Abstract
AbstractThe lunar permanently shadowed regions (PSRs) are expected to host large quantities of water-ice, which are key for sustainable exploration of the Moon and beyond. In the near future, NASA and other entities plan to send rovers and humans to characterize water-ice within PSRs. However, there exists only limited information about the small-scale geomorphology and distribution of ice within PSRs because the orbital imagery captured to date lacks sufficient resolution and/or signal. In this paper, we develop and validate a new method of post-processing LRO NAC images of PSRs. We show that our method is able to reveal previously unseen geomorphological features such as boulders and craters down to 3 meters in size, whilst not finding evidence for surface frost or near-surface ice. Our post-processed images significantly facilitate the exploration of PSRs by reducing the uncertainty of target selection and traverse/mission planning.
Funder
Max Planck Institute for Solar System Research
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy,General Biochemistry, Genetics and Molecular Biology,General Chemistry
Reference69 articles.
1. National Aeronautics and Space Administration. Artemis III science definition team report. Report No. NASA/SP-20205009602. (NASA, 2020).
2. National Aeronautics and Space Administration. NASA’s plan for sustained lunar exploration and development. https://www.nasa.gov/sites/default/files/atoms/files/a_sustained_lunar_presence_nspc_report4220final.pdf (2020).
3. Watson, K., Murray, B. & Brown, H. On the possible presence of ice on the Moon. J. Geophys. Res. 66, 1598–1600 (1961).
4. Arnold, J. R. Ice in the lunar polar regions. J. Geophys. Res. 84, 5659–5668 (1979).
5. Feldman, W. C. et al. Evidence for water ice near the lunar poles. J. Geophys.l Res. 106, 23231–23251 (2011).
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