The Clementine I satellite had a radar experiment which measured the reflectivity of the Moon's surface directly below the orbiting space craft. A few of the orbits passed directly over a couple of craters on the Moon's south polar region which have been known for some years to have portions of their crater floors in total darkness during the entire lunar month. Even the yearly libration effect has been unable to bring these regions into sunlight, so it is believed they have been in complete shadow for thousands or even billions of years. Clementine discovered that these same shadowed areas coincided with radar reflections that are normally found associated with rock that contains ice on the Earth, but the discovery on the Moon only involved a single pass worth of data so confirmation is desperately needed before we get too excited. Still, NASA is now planning to send a Lunar Ice Discovery mission to the Moon which will cost about $200 million, and it will include a lunar rover robot weighing about 290 kilograms which will cover 10 kilometers per day looking for surface water and taking sub-surface core samples every now and then. It is believed that as much as 10 billion cubic meters of water could exist there. A NASA mission called Lunar Prospector will be launched in September 1997 to confirm or refute Clementine's discovery.
Update (May, 2000).
By now you will have heard that NASA's Lunar Prospector did in fact confirm the Clementine discovery of ice locked in the lunar soil in dark craters near the poles. The evidence appears to be water-tight in so far as the strength of the detection is concerned. Future expeditions to the Moon will hone-in on this region not only to determine just how much ice is there, but its composition, abundance and utility for fuel and human consumption. Here is the news release by NASA about this discovery and other matters:
RELEASE: 99-119
NO WATER ICE DETECTED FROM LUNAR PROSPECTOR IMPACT
The controlled crash of NASA's Lunar Prospector spacecraft into a crater near the south pole of the Moon on July 31 produced no observable signature of water, according to scientists digging through data from Earth- based observatories and spacecraft such as the Hubble Space Telescope.
This lack of physical evidence leaves open the question of whether ancient cometary impacts delivered ice that remains buried in permanently shadowed regions of the Moon, as suggested by the large amounts of hydrogen measured indirectly from lunar orbit by Lunar Prospector during its main mapping mission. Research group leaders from the University of Texas at Austin announced their results today at the annual meeting of the American Astronomical Society's Division for Planetary Sciences meeting in Padua, Italy.
In a low-budget attempt to wring one last bit of scientific productivity from the low-cost Lunar Prospector mission, NASA worked with engineers and astronomers at the University of Texas to precisely crash the barrel-shaped spacecraft into a specific shadowed crater. NASA accepted the team's proposal based on successful scientific peer review of the idea and the pending end of the spacecraft's useful life, although the chances of positive detection of water were judged to be less than 10 percent.
Worldwide observations of the crash were focused primarily on using sensitive spectrometers tuned to look for the ultraviolet emission lines expected from the hydroxyl (OH) molecules that should be a by-product of ] any icy rock and dust kicked up by the impact of the 354- pound spacecraft.
"There are several possible explanations why we did not detect any water signature, and none of them can really be discounted at this time," said Dr. Ed Barker, assistant director of the university's McDonald Observatory at UT Austin, who coordinated the observing campaign. These explanations include:
* the spacecraft might have missed the target area;
* the spacecraft might have hit a rock or dry soil at the target site;
* water molecules may have been firmly bound in rocks as hydrated mineral as opposed to existing as free ice crystals, and the crash lacked enough energy to separate water from hydrated minerals;
* no water exists in the crater and the hydrogen detected by the Lunar Prospector spacecraft earlier is simply pure hydrogen;
* studies of the impact's physical outcome were inadequate;
* the parameters used to model the plume that resulted from the impact were inappropriate;
* the telescopes used to observe the crash, which have a very small field of view, may not have been pointed correctly;
* water and other materials may not have risen above the crater wall or otherwise were directed away from the telescopes' view.
Although the crash did not confirm the existence of water ice on the Moon, "this high-risk, potentially high- payoff experiment did produce several benefits," said Dr. David Goldstein, the aerospace engineer who led the UT Austin team. "We now have experience building a remarkably complex, coordinated observing program with astronomers across the world, we established useful upper limits on the properties of the Moon's natural atmosphere, and we tested a possible means of true 'lunar prospecting' using direct impacts."
Lunar Prospector was launched on Jan. 6, 1998, from Cape Canaveral Air Station, FL, aboard an Athena 2 rocket. In March 1998, mission scientists announced their first tentative findings of the presence of water ice in shadowed craters near the Moon's south and north poles. They estimated later that up to six billion metric tons of water ice may be buried in these craters under about 18 inches of soil, in more concentrated deposits than originally thought. However, the evidence was indirect, they cautioned, based on reasonable scientific assumptions given the levels of hydrogen detected, from which water ice is inferred.
Since then, Prospector data have also been used to develop the first precise gravity map of the entire lunar surface. While the Moon's magnetic field is relatively weak, Prospector has confirmed the presence of local magnetic fields that create the two smallest magnetospheres in the Solar System. Another scientific landmark is the assembly of the first global maps of the Moon's elemental composition.
The $63 million Lunar Prospector mission was led by Dr. Alan Binder of the Lunar Research Institute, Tucson, AZ, and managed by NASA's Ames Research Center in Moffett Field, CA. It was built by Lockheed Martin Missiles & Space, Sunnyvale, CA. Other participating organizations included the Department of Energy's Los Alamos National Laboratory, NM, and NASA's Goddard Space Flight Center, Greenbelt, MD, and Jet Propulsion Laboratory, Pasadena, CA.
Copyright 1997 Dr. Sten Odenwald
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