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Field geology on the Moon: Some lessons learned from the exploration of the Haughton impact structure, Devon Island, Canadian High Arctic

机译:月球上的现场地质:从加拿大高北极地区德文岛(Devon Island)的霍顿(Haughton)撞击结构探索中获得的一些经验教训

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摘要

With the prospect of humans returning to Moon by the end of the next decade, considerable attention is being paid to technologies required to transport astronauts to the lunar surface and then to be able to carry out surface science. Recent and ongoing initiatives have focused on scientific questions to be asked. In contrast, few studies have addressed how these scientific priorities will be achieved. In this contribution, we provide some of the lessons learned from the exploration of the Haughton impact structure, an ideal lunar analogue site in the Canadian Arctic. Essentially, by studying how geologists carry out field science, we can provide guidelines for lunar surface operations. Our goal in this contribution is to inform the engineers and managers involved in mission planning, rather than the field geology community. Our results show that the exploration of the Haughton impact structure can be broken down into 3 distinct phases: (1) reconnaissance; (2) systematic regional-scale mapping and sampling; and (3) detailed local-scale mapping and sampling. This break down is similar to the classic scientific method practiced by field geologists of regional exploratory mapping followed by directed mapping at a local scale, except that we distinguish between two different phases of exploratory mapping. Our data show that the number of stops versus the number of samples collected versus the amount of data collected varied depending on the mission phase, as does the total distance covered per EVA. Thus, operational scenarios could take these differences into account, depending on the goals and duration of the mission. Important lessons learned include the need for flexibility in mission planning in order to account for serendipitous discoveries, the highlighting of key "science supersites" that may require return visits, the need for a rugged but simple human-operated rover, laboratory space in the habitat, and adequate room for returned samples, both in the habitat and in the return vehicle. The proposed set of recommendations ideally should be tried and tested in future analogue missions at terrestrial impact sites prior to planetary missions.
机译:随着人类在下一个十年期末重返月球的前景,人们将注意力集中在将宇航员运送到月球表面然后进行表面科学所需的技术上。最近和正在进行的举措都集中在要提出的科学问题上。相反,很少有研究探讨如何实现这些科学优先事项。在这项贡献中,我们提供了从探索加拿大北极地区理想的月球模拟场“霍顿”撞击结构中学到的一些经验教训。本质上,通过研究地质学家如何进行野外科学,我们可以为月球表面作业提供指导。我们为此做出贡献的目标是告知参与任务计划的工程师和经理,而不是现场地质界。我们的结果表明,对霍顿撞击结构的探索可以分为三个不同的阶段:(1)侦察; (2)系统的区域规模制图和抽样; (3)详细的当地比例尺制图和抽样。这种分解类似于区域地质勘测的野外地质学家所采用的经典科学方法,然后是局部规模的定向勘测,只是我们区分了勘探勘测的两个不同阶段。我们的数据表明,停站数与收集的样本数与收集的数据量随任务阶段的不同而变化,每个EVA覆盖的总距离也有所不同。因此,根据任务的目标和持续时间,作战方案可以考虑到这些差异。汲取的重要经验教训包括:为应对偶然发现而需要灵活执行任务计划;突出显示可能需要回访的关键“科学超级站点”;需要坚固但简单的人工漫游车;在栖息地需要实验室空间,并在栖息地和返还媒介中留有足够的返还样品空间。理想情况下,建议的建议集应该在未来的模拟飞行中在行星飞行之前在地面撞击地点进行尝试和测试。

著录项

  • 来源
    《Planetary and space science》 |2010年第4期|p.646-657|共12页
  • 作者单位

    Departments of Earth Sciences/Physics and Astronomy, University of Western Ontario, 1757 Richmond Street, London, ON, Canada N6A 5B7;

    rnMars Institute, SETI Institute, and NASA Ames Research Center, Moffett Field, CA 94035-1000, USA;

    rnCentre for Earth, Planetary, Space and Astronomical Research, Open University, Milton Keynes, MK7 6AA, UK;

    rnCentre for Earth, Planetary, Space and Astronomical Research, Open University, Milton Keynes, MK7 6AA, UK NASA Coddard Space Flight Center, Mail Code 693, Creenbelt, MD 20771, USA;

    rnNASA Ames Research Center, Moffett Field, CA 94035-1000, USA;

    rnDepartment of Mathematics and Statistics, Simon Eraser University, Burnaby, BC, Canada V5A 1S6;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

    moon; human exploration; apollo; analogues;

    机译:月亮;人类探索;阿波罗类似物;

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