来自利略近红外测绘光谱仪的Io近距离观察
R Lopes-Gautier1, S Douté, W D Smythe
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
概括
利略航天器的红外图像揭示了木星的木星.
科学领域:
- 行星科学 行星科学
- 火山学 火山学是一门学科.
- 天文地质学 天文地质学
背景情况:
- 木星的卫星Io是太阳系中火山活动最活跃的天体.
- 了解Io的火山活动,可以了解行星进化和内部过程.
研究的目的:
- 为了研究Io的活火山的热结构.
- 为了绘制Io表面二氧化硫分布的地图.
- 分析火山活动,热量排放和表面组成之间的关系.
主要方法:
- 来自利略航天器的红外光谱图像的分析.
- 绘制火山区域的热辐射模式.
- 表面特征与二氧化硫沉积物的相关性.
主要成果:
- 洛基帕特拉 (Loki Patera) 显示了大量冷却岩的区域,表明了火山的显著重新浮出水面.
- 普罗米修斯表现出明显的热辐射区域,支持羽毛迁移模型.
- 二氧化硫沉积物与表面颜色呈现复杂的空间关系,表明存在各种各样的硫化合物.
结论:
- 伊奥的火山活动是动态的,像洛基·帕特拉和普罗米修斯这样的特征为火山过程提供了关键的见解.
- 二氧化硫的分布比以前理解的要复杂得多,这意味着表面化学的范围更广.
- 红外成像对于描述活跃火山卫星的热量和组成状况至关重要.
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