在土星环落入大气中的尘埃颗粒的现场收集
Hsiang-Wen Hsu1, Jürgen Schmidt2, Sascha Kempf3
1Laboratory for Atmospheric and Space Physics, University of Colorado-Boulder, Boulder, CO, USA. sean.hsu@lasp.colorado.edu.
概括
土星的环不仅仅是冰. 卡西尼探测器的数据显示,酸盐粒, 不仅仅是水冰, 落入土星,
科学领域:
- 星球科学
- 太空尘埃分析
- 土星系统动态
背景情况:
- 土星的主要环主要是水冰 (>95%).
- 剩下的几百分之一的环材料的组成是不确定的.
- 之前的研究推断"环雨"物质从环落到土星.
研究的目的:
- 直接检测和描述来自土星主要环的物质.
- 通过实地测量分析入环材料的组成.
- 澄清土星环中的非冰成分的性质.
主要方法:
- 使用卡西尼太空船的宇宙尘埃分析仪 (CDA) 撞击质谱仪.
- 在土星和D环之间的穿越过程中收集和分析尘埃粒.
- 检测到的颗粒的大小,组成 (水冰,酸盐) 和动态.
主要成果:
- 从土星主要环中释放的纳米大小的颗粒直接在现场检测.
- 在降落材料中识别水冰和酸盐颗粒.
- 酸盐颗粒包括高达30%的落入颗粒,超过环的散装酸盐含量.
结论:
- 土星的环中含有重要的,以前被低估的非冰 () 成分.
- 发现的酸盐颗粒有助于"环雨"影响土星的现象.
- 这些发现需要对环组成和进化模型进行修订.
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