File:Water equivalent hydrogen abundance in the high latitudes of Mars.jpg

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English: This map displays the proportion of water ice present in the upper meter of the Martian surface within 30 degrees of the poles. The percentages are derived through stochiometric calculations based on epithermal neutron fluxes. These fluxes were detected by the Neutron Spectrometer aboard the 2001 Mars Odyssey spacecraft. For more information see Feldman, W. C., Prettyman, T. H., Maurice, S., et al., Global distribution of near-surface hydrogen on Mars: Journal of Geophysical Research: Planets, v. 109, E09006, doi:10.1029/2003JE002160.
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Source http://mars.jpl.nasa.gov/odyssey/gallery/latestimages/20030724a.html
Author Feldman, W.C., Prettyman, T.H., Maurice, S., et al., Los Alamos National Laboratory/JPL

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current04:41, 24 July 2013Thumbnail for version as of 04:41, 24 July 20133,187 × 2,125 (1.64 MB)DanHobley (talk | contribs)User created page with UploadWizard

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