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This stereo mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 93.3-meter (306-foot) drive east-northeastward on Oct. 6, 2010. 3D glasses are necessary to view this image.
This stereo mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 93.3-meter (306-foot) drive east-northeastward on Oct. 6, 2010. 3D glasses are necessary to view this image.

Opportunity's Eastward View After Sol 2382 Drive (Stereo)

This small unnamed channel is located in southern Tyrrhena Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
This small unnamed channel is located in southern Tyrrhena Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Channel

The interconnected collapse pits at the top of this image, taken by NASA's 2001 Mars Odyssey spacecraft, are part of Coprates Catena. Notice the dunes in the bottom of each pit.
The interconnected collapse pits at the top of this image, taken by NASA's 2001 Mars Odyssey spacecraft, are part of Coprates Catena. Notice the dunes in the bottom of each pit.

Coprates Catena

The streamlined islands in this image from NASA's Mars Odyssey are located in Maja Valles.
The streamlined islands in this image from NASA's Mars Odyssey are located in Maja Valles.

Maja Valles

This mosaic of images from NASA's Mars Exploration Rover Opportunity shows terrain that includes light-toned bedrock and darker ripples of wind-blown sand. Portions of Endeavour Crater's rim are visible in the horizon of this scene.
This mosaic of images from NASA's Mars Exploration Rover Opportunity shows terrain that includes light-toned bedrock and darker ripples of wind-blown sand. Portions of Endeavour Crater's rim are visible in the horizon of this scene.

Opportunity's Eastward View After Sol 2401 Drive

The tectonic fractures in this image captured by NASA's Mars Odyssey on July 8, 2010 are part of Aram Chaos.
The tectonic fractures in this image captured by NASA's Mars Odyssey on July 8, 2010 are part of Aram Chaos.

Aram Chaos

By repeated measurements of the concentration of methane in the atmosphere at Gale Crater, NASA's Curiosity Mars rover has detected long-term variation in background levels below one part per billion.
By repeated measurements of the concentration of methane in the atmosphere at Gale Crater, NASA's Curiosity Mars rover has detected long-term variation in background levels below one part per billion.

Methane Background Levels at Gale Crater, Mars

This mosaic of four images from NASA's Mars rover Curiosity shows detailed texture in a ridge that stands higher than surrounding rock. The rock is at a location called 'Darwin,' inside Gale Crater.
This mosaic of four images from NASA's Mars rover Curiosity shows detailed texture in a ridge that stands higher than surrounding rock. The rock is at a location called 'Darwin,' inside Gale Crater.

Close-up of Ridge in Rock Outcrop at Curiosity's 'Waypoint 1'

This image from NASA's 2001 Mars Odyssey spacecraft is of Lismore Crater. This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.
This image from NASA's 2001 Mars Odyssey spacecraft is of Lismore Crater. This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.

Lismore Crater

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small section of Samara Valles.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small section of Samara Valles.

Samara Valles

Several landslide deposits are visible in this image captured by NASA's 2001 Mars Odyssey spacecraft of an unnamed crater in Terra Cimmeria.
Several landslide deposits are visible in this image captured by NASA's 2001 Mars Odyssey spacecraft of an unnamed crater in Terra Cimmeria.

Landslides

Rock fins up to about 1 foot (30 centimeters) tall dominate this approximate true color scene from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Opportunity.
Rock fins up to about 1 foot (30 centimeters) tall dominate this approximate true color scene from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Opportunity.

Opportunity Eyes Rock Fins on Cape York, Sol 3058

This observation from NASA's Mars Reconnaissance Orbiter shows the edge of a dark dune field on the floor of Proctor Crater in the Southern highlands of Mars. The dark dunes are composed of basaltic sand that has collected on the bottom of the crater.
This observation from NASA's Mars Reconnaissance Orbiter shows the edge of a dark dune field on the floor of Proctor Crater in the Southern highlands of Mars. The dark dunes are composed of basaltic sand that has collected on the bottom of the crater.

Proctor Crater Dune Field

This set of images shows what might be hardware from the Soviet Union's 1971 Mars 3 lander, seen in a pair of images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
This set of images shows what might be hardware from the Soviet Union's 1971 Mars 3 lander, seen in a pair of images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.

Could This Be the Mars Soviet 3 Lander?

This image from NASA's Mars Global Surveyor and Mars Odyssey spacecraft shows the context for orbital observations of exposed rocks that had been buried on Mars. The area is dominated by the Huygens crater, which is about the size of Wisconsin.
This image from NASA's Mars Global Surveyor and Mars Odyssey spacecraft shows the context for orbital observations of exposed rocks that had been buried on Mars. The area is dominated by the Huygens crater, which is about the size of Wisconsin.

Nature's Drilling Exposes Deeply Buried Minerals

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

Syrtis Major - False Color

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

Gale Crater - False Color

This map shows the route driven by NASA's Curiosity Mars rover from the location where it landed in August 2012 to its location in September 2016 at 'Murray Buttes', and the path planned for reaching destination at lower Mount Sharp.
This map shows the route driven by NASA's Curiosity Mars rover from the location where it landed in August 2012 to its location in September 2016 at 'Murray Buttes', and the path planned for reaching destination at lower Mount Sharp.

Curiosity Destinations for Second Extended Mission

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Noachis Terra.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Noachis Terra.

Noachis Terra - False Color

These images at 'Garden City' from the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover indicate similarly dark material, but with very different chemistries, in mineral veins.
These images at 'Garden City' from the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover indicate similarly dark material, but with very different chemistries, in mineral veins.

Thick, Dark Veins at 'Garden City,' Mars

This non-circular pit seen in this image from NASA's Mars Reconnaissance Orbiter is due to a low angle impact from an asteroid or comet. The raised plateau west of the crater was where most of the impact debris landed.
This non-circular pit seen in this image from NASA's Mars Reconnaissance Orbiter is due to a low angle impact from an asteroid or comet. The raised plateau west of the crater was where most of the impact debris landed.

Martian Thunderbird

This image demonstrates how engineers place the drill carried by NASA's Mars rover Curiosity onto rock targets. They first set down the drill's two stabilizing prongs near the target, as shown by the dashed line.
This image demonstrates how engineers place the drill carried by NASA's Mars rover Curiosity onto rock targets. They first set down the drill's two stabilizing prongs near the target, as shown by the dashed line.

Checking Contact Points for Curiosity's Drill

This image shows the topography, with shading added, around the area where NASA's Curiosity rover landed. An alluvial fan, or fan-shaped deposit where debris spreads out downslope, has been highlighted in lighter colors for better viewing.
This image shows the topography, with shading added, around the area where NASA's Curiosity rover landed. An alluvial fan, or fan-shaped deposit where debris spreads out downslope, has been highlighted in lighter colors for better viewing.

Where Water Flowed Downslope

As northern spring progresses, clouds continue to cover large portions of the north polar region. This image captured by NASA's 2001 Mars Odyssey spacecraft.
As northern spring progresses, clouds continue to cover large portions of the north polar region. This image captured by NASA's 2001 Mars Odyssey spacecraft.

Polar Clouds

The many channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are volcanic collapse features on the southern flank of Ascraeus Mons.
The many channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are volcanic collapse features on the southern flank of Ascraeus Mons.

Ascraeus Mons

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