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关于Io的长期火山活动的同位素证据
Katherine de Kleer1, Ery C Hughes1,2, Francis Nimmo3
1Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
概括
木星
科学领域:
- 星球科学
- 天体化学
- 地质学
背景情况:
- 由于潮的加热, 木星的卫星Io表现出强烈的火山活动.
- 岩石上的挥发性元素同位素构成提供了关于其脱气和质量损失历史的见解.
- 了解Io的演变需要分析其大气中的挥发性库存.
研究的目的:
- 测量Io大气中的硫和同位素.
- 通过同位素分析来限制Io的排气和质量损失历史.
- 为了推断Io的火山活动的持续时间和强度.
主要方法:
- 我们使用了小米级的观测仪.
- 在二氧化硫和一氧化硫气体中测量了硫同位素.
- 在气态化和化中测量同位素.
主要成果:
- 硫同位素比率 (34S/32S) 是高度丰富的 (δ34S = +347 ± 86‰).
- 同位素比率 (37Cl/35Cl) 也显著丰富 (δ37Cl = +263±88‰).
- 它已经失去了94%到99%的硫,
结论:
- 在它大部分的历史中都经历了广泛的火山活动.
- 观察到的同位素丰富表明在地质时间尺度上存在显著的挥发性损失.
- 过去的脱气和质量损失率可能高于目前的速度.
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