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彗星67P/Churyumov-Gerasimenko上的日间水冰周期
M C De Sanctis1, F Capaccioni1, M Ciarniello1
1Istituto di Astrofisica e Planetologia Spaziali - INAF, via del fosso del cavaliere 100, 00133 Rome, Italy.
彗星67P/Churyumov-Gerasimenko表现出表面水冰,随着太阳照射而循环出现和消失. 这种水循环影响彗星活动和表面演变.
科学领域:
- 星球科学
- 彗星科学
- 天体生物学
背景情况:
- 彗星核上有限的表面水冰对观察到的水脱气的解释提出了挑战.
- 彗星活动,就像9P/Tempel 1上的尘埃喷流,与暴露的冰相对应.
- 在67P/Churyumov-Gerasimenko上的日间活动变化与阳光照射的变化有关.
研究的目的:
- 研究67P/Churyumov-Gerasimenko彗星表面水冰的存在和行为.
- 了解太阳光照射与彗星水冰之间的关系.
- 确定表面水冰在彗星活动和演变中的作用.
主要方法:
- 彗星67P/Churyumov-Gerasimenko的表面观测
- 分析彗星活动的日间变化.
- 冰的存在与当地的照明条件的相关性
主要成果:
- 在彗星67P/Churyumov-Gerasimenko上进行了表面水冰的直接观测.
- 水冰表现出循环的模式,随着当地的照明出现和消失.
- 这提供了与太阳照明相关的局部活动源.
结论:
- 在彗星67P/Churyumov-Gerasimenko上证实了由太阳照射驱动的表面水循环.
- 这一过程有助于局部彗星活动.
- 水循环循环地改变了表面水冰的丰富性,影响了彗星的演化.
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