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This view in the Meridiani Planum region of Mars shows the region around NASA's Mars Exploration Rover Opportunity. The rover, in the seventh year of its exploration of Mars, is in the upper central portion of the image.
This view in the Meridiani Planum region of Mars shows the region around NASA's Mars Exploration Rover Opportunity. The rover, in the seventh year of its exploration of Mars, is in the upper central portion of the image.

Orbital View of Opportunity's Region

The dunes in this image are located on the floor of an unnamed crater in Tyrrhena Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
The dunes in this image are located on the floor of an unnamed crater in Tyrrhena Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Dunes in Tyrrhena Terra

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Nili Fossae.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Nili Fossae.

Nili Fossae - False Color

NASA's rover Curiosity took this close-up view of 'Tintina' showing interesting linear textures in the bright white material on the rock.
NASA's rover Curiosity took this close-up view of 'Tintina' showing interesting linear textures in the bright white material on the rock.

Close-up View of Broken Mars Rock 'Tintina'

The faint dark lines in this image captured by NASA's 2001 Mars Odyssey spacecraft are caused by dust devils. As the dust devil travels along the surface it scours away the loose surface dust, revealing the darker surface beneath.
The faint dark lines in this image captured by NASA's 2001 Mars Odyssey spacecraft are caused by dust devils. As the dust devil travels along the surface it scours away the loose surface dust, revealing the darker surface beneath.

Dust Devil Tracks

This image from an animation shows a patch of sandstone scrubbed with the Dust Removal Tool, a wire-bristle brush, on NASA's Curiosity Mars rover. This rock target is called 'Windjana,' after a gorge in Western Australia.
This image from an animation shows a patch of sandstone scrubbed with the Dust Removal Tool, a wire-bristle brush, on NASA's Curiosity Mars rover. This rock target is called 'Windjana,' after a gorge in Western Australia.

Martian Sandstone Target 'Windjana' Before and After Brushing

The volcanic flows in image from NASA's 2001 Mars Odyssey spacecraft are located south of Ascraeus Mons and east of Pavonis Mons.
The volcanic flows in image from NASA's 2001 Mars Odyssey spacecraft are located south of Ascraeus Mons and east of Pavonis Mons.

Tharsis Flows

NASA's Mars Exploration Rover Opportunity captured this view of a wee crater, informally named 'Skylab,' along the rover's route. Based on the estimated age of the area's sand ripples, the crater was likely formed within the past 100,000 years.
NASA's Mars Exploration Rover Opportunity captured this view of a wee crater, informally named 'Skylab,' along the rover's route. Based on the estimated age of the area's sand ripples, the crater was likely formed within the past 100,000 years.

Opportunity Beside a Small, Young Crater

A small channel enters this unnamed crater in Arabia Terra. There appears to be a small fan or delta formed where the channel meets the crater floor. This image was captured by NASA's Mars Odyssey on June 15, 2010.
A small channel enters this unnamed crater in Arabia Terra. There appears to be a small fan or delta formed where the channel meets the crater floor. This image was captured by NASA's Mars Odyssey on June 15, 2010.

Crater in Arabia

This image captured by NASA's Mars Reconnaissance Orbiter shows the edge of a dark dune field on the floor of Proctor Crater, a 150 kilometer diameter crater in the southern highlands of Mars.
This image captured by NASA's Mars Reconnaissance Orbiter shows the edge of a dark dune field on the floor of Proctor Crater, a 150 kilometer diameter crater in the southern highlands of Mars.

Proctor Crater Dune Field

NASA's Mars Exploration Rover used its panoramic camera to record this view of the rim of a crater about 65 kilometers (40 miles) in the distance, on the southwestern horizon. This crater, Bopolu, is about 19 kilometers (12 miles) in diameter.
NASA's Mars Exploration Rover used its panoramic camera to record this view of the rim of a crater about 65 kilometers (40 miles) in the distance, on the southwestern horizon. This crater, Bopolu, is about 19 kilometers (12 miles) in diameter.

Rim of Bopolu Crater Far to the Southwest of Opportunity

This mosaic of images of the region around NASA's Mars Exploration Rover Opportunity shows the relative locations of several craters, including Endeavour, in the Meridiani Planum region of Mars.
This mosaic of images of the region around NASA's Mars Exploration Rover Opportunity shows the relative locations of several craters, including Endeavour, in the Meridiani Planum region of Mars.

Opportunity Amid Mars Craters

This image from NASA's Mars Odyssey shows part of the eastern region of Aram Chaos.
This image from NASA's Mars Odyssey shows part of the eastern region of Aram Chaos.

Aram Chaos

This image captured by NASA's 2001 Mars Odyssey spacecraft location is slightly east of Monday's image. In this image the polar scarp (called Tenuis Rupes) bisects the image.
This image captured by NASA's 2001 Mars Odyssey spacecraft location is slightly east of Monday's image. In this image the polar scarp (called Tenuis Rupes) bisects the image.

Tenuis Rupes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows another unnamed crater near the north pole with dunes on its floor.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows another unnamed crater near the north pole with dunes on its floor.

Crater Dunes

As the season changes from spring to summer, the dunes surrounding the north polar cap become darker and darker as seen by NASA's 2001 Mars Odyssey spacecraft.
As the season changes from spring to summer, the dunes surrounding the north polar cap become darker and darker as seen by NASA's 2001 Mars Odyssey spacecraft.

Polar Dunes

This image from NASA's 2001 Mars Odyssey shows a portion of Rhabon Vallis, a channel south of Uranius Mons.
This image from NASA's 2001 Mars Odyssey shows a portion of Rhabon Vallis, a channel south of Uranius Mons.

Rhabon Vallis

This image from NASA's rover Opportunity shows mostly a portion of Endeavour's western rim (left); a paler-looking terrain on the horizon beyond Endeavour (right) is part of a thick deposit of material ejected by the impact that excavated Iazu Crater.
This image from NASA's rover Opportunity shows mostly a portion of Endeavour's western rim (left); a paler-looking terrain on the horizon beyond Endeavour (right) is part of a thick deposit of material ejected by the impact that excavated Iazu Crater.

Super-Resolution View of Endeavour Rim, Sol 2239

NASA's 2001 Mars Odyssey captured this region of Mars which has been eroded by the wind. Linear hills called yardangs indicate the wind direction, which varies in this area of Medusae Fossae.
NASA's 2001 Mars Odyssey captured this region of Mars which has been eroded by the wind. Linear hills called yardangs indicate the wind direction, which varies in this area of Medusae Fossae.

Wind Effects

This graphic depicts the Mars Climate Sounder instrument on NASA's Mars Reconnaissance Orbiter measuring the temperature of a cross section of the Martian atmosphere as the orbiter passes above the south polar region.
This graphic depicts the Mars Climate Sounder instrument on NASA's Mars Reconnaissance Orbiter measuring the temperature of a cross section of the Martian atmosphere as the orbiter passes above the south polar region.

Scanning Martian Atmospheric Temperatures (Graphic)

Light blue clouds fill Coprates Chasma on Mars, part of Valles Marineris, the vast 'Grand Canyon of Mars.' The clouds are mostly ice crystals and they appear blue in color in this image from NASA's Mars Odyssey.
Light blue clouds fill Coprates Chasma on Mars, part of Valles Marineris, the vast 'Grand Canyon of Mars.' The clouds are mostly ice crystals and they appear blue in color in this image from NASA's Mars Odyssey.

Mars Odyssey View of Morning Clouds in Canyon

This image was taken by NASA's Mars Reconnaissance Orbiter spacecraft, in one of the regions on Mars well-known for its viscous flow features (VFF), which are massive flowing deposits believed to be composed of a mixture of ice and dust.
This image was taken by NASA's Mars Reconnaissance Orbiter spacecraft, in one of the regions on Mars well-known for its viscous flow features (VFF), which are massive flowing deposits believed to be composed of a mixture of ice and dust.

A Tale of Two Flows

The windstreaks in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Terra Sabaea.
The windstreaks in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Terra Sabaea.

Windstreaks

This unnamed crater in Terra Cimmeria is not as round in shape as other craters. Major landslides have occurred on the crater rim, resulting in the final shape as seen by NASA's 2001 Mars Odyssey spacecraft.
This unnamed crater in Terra Cimmeria is not as round in shape as other craters. Major landslides have occurred on the crater rim, resulting in the final shape as seen by NASA's 2001 Mars Odyssey spacecraft.

Out of Round

This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering and linear ridges in Cavi Angusti. This region is near the south polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering and linear ridges in Cavi Angusti. This region is near the south polar cap.

Cavi Angusti

Currently displaying images 2126-2150 of 4027
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