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彗星67P上复杂的有机硫分子:来自ROSINA测量的证据和实验室模拟的见解
Ahmed Mahjoub1,2, Kathrin Altwegg3, Michael J Poston4
1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Science advances
|June 7, 2023
概括
罗塞塔任务在彗星67P/Churyumov-Gerasimenko尘埃中检测到复杂的有机硫化合物. 实验室模拟表明,这些由辐射冰形成,突出硫.
科学领域:
- 行星科学 行星科学
- 天体化学是天体化学.
- 彗星科学 彗星科学
背景情况:
- 罗塞塔任务的ROSINA仪器提供了前所未有的彗星组成数据.
- 彗星67P/Churyumov-Gerasimenko表现出复杂的物质组成.
- 以前的研究表明,彗星的昏迷中存在硫化物种.
研究的目的:
- 为了分析来自2016年9月彗星67P/Churyumov-Gerasimenko上的尘埃事件的挥发性尘埃颗粒.
- 为了识别和描述彗星尘埃中的有机硫物种.
- 研究这些含硫有机化合物的形成途径.
主要方法:
- 来自ROSINA (罗塞塔轨道仪离子和中性分析光谱仪) 仪器的数据分析.
- 研究在特定的彗星尘埃事件中挥发的尘埃颗粒.
- 冰辐射的实验室模拟来复制潜在的形成机制.
主要成果:
- 在挥发性尘埃中检测大型有机硫物种.
- 观察到以前检测到的硫化物种在昏迷中的丰度增加.
- 数据支持彗星表面存在复杂的含硫有机物质.
结论:
- 硫化学在彗星和彗星前物质中起着至关重要的作用.
- 含有硫化 (H2S) 的混合冰的辐射可以启动形成这些有机硫化合物的反应.
- 未来使用詹姆斯·韦伯太空望远镜的观测可以描述其他冰体上的类似材料.
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