Mars Odyssey Epithermal Neutron Data overlayed on MGS/MOLA Topography Data (Flyover, Unsmoothed)

  • Released Friday, May 31, 2002
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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.

Flyover of Mars false color (epithermal neutron) globe

False color (epithermal neutron) view of Mars at the equator

False color (epithermal neutron) view of Mars at the equator

False color (epithermal neutron) view of Mars at the south pole

False color (epithermal neutron) view of Mars at the south pole

False color (epithermal neutron) view of Mars at the equator

False color (epithermal neutron) view of Mars at the equator

False color (epithermal neutron) view of Mars at the north pole

False color (epithermal neutron) view of Mars at the north pole

Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio

This page was originally published on Friday, May 31, 2002.
This page was last updated on Wednesday, May 3, 2023 at 1:57 PM EDT.

Missions

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Datasets used in this visualization

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