Lunar Prospector data support the contention that water ice reservoirs exis
t in the permanently shaded craters near the lunar poles. Yet the question
remains whether the detected hydrogen abundance is actually water ice or is
hydrogen in some other form. Present plans call for a controlled impact of
Lunar Prospector into a polar crater at the end of July, 1999, in an attem
pt to liberate a small amount of water vapor that may be detected by ground
- and space-based observatories. A positive spectral detection of water vap
or or its photo-dissociated byproduct, OH, would be definite proof of the p
resence of water ice in the regolith. The following represents both an anal
ysis of this method of searching for water ice as well as an announcement t
o the observing community of the event.