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Twelve orbits a day provided the Mars Global Surveyor MOC wide angle cameras a global snapshot of 

weather patterns across the planet in April, 1999. Here, bluish-white water ice clouds hang above the 

Tharsis volcanoes. This computer generated image was created by wrapping a global map onto a sphere. 

The center of this sphere is 15 degrees North latitude, 90 degrees West longitude. This perspective rotates 

the south pole (which has no data coverage in the original map) away from our field of view.

                                                                                                                                         South Candor Chasma   Candor Chasm's geomorphology 

is complex, shaped by tectonics, mass wasting, wind, and perhaps by water and volcanism. (Courtesy USGS)     

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  This mosaic of Mars is similar to the view you 

would see from a spacecraft. The center of the scene shows the entire Valles Marineris canyon system, 

over 4000 km (2486 mi) long and up to 7 km (5 mi) deep. It extends from Noctis Labyrinthus, the arcuate 

system of graben on the west side, to the chaotic terrain on the east side. Many ancient river channels 

begin from the chaotic terrain and north-central canyons and run north. Three Tharsis volcanoes are 

visible to the west (dark red spots). They rise 10 to 18 km (6 to 11 mi) above the Tharsis Plateau, attaining 

elevations of 18 to 26 km (11 to 16 mi).                                              Return to Solar System