火星的大气.火星的大气. 火星甲检测和在盖尔火山口的变异性
Christopher R Webster1, Paul R Mahaffy2, Sushil K Atreya3
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. chris.r.webster@jpl.nasa.gov.
概括
火星的背景甲含量很低,但偶尔出现的高甲峰值表明来源不明. 因为好奇心,好奇心.
科学领域:
- 行星科学 行星科学
- 天体生物学 天体生物学
- 大气化学 大气化学
背景情况:
- 火星上的甲羽毛已经被观察到,但缺乏解释.
- 之前的模型建议来自尘埃或石的甲,但这些不足.
- 了解火星甲是评估潜在可居住性的关键.
研究的目的:
- 使用现场数据测量火星大气中的甲丰度.
- 为了调查火星上观察到的甲变化的来源.
- 将测量结果与现有的地球化学和大气模型进行比较.
主要方法:
- 在火星样本分析 (SAM) 仪器套件上使用了可调节激光光谱仪 (TLS).
- 在盖尔火山口进行了20个月的现场测量.
- 分析了背景甲水平和偶尔高度的数据.
主要成果:
- 检测到的平均背景甲水平为0.69 ± 0.25 ppbv.
- 观测到的偶尔甲峰值在60个月内高达7.2±2.1ppbv.
- 背景水平低于紫外线降解模型预测的水平.
结论:
- 火星的背景甲含量明显低于之前的模型.
- 偶尔的甲释放表明火星上有一个活跃的,未知的甲来源.
- 需要进一步的研究来确定这种偶发的甲的来源.
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