Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Full Globe, Viking True Color)
- Visualizations by:
- Greg Shirah
- View full credits
Mars Odyssey's Gamma-ray spectrometer (GRS) instrument has detected large amounts of Hydrogen on Mars, particularly near the south pole. This is an indication that water ice exists in the upper meter of these areas of the Martian surface. The epithermal neutron data ranges from 0 to about 12 counts per second. The blue areas indicate high concentrations of Hydrogen (low epithermal neutron counts).
A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data.
A series of animations was generated to support a Space Science Update (SSU) on the topic. These animations were match-rendered with unsmoothed, smoothed, and Viking true-color data.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
Animator
- Greg Shirah (NASA/GSFC) [Lead]
Scientists
- James Garvin (NASA, Chief Scientist Goddard)
- William Boynton (The University of Arizona)
Missions
This visualization is related to the following missions:Datasets used in this visualization
MGS (Collected with the MOLA sensor)
Mars Odyssey (Collected with the GRS sensor)
Note: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.
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