Difference between revisions of "Mars atlas water"

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rect 70 80 2370 200 [[Mare Boreum quadrangle|Mare Boreum]]
 
rect 70 80 2370 200 [[Mare Boreum quadrangle|Mare Boreum]]
  
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rect 1380 310 1420 360[[Lyot Crater]]
 
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rect 2160 490 2190 520[[Hecates Tholus]]
 
  
 
rect 70 200 445 520[[Diacria quadrangle|Diacria]]
 
rect 70 200 445 520[[Diacria quadrangle|Diacria]]
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rect 1600 200 1990 520[[Casius quadrangle|Casius]]
 
rect 1600 200 1990 520[[Casius quadrangle|Casius]]
 
rect 1990 200 2370 520[[Cebrenia quadrangle|Cebrenia]]
 
rect 1990 200 2370 520[[Cebrenia quadrangle|Cebrenia]]
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rect 320 560 400 630[[Olympus Mons]]
 
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rect 620 760 940 830[[Valles Marineris|Valles Marineris]]
 
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rect 540 720 620 800[[Noctis Labyrinthus|Noctis Labyrinthus]]
 
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rect 2130 540 2190 590[[Elysium Mons|Elysium Mons]]
 
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rect 535 625 565 660[[Ascraeus Mons|Ascraeus Mons]]
 
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rect 480 700 510 740[[Pavonis Mons|Pavonis Mons]]
 
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rect 435 750 470 795[[Arsia Mons|Arsia Mons]]
 
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rect 2080 740 2120 770[[Gale Crater]]
 
  
 
rect 70 520 340 720[[Amazonis quadrangle|Amazonis]]
 
rect 70 520 340 720[[Amazonis quadrangle|Amazonis]]

Revision as of 15:52, 26 January 2020

Mare BoreumDiacriaArcadiaMare AcidaliumIsmenius LacusCasiusCebreniaAmazonisTharsisLunae 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.

View a map of:

General map

Exploration

Volcanoes and Craters

Quadrangles

Geological map

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