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Robotics Institute Special Seminar, Thursday, September 10, 1998
Robotics Institute Carnegie Mellon University Pittsburgh PA 15213-3891 412/268-8525 . 412/268-5576 (fax)
Warning
Latest Results from the Lunar Prospector Satellite and their
Implications for Lunar Rover Exploration
Place and Time
Abstract In March, mission scientists reported a water signal with a minimum abundance of one percent by weight of water ice in lunar soil corresponding to an estimated total of 300 million metric tons of ice. These conservative numbers were based on graphs of neutron spectrometer data, which showed distinctive dips over the poles, a telltale signature of the presence of water ice. Subsequent analysis, combined with improved lunar models, shows conclusively that there is hydrogen at the Moon's poles. Though other explanations are possible, this data has been interpreted as an indication of significant quantities of water ice are located in permanently shadowed craters in both lunar polar regions. Dr. Binder, joint with Carnegie Mellon University, has an active proposal to NASA to send a robot to the surface of the Moon which would definitively confirm or refute the existence of lunar ice. The robot, equipped with a cryogenic drill and a Thermal and Evolved Gas Analyzer (TEGA), would venture into permanent shadow to acquire soil samples for onboard analysis. The drill, would be able to acquire soil samples in cryogenic conditions down to one meter below the surface. The TEGA, which is scheduled to fly on the upcoming Mars 98 lander, would accept samples from the drill and detect whether they contain traces of ice. The TEGA is capable of unambiguously detecting water and other volatiles in very small concentratations.
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