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File:PIA04907 Water Mass Map from Neutron Spectrometer.jpg|left|thumb|800x800px|Water abundance from the Mars Odyssey gamma ray spectrometer. This map shows the estimated lower limit of the water content of the upper meter of Martian soil.
File:PIA04907 Water Mass Map from Neutron Spectrometer.jpg|left|thumb|800x800px|This map shows the estimated lower limit of the water content of the upper meter of Martian soil. The estimates are derived from the hydrogen abundance measured by the neutron spectrometer component of the gamma ray spectrometer suite on NASA's Mars Odyssey spacecraft.


rect 70 80 2370 200 [[Mare Boreum quadrangle|Mare Boreum]]
rect 70 80 2370 200 [[Mare Boreum quadrangle|Mare Boreum]]

Revision as of 18:27, 25 January 2020

Mare BoreumLyot CraterHecates TholusDiacriaArcadiaMare AcidaliumIsmenius LacusCasiusCebreniaOlympus MonsValles MarinerisNoctis LabyrinthusElysium MonsAscraeus MonsPavonis MonsArsia MonsMa'adim Vallis & Gusev craterGale CraterAmazonisTharsisLunae PalusOxia PalusArabiaSyrtis MajorAmenthesElysiumMemnoniaPhoenicis LacusCopratesMargaritifer SinusSinus SabaeusIapygiaMare TyrrhenumAeolisPhaethontisThaumasiaArgyreNoachisHellasEridaniaMare Australe
This map shows the estimated lower limit of the water content of the upper meter of Martian soil. The estimates are derived from the hydrogen abundance measured by the neutron spectrometer component of the gamma ray spectrometer suite on NASA's Mars Odyssey spacecraft.

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General map

Exploration

Volcanoes and Craters

Quadrangles

Geological map

Water abundance from the Mars Odyssey Neutron spectrometer
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