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Updated: Jun 15, 2026

09:33
An Anaerobic Biosensor Assay for the Detection of Mercury and Cadmium
Published on: December 17, 2018
在水星大气层中发现
T A Bida1, R M Killen, T H Morgan
1W.M. Keck Observatory, CARA, Kamuela, Hawaii 96743, USA. tbida@keck.hawaii.edu
Nature
|March 21, 2000
概括
科学家们在水星中发现.
科学领域:
- 行星科学 行星科学
- 大气化学 大气化学
背景情况:
- 水星的地组成和演变仍然不确定.
- 预测的耐火,无水组成与观察到的大气挥发物形成鲜明对比.
- 大气组成被认为是通过各种过程从表面材料产生.
研究的目的:
- 为了研究水星大气中的的存在和起源.
- 了解导致水星大气组成的过程.
主要方法:
- 在靠近两极的水星大气中观察.
- 对大气柱密度和温度的分析.
主要成果:
- 在水星两极附近的大气中发现.
- 观察到大气的低柱密度和高温度 (12,000K).
- 局部分布表明与极光带的潜在联系.
结论:
- 大气中的可能起源于极光区的离子诱导喷射.
- 低丰度表明,水星上有一个耗尽的细岩.
- 这些发现挑战了关于水星表面组成的先前假设.
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