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The 67P/Churyumov–Gerasimenko observation campaign in support of the Rosetta mission

机译:67P / Churyumov–Gerasimenko观察运动以支持罗塞塔任务

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摘要

We present a summary of the campaign of remote observations that supported the European Space Agency's Rosetta mission. Telescopes across the globe (and in space) followed comet 67P/Churyumov–Gerasimenko from before Rosetta's arrival until nearly the end of the mission in September 2016. These provided essential data for mission planning, large-scale context information for the coma and tails beyond the spacecraft and a way to directly compare 67P with other comets. The observations revealed 67P to be a relatively ‘well-behaved’ comet, typical of Jupiter family comets and with activity patterns that repeat from orbit to orbit. Comparison between this large collection of telescopic observations and the in situ results from Rosetta will allow us to better understand comet coma chemistry and structure. This work is just beginning as the mission ends—in this paper, we present a summary of the ground-based observations and early results, and point to many questions that will be addressed in future studies.This article is part of the themed issue ‘Cometary science after Rosetta’.
机译:我们提供了支持欧洲航天局罗塞塔号任务的远程观测运动的摘要。从罗塞塔号到达之前到2016年9月任务结束之前,全球(及太空)望远镜一直跟踪着67P /丘留莫夫-格拉西缅科彗星。这些望远镜为任务计划提供了必要的数据,为昏迷提供了大范围的背景信息,并提供了尾巴以外的信息飞船,以及直接将67P与其他彗星进行比较的一种方法。观测结果表明67P是相对“行为良好”的彗星,是木星家族彗星的典型特征,其活动模式在轨道之间不断重复。将大量望远镜观测资料与Rosetta的原位结果进行比较,可以使我们更好地了解彗星彗形象差和结构。这项工作只是在任务结束时才开始–在本文中,我们将对地面观测和早期结果进行总结,并指出许多将在未来研究中解决的问题。本文是主题课题“罗塞塔之后的彗星科学。

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