Radar data evaporate Moon's ice sheets
The thick ice sheets many astronomers thought were hidden in some of the Moon's craters almost certainly do not exist, according to observations from the world's biggest radar.
The 300-metre Arecibo dish in Puerto Rico was used to bounce radio waves into dark craters at the Moon's north and south poles. Sunlight never reaches the bottom of these craters, meaning ice could survive there.
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But the new Arecibo investigation has come to a very different conclusion. Team leader Bruce Campbell, at the Smithsonian Institution, Washington DC, told New Scientist: "There are no thick ice deposits in the areas we observed." The researchers surveyed 20 per cent of the Moon's shadowed regions.
One crater, called Shackleton, did return a strong echo, mimicking the Clementine data. But so did another crater that is not permanently shadowed, meaning it could not be caused by ice.
"We think that the rough, tilted walls of those craters were producing the strong reflections, not ice," Campbell explains.
The new data does not rule out ice altogether. The experiment would only detect ice sheets more than a metre thick. Any thinner deposits, or small ice crystals distributed in the lunar dust, would have remained undetected.