Researchers   estimate ice content of crater at Moon's south pole
  In addition to the possible evidence of ice, the scientists' map   of Shackleton revealed a remarkably preserved crater that has remained   relatively unscathed since its formation more than 3 billion years   ago.
By NASA Headquarters, Washington, D.C., NASA's Goddard Space   Flight Center, Greenbelt, Maryland — Published: June 21, 2012                  |         NASA's Lunar Reconnaissance Orbiter (LRO)         spacecraft has returned data that indicate ice may make up as much as 22         percent of the surface material in a crater located on the Moon's south         pole.  Elevation (left) and shaded relief (right) image of         Shackleton, a 12.5-mile-diameter (20 kilometers) permanently shadowed         crater adjacent to the lunar south pole. The structure of the crater's         interior was revealed by a digital elevation model constructed from over 5         million elevation measurements from the Lunar Orbiter Laser         Altimeter. Credit: NASA/Zuber, M.T. et al., Nature,         2012 
 A team of NASA and university scientists using laser         light from LRO's laser altimeter examined the floor of Shackleton Crater.         They found that the crater's floor is brighter than those of other nearby         craters, which is consistent with the presence of small amounts of ice.         This information will help researchers understand crater formation and         study other uncharted areas of the Moon.
 
 "The brightness         measurements have been puzzling us since two summers ago," said Gregory         Neumann of NASA's Goddard Space Flight Center in Greenbelt, Maryland.         "While the distribution of brightness was not exactly what we had         expected, practically every measurement related to ice and other volatile         compounds on the Moon is surprising, given the cosmically cold         temperatures inside its polar craters."
 
 The spacecraft mapped         Shackleton Crater with unprecedented detail, using a laser to illuminate         the crater's interior and measure its albedo, or natural reflectance. The         laser light measures to a depth comparable to its wavelength, or about a         micron. That represents a millionth of a meter, or less than one         ten-thousandth of an inch. The team also used the instrument to map the         relief of the crater's terrain based on the time it took for laser light         to bounce back from the Moon's surface. The longer it took, the lower the         terrain's elevation.
 
 In addition to the possible evidence of ice,         the group's map of Shackleton revealed a remarkably preserved crater that         has remained relatively unscathed since its formation more than 3 billion         years ago. The crater's floor is itself pocked with several small craters,         which may have formed as part of the collision that created         Shackleton.
 
 The crater, named after the Antarctic explorer Ernest         Shackleton, is 2 miles (3 kilometers) deep and more than 12 miles (19         kilometers) wide. Like several craters at the Moon's south pole, the small         tilt of the lunar spin axis means Shackleton Crater's interior is         permanently dark, and therefore extremely cold.
 
 "The crater's         interior is extremely rugged," said Maria Zuber from the Massachusetts         Institute of Technology in Cambridge. "It would not be easy to crawl         around in there."
 
 While the crater's floor was relatively         bright, Zuber and her colleagues observed that its walls were even         brighter. The finding was at first puzzling. Scientists had thought that         if ice were anywhere in a crater, it would be on the floor where no direct         sunlight penetrates. The upper walls of Shackleton Crater are occasionally         illuminated, which could evaporate any ice that accumulates. A theory         offered by the team to explain the puzzle is that "moonquakes"— seismic         shaking brought on by meteorite impacts or gravitational tides from Earth         — may have caused Shackleton's walls to slough off older darker soil,         revealing newer, brighter soil underneath. Zuber's team's         ultra-high-resolution map provides strong evidence for ice on both the         crater's floor and walls.
 
 "There may be multiple explanations         for the observed brightness throughout the crater," said Zuber. "For         example, newer material may be exposed along its walls, while ice may be         mixed in with its floor."
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