File:Water equivalent hydrogen abundance in the lower latitudes of Mars 01.jpg
Water_equivalent_hydrogen_abundance_in_the_lower_latitudes_of_Mars_01.jpg (800 × 533 pixels, file size: 103 KB, MIME type: image/jpeg)
Summary
This map displays the proportion of water ice present in the upper meter of the Martian surface within 60 degrees of the equator. 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. Date 24 July 2003, 09:41:17 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
Image credit: NASA/JPL/Feldman, W. et al.
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Creative Commons Attribution-ShareAlike 4.0 (More Details)
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 07:49, 31 October 2018 | | 800 × 533 (103 KB) | Suitupandshowup (talk | contribs) | This map displays the proportion of water ice present in the upper meter of the Martian surface within 60 degrees of the equator. The percentages are derived through stochiometric calculations based on epithermal neutron fluxes. These fluxes were detec... |
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