File:Water equivalent hydrogen abundance in the lower latitudes of Mars 01.jpg
From Infogalactic: the planetary knowledge core
Size of this preview: 800 × 533 pixels. Other resolutions: 320 × 213 pixels | 3,187 × 2,125 pixels.
Original file (3,187 × 2,125 pixels, file size: 2.25 MB, 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.
Licensing
Lua error in package.lua at line 80: module 'strict' not found.
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 04:11, 15 January 2017 | 3,187 × 2,125 (2.25 MB) | 127.0.0.1 (talk) | 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. |
- You cannot overwrite this file.
File usage
The following page links to this file: