Evidence Mounts for Ice in Shackleton Crater
June 21, 2012: According to data from NASA's Lunar Reconnaissance Orbiter (LRO), ice may make up as much as 22 percent of the surface material in Shackleton crater at the Moon's south pole.The huge crater, named after the Antarctic explorer Ernest Shackleton, is two miles deep and more than 12 miles wide. The small tilt of the lunar spin axis means Shackleton's interior is permanently dark and very cold.. Researchers have long thought that ice might collect there.
When a team of NASA and university scientists used LRO's laser altimeter to examine the floor of Shackleton crater, they found it to be brighter than the floors of other nearby craters around the South Pole. This is consistent with the presence of small amounts of reflective ice preserved by cold and darkness. The findings are published in today's edition of the journal Nature.
This visualization, created using Lunar Reconnaissance Orbiter
laser altimeter data, offers a view of Shackleton Crater located in the
south pole of the moon. Play it
"The crater's interior is extremely rugged," said Maria Zuber, the team's lead investigator from the Massachusetts Institute of Technology in Cambridge in Mass. "It would not be easy to crawl around in there."
In this laser elevation map of Shackleton crater, false colors
indicate height, with blue lowest and red highest. Credit: NASA/Zuber,
M.T. et al., Nature, 2012
"The brightness measurements have been puzzling us since two summers ago," said Gregory Neumann of NASA's Goddard Space Flight Center in Greenbelt, Md., a co-author on the paper.
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."
For more information on LRO and the Lunar Orbiter Laser Altimeter, visit:
http://lunar.gsfc.nasa.gov
Production editor: Dr. Tony Phillips | Credit: Science@NASA
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