Mars Global Surveyor (MGS)



The Spacecraft


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Read about the MGS Science Objectives here





A selection of images from MGS's Mars Orbiter Camera



Layered rock deep in martian crust




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Sedimentary Rocks




  West Candor Chasma
  (Mariner 9 and Viking)


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  West Candor Chasma
  (zoom with MOC)


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Groundwater, co2 and gullies





Groundwater may be the source for erosion in martian gullies. Another possibility is that under direct sunlight, CO2 frost incorporated into a martian sand dune could sublime. This CO2 gas may act to fluidize overlying sand, causing it to flow rather than avalanche, and thus create a gully.





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But when did that happen ?






 New gullies forming in the last 5 years
 (larger view)


   Full resolution image (3.5 MB)
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 New gullies forming in the last 5 years
 (already present on images of Feb. 21, 2004)


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  New Dune Gullies
  (larger view)


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  New Dune Gullies
  (detail)


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  Gullies With Light-Toned Deposits


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  Gullies and Avalanches


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See more than 100 gully pictures here.




Eberswalde delta





  Eberswalde delta (context map)


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  Eberswalde delta


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  River reconstruction


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  Only the 11 avulsions
  (Credit: J. P. Bhattacharya1)


  Close-up view of meanders


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  Close-up view of channels


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All the MOC pictures






See more than 212'000 images of
the Mars Orbiter Camera here.






Topographic maps of mars





  Topographic map


  Full resolution
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  Rectangular Projection


  Full resolution
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  Full resolution (15.9 MB)
  Full resolution with contours (15.7 MB)
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   Snow on Mars


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In a distant past, Mars may have had oceans



   What Mars might have looked like,
   ... with oceans !


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background photo: Gullies eroded into the wall of a meteor impact crater in Noachis Terra (Credit: MGS, NASA).
http://www.msss.com/mars_images/moc/june2000/scicover/index.html