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No evidence for thick deposits of ice at the lunar south pole

Author

Listed:
  • Donald B. Campbell

    (Cornell University)

  • Bruce A. Campbell

    (Smithsonian Institution)

  • Lynn M. Carter

    (Smithsonian Institution)

  • Jean-Luc Margot

    (Cornell University)

  • Nicholas J. S. Stacy

    (Defence Science and Technology Organization)

Abstract

Lunar ice on the rocks The rim of the Shackleton crater at the lunar south pole is a candidate crash site for NASA's LCROSS probe (Lunar CRater Observation and Sensing Satellite), due to launch in 2008. The plume of debris kicked up by the crash is to be analysed in the hope that it will reveal the water thought to be there. Suggestions of lunar ice date from 1996 when data from the Clementine spacecraft gave some indications of the presence of ice on crater walls at the south pole. Now using high-resolution radar imagery, the radar scattering parameter thought indicative of thick ice deposits has been found also to match radar echoes from the rock-strewn walls and ejecta of young impact craters at all lunar latitudes. There is no evidence for thick ice, though there could be grains of water ice spread more thinly through the lunar soil.

Suggested Citation

  • Donald B. Campbell & Bruce A. Campbell & Lynn M. Carter & Jean-Luc Margot & Nicholas J. S. Stacy, 2006. "No evidence for thick deposits of ice at the lunar south pole," Nature, Nature, vol. 443(7113), pages 835-837, October.
  • Handle: RePEc:nat:nature:v:443:y:2006:i:7113:d:10.1038_nature05167
    DOI: 10.1038/nature05167
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