红外光谱测量.
- 为了检索中大层温度概况和云的参数.
- 为了评估几十年来金星大气层的稳定性.
主要方法:
- 使用了水星辐射仪和热红外光谱仪 (MERTIS) 仪器.
- 在BepiColombo任务的第二次飞越金星期间进行了测量.
- 进行了用于大气回收的光谱分析.
主要成果:
- 成功地获取了60至75公里高度之间的中大层温度概况和云参数.
- 为了水星而设计的MERTIS提供了可靠的金星数据.
- 结果与Venera-15的发现一致,表明大气稳定.
结论:
- 金星大中层在几十年的时间尺度上表现出了显著的稳定性.
- 新的MERTIS数据验证了长期大气的一致性.
- 这项研究弥合了金星大气研究中的重大数据缺口.
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