Difference between revisions of "June 5, 2013"

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<em>image by [http://www.nasa.gov/multimedia/videogallery/index.html" rel="nofollow Goddard Visualization Lab] (NASA/GSFC)</em><br />
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<em>image by [http://www.nasa.gov/multimedia/videogallery/index.html Goddard Visualization Lab] (NASA/GSFC)</em><br />
 
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Did you know that one of the most important instruments on LRO is from Russia? The [http://l503.iki.rssi.ru/LEND-en.html" rel="nofollow Institute for Space Research] in Moscow supplied the Lunar Exploration Neutron Detector (LEND) that maps the distribution of hydrogen near the lunar surface. Cosmic rays striking the Moon dislodge neutrons from atoms in soils, and from the velocity of the neutrons hydrogen abundances as small as 100 ppm can be detected with a resolution of 5 km. The assumption is that the hydrogen maps are actually maps of the locations and quantities of near-surface water ice deposits. It was anticipated that ice would be localized to the bottoms of craters that were permanently shadoawed, but as the image above shows H concentrations also occur outside the permanently shadowed holes. The reasons for this are still a mystery but if true accessing water in regions not at the bottoms of permanently dark and hyper-cold craters should be technologically easier. <br />
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Did you know that one of the most important instruments on LRO is from Russia? The [http://l503.iki.rssi.ru/LEND-en.html Institute for Space Research] in Moscow supplied the Lunar Exploration Neutron Detector (LEND) that maps the distribution of hydrogen near the lunar surface. Cosmic rays striking the Moon dislodge neutrons from atoms in soils, and from the velocity of the neutrons hydrogen abundances as small as 100 ppm can be detected with a resolution of 5 km. The assumption is that the hydrogen maps are actually maps of the locations and quantities of near-surface water ice deposits. It was anticipated that ice would be localized to the bottoms of craters that were permanently shadoawed, but as the image above shows H concentrations also occur outside the permanently shadowed holes. The reasons for this are still a mystery but if true accessing water in regions not at the bottoms of permanently dark and hyper-cold craters should be technologically easier. <br />
 
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<em>[mailto:tychocrater@yahoo.com" rel="nofollow Chuck Wood]</em><br />
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<em>[mailto:tychocrater@yahoo.com Chuck Wood]</em><br />
 
PS: Note the spectacular shadow of Amundsen's rim at about 0:50 sec.<br />
 
PS: Note the spectacular shadow of Amundsen's rim at about 0:50 sec.<br />
 
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Revision as of 18:05, 11 January 2015

Blue Ice

<iframe width="853" height="480" src="//www.youtube.com/embed/qYW4rTrAA5I?rel=0" frameborder="0" allowfullscreen></iframe>
image by Goddard Visualization Lab (NASA/GSFC)

Did you know that one of the most important instruments on LRO is from Russia? The Institute for Space Research in Moscow supplied the Lunar Exploration Neutron Detector (LEND) that maps the distribution of hydrogen near the lunar surface. Cosmic rays striking the Moon dislodge neutrons from atoms in soils, and from the velocity of the neutrons hydrogen abundances as small as 100 ppm can be detected with a resolution of 5 km. The assumption is that the hydrogen maps are actually maps of the locations and quantities of near-surface water ice deposits. It was anticipated that ice would be localized to the bottoms of craters that were permanently shadoawed, but as the image above shows H concentrations also occur outside the permanently shadowed holes. The reasons for this are still a mystery but if true accessing water in regions not at the bottoms of permanently dark and hyper-cold craters should be technologically easier.

Chuck Wood
PS: Note the spectacular shadow of Amundsen's rim at about 0:50 sec.

Related Links
21st Century Atlas chart L4.

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