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彗星67P/Churyumov-Gerasimenko核上的暴露水冰
G Filacchione1, M C De Sanctis1, F Capaccioni1
1INAF-IAPS, Istituto di Astrofisica e Planetologia Spaziali, Rome, Italy.
Nature
|January 14, 2016
概括
科学家在67P/Churyumov-Gerasimenko彗星上的碎片中发现了毫米大小的水冰粒. 这些发现表明进化过程形成了复杂的涂层,不一定是形成的全球层.
科学领域:
- 彗星科学
- 星球科学
- 天体生物学
背景情况:
- 彗星67P/Churyumov-Gerasimenko的昏迷中大量存在水蒸气,水冰是彗星核的主要组成部分.
- 彗星表面的暴露水冰区域很少被观察到,核通常被脱水,耐火和有机材料覆盖.
研究的目的:
- 在彗星67P/Churyumov-Gerasimenko表面识别和描述水冰.
- 研究观察到的水冰粒的形成机制和影响.
主要方法:
- 红外光谱被用来检测彗星核心的特定区域的水冰.
- 进行了定量分析以确定水冰颗粒的数量和大小.
主要成果:
- 在Imhotep地区的碎片中发现了水冰,
- 检测到毫米大小的纯水冰粒, 比之前观察到的要大得多.
- 这些大颗粒的存在表明它们是通过富含冰层的蒸汽扩散或烧结形成的.
结论:
- 观察到的水冰分布和颗粒大小表明了核的上层进化过程.
- 彗星核可以形成复杂的覆盖物,
- 这些发现挑战了从彗星形成时代的全球分层的必要性,以解释观察到的层状结构.
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