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[[Category:Mars Atlas]]
[[Category:Mars Atlas]]
[[File:Water_equivalent_hydrogen_abundance_in_the_lower_latitudes_of_Mars_01.jpg|alt=|left|frame|Water abundance from the Mars Odyssey Neutron spectrometer]]
 
[[File:Water equivalent hydrogen abundance in the lower latitudes of Mars 01.jpg|alt=|left|frame|Water equivalent hydrogen abundance in the lower latitudes of Mars from the Mars Odyssey Neutron spectrometer]]

Revision as of 18:30, 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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Geological map

Water equivalent hydrogen abundance in the lower latitudes of Mars from the Mars Odyssey Neutron spectrometer
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