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This is a small volcano superimposed on the flanks of a larger one of the Cerberus Tholi.
Small Floral-Shaped Volcano
This picture was taken during the Martian summer with only small patches of ice remaining at the surface; they show up as bright, somewhat blue, spots on slopes that provide some shading from the Sun.
Sand Dunes Near the North Pole
This crater, formed in 2008, exposes shallow, clean ice that is not uncommon in the middle-to-high latitudes on Mars.
Icy New Impact
This unnamed impact crater is about 8 kilometers in diameter and contains numerous gullies.
Bright Gully Deposits on Mars
A towering dust devil, casts a serpentine shadow over the Martian surface in this image acquired by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
The Serpent Dust Devil of Mars
This image, taken Jan. 26, 2012, shows NASA's no-longer-active Phoenix Mars Lander spacecraft after its second Martian arctic winter.
Phoenix Lander After Second Martian Winter
This image, taken Jan. 26, 2012, shows the back shell of NASA's Phoenix Mars Lander spacecraft after its second Martian arctic winter.
Phoenix Back Shell After Second Martian Winter
Near the lower left corner of this view is the three-petal lander platform that NASA's Mars Exploration Rover Spirit drove off in January 2004.
Spirit Lander and Bonneville Crater in Color
This enhanced-color image shows sand dunes trapped in an impact crater in Noachis Terra, Mars.
Dunes in Noachis Terra Region of Mars
This scene is from early spring in the northern hemisphere of Mars. These dunes are covered with a layer of seasonal carbon dioxide ice (dry ice).
Edge of North Polar Erg
Recent small craters discovered by the High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter expose buried ice in the middle latitudes of Mars.
Fresh Crater Revealing Buried Ice
A dune in the northern polar region of Mars shows significant changes between two images taken on June 25, 2008 and May 21, 2010 by NASA's Mars Reconnaissance Orbiter.
Movement in Martian Dune Field
A rippled dune front in Herschel Crater on Mars moved an average of about one meter (about one yard) between March 3, 2007 and December 1, 2010, as seen in these images from NASA's Mars Reconnaissance Orbiter.
Rippling Dune Front in Herschel Crater on Mars
A rippled dune front in Herschel Crater on Mars moved an average of about two meters (about two yards) between March 3, 2007 and December 1, 2010, as seen in these images from NASA's Mars Reconnaissance Orbiter.
Rippling Dune Front in Herschel Crater on Mars
The eastern margin of a rippled dune in Herschel Crater on Mars moved an average distance of three meters (about three yards) between March 3, 2007 and December 1, 2010, as seen by NASA's Mars Reconnaissance Orbiter.
Shifting Sand in Herschel Crater
A rippled patch of sand in Becquerel Crater on Mars moved about two meters (about two yards) between November 24, 2006 and September 5, 2010, as observed in these images taken by NASA's Mars Reconnaissance Orbiter.
Blowing in the Martian Wind
Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
Clay Minerals in Craters and Escarpments on Mars (Figure 2)
Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
Clay Minerals in Craters and Escarpments on Mars (Figure 4)
Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
Clay Minerals in Craters and Escarpments on Mars (Figure 3)
Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
Clay Minerals in Craters and Escarpments on Mars (Figure 1)
Impact cratering and erosion combine to reveal the composition of the Martian underground by exposing materials from the subsurface.
Clay Minerals in Craters and Escarpments on Mars
This series of images shows warm-season features that might be evidence of salty liquid water active on Mars today.
Warm-Season Flows on Slope in Horowitz Crater (Nine-Image Sequence)
This back and forth comparison shows changes that occurred in a gully on a south-facing slope in middle southern latitudes of Mars.
Changes in a Gully in a Mars Crater (Two-Image Comparison)
This series of images shows warm-season features that might be evidence of salty liquid water active on Mars today.
Warm-Season Flows in Well-Preserved Crater in Terra Sirenum (Six-Image Sequence)
This series of images shows warm-season features that might be evidence of salty liquid water active on Mars today.
Warm-Season Flows on Steep Slope in Slope in Terra Cimmeria (Eight-Image Sequence)
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