Smith, A.; Crawford, I. A.; Ball, A. J.; Barber, S. J.; Church, P.; Gao, Y.; Gowen, R. A.; Griffiths, A.; Hagermann, A.; Pike, W. T.; Phipps, A.; Sheridan, S.; Sims, M. R.; Talboys, D. L. and Wells, N.
PDF (Not Set)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
|Google Scholar:||Look up in Google Scholar|
Introduction: While the surface missions to the Moon of the 1960s and 1970s achieved a great deal, scientifically a great deal was also left unresolved. The recent plethora of lunar missions (flown or proposed) reflects resurgence in interest in the Moon, not only in its own right, but also as a record of the formation of the Earth-Moon System and the interplanetary environment at 1 AU. Results from orbiter missions have indicated the possible presense of ice within permanently shaded craters at the lunar poles  – a situation that, if confirmed, will have profound impacts on lunar exploration.
|Item Type:||Conference Item|
|Extra Information:||Abstract number 1238|
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||Karen Guyler|
|Date Deposited:||31 Mar 2008|
|Last Modified:||02 Aug 2016 14:17|
|Share this page:|
Download history for this item
These details should be considered as only a guide to the number of downloads performed manually. Algorithmic methods have been applied in an attempt to remove automated downloads from the displayed statistics but no guarantee can be made as to the accuracy of the figures.