Illumination conditions of the south pole of the Moon derived using Kaguya topography

Details Illumination conditions of the south pole of the Moon derived using Kaguya topography Illumination conditions of the south pole of the Moon derived using Kaguya topography

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010icar..208..558b&link_type=abstract

Icarus, Volume 208, Issue 2, p. 558-564.

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Scientific paper

We have used the Kaguya laser altimeter-derived topography to conduct a comprehensive study of the illumination conditions at the Moon’s south pole. We have determined, by comparing simulated and actual Clementine images, that the Kaguya topography can be used to generate realistic illumination conditions. We generated an average illumination map for the year 2020 for the lunar south pole region. From this we identified the areas that receive the most illumination. The place receiving the most illumination (86% of the year) is located close to the rim of Shackleton crater at 88.74°S 124.5°E. However two other areas, less than 10 km apart from each other, are collectively lit for 94% of the year. We found that sites exist near the south pole that are continuously lit for several months during summer. We were also able to map the locations and durations of eclipse periods for these areas. Finally we analyzed the seasonal variations in lighting conditions, from summer to winter, for key areas near the south pole. We conclude that areas exist near the south pole that have illumination conditions that make them ideal candidates as future outpost sites.

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