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在甘尼米得上检测到臭氧
K S Noll1, R E Johnson, A L Lane
1Space Telescope Science Institute, Baltimore, MD 21218, USA.
用哈勃太空望远镜在加尼米得上检测到臭氧 (O3). 这一发现表明,在加尼米德的冰冷表面中,有被困的O3-O2大气层.
科学领域:
- 行星科学 行星科学
- 天体生物学 天体生物学
- 频谱学是一种光谱学.
背景情况:
- 木星最大的卫星加尼米德的大气层很薄弱.
- 之前的观测已经在甘尼米德的后半球上检测到分子氧 (O2).
研究的目的:
- 在甘尼米得上检测和描述臭氧 (O3).
- 调查发现的大气物种的起源和状态.
主要方法:
- 利用哈勃太空望远镜观测260nm的吸收带.
- 分析了臭氧 (O3) 的哈特利波段,以确定其丰富度和特性.
主要成果:
- 检测到一个臭氧吸收带,确定它为哈特利带.
- 测量了每平方厘米4.5 x 10^16个分子的臭氧柱丰富度.
- 推断出臭氧与氧的比率 ([O3]/[O2]) 在10^-4和10^-3.之间.
结论:
- 观察到的臭氧和氧气可能会在加尼米德的冰中形成表面被困的"大气".
- 臭氧带的光谱特征支持它被限制在冰中,而不是气态.
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