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This daytime infrared image taken by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field located on the floor of Proctor Crater.
This daytime infrared image taken by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field located on the floor of Proctor Crater.

Proctor Crater Dunes

This image, taken by NASA's Mars Odyssey, shows dunes of several sizes in Terra Cimmeria.
This image, taken by NASA's Mars Odyssey, shows dunes of several sizes in Terra Cimmeria.

Terra Cimmeria Dunes

This view, taken by NASA's Mars Reconnaissance Orbiter from Martian orbit, shows a pale circular shape in the center is a low plateau called
This view, taken by NASA's Mars Reconnaissance Orbiter from Martian orbit, shows a pale circular shape in the center is a low plateau called

Orbital View of Spirit at 'Troy'

NASA's Mars Exploration Rover Opportunity used its navigation camera to take the images combined into this 360-degree polar view of the rover's surroundings on the 1,950th Martian day, or sol, of its surface mission (July 19, 2009).
NASA's Mars Exploration Rover Opportunity used its navigation camera to take the images combined into this 360-degree polar view of the rover's surroundings on the 1,950th Martian day, or sol, of its surface mission (July 19, 2009).

Opportunity's Surroundings on Sol 1950 (Polar)

NASA's Opportunity had driven 72.3 meters southward (237 feet) that sol. Engineers drove the rover backward as a strategy to counteract an increase in the amount of current drawn by the drive motor of the right-front wheel. This is a cylindric projection.
NASA's Opportunity had driven 72.3 meters southward (237 feet) that sol. Engineers drove the rover backward as a strategy to counteract an increase in the amount of current drawn by the drive motor of the right-front wheel. This is a cylindric projection.

Opportunity's View After 72-Meter Drive, Sol 1912

The Thermal and Electrical Conductivity Probe on NASA's Phoenix Mars Lander detected small and variable amounts of water in the Martian soil.
The Thermal and Electrical Conductivity Probe on NASA's Phoenix Mars Lander detected small and variable amounts of water in the Martian soil.

Adsorbed Water Illustration

This graph presents simplified data from overnight measurements by the Thermal and Electrical Conductivity Probe on NASA's Phoenix Mars Lander from noon of the mission's 70th Martian day, or sol, to noon the following sol (Aug. 5 to Aug. 6, 2008).
This graph presents simplified data from overnight measurements by the Thermal and Electrical Conductivity Probe on NASA's Phoenix Mars Lander from noon of the mission's 70th Martian day, or sol, to noon the following sol (Aug. 5 to Aug. 6, 2008).

Overnight Changes Recorded by Phoenix Conductivity Probe

The Surface Stereo Imager onboard NASA's Phoenix Mars Lander captures a scene with three different filters. The images are sent to Earth in black and white and the color is added by mission scientists.
The Surface Stereo Imager onboard NASA's Phoenix Mars Lander captures a scene with three different filters. The images are sent to Earth in black and white and the color is added by mission scientists.

How Phoenix Creates Color Images (Animation)

This 360-degree view, called the 'McMurdo' panorama, comes from the panoramic camera aboard NASA's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as 'Low Ridge.' 3D glasses are necessary.
This 360-degree view, called the 'McMurdo' panorama, comes from the panoramic camera aboard NASA's Mars Exploration Rover Spirit. From April through October 2006, Spirit has stayed on a small hill known as 'Low Ridge.' 3D glasses are necessary.

'McMurdo' Panorama from Spirit's 'Winter Haven' (Stereo)

This anaglyph from from NASA's Mars Exploration Rover Opportunity is of 'Victoria crater' is looking southeast from 'Duck Bay' towards the dramatic promontory called 'Cabo Frio.' 3D glasses are necessary to view this image.
This anaglyph from from NASA's Mars Exploration Rover Opportunity is of 'Victoria crater' is looking southeast from 'Duck Bay' towards the dramatic promontory called 'Cabo Frio.' 3D glasses are necessary to view this image.

Layers of 'Cabo Frio' in 'Victoria Crater' (Stereo)

This 3-D cylindrical-perspective mosaic was created from navigation camera images that NASA's Mars Exploration Rover Spirit captured on on sol 103. 3D glasses are necessary to view this image.
This 3-D cylindrical-perspective mosaic was created from navigation camera images that NASA's Mars Exploration Rover Spirit captured on on sol 103. 3D glasses are necessary to view this image.

Riding the Rim of 'Endurance' (3-D)

This 3D anaglyph, from NASA's Mars Exploration Rover Spirit, shows a microscopic image taken of the rock called Adirondack. 3D glasses are necessary to view this image.
This 3D anaglyph, from NASA's Mars Exploration Rover Spirit, shows a microscopic image taken of the rock called Adirondack. 3D glasses are necessary to view this image.

Adirondack Post-Drill (3-D)

This 3D anaglyph, from NASA's Mars Exploration Rover Spirit, shows a microscopic image taken of the rock called Adirondack. 3D glasses are necessary to view this image.
This 3D anaglyph, from NASA's Mars Exploration Rover Spirit, shows a microscopic image taken of the rock called Adirondack. 3D glasses are necessary to view this image.

A Clean Adirondack (3-D)

Heavy water ice clouds almost completely obscure the surface in Vastitas Borealis, as seen in this image from NASA's Mars Odyssey spacecraft.
Heavy water ice clouds almost completely obscure the surface in Vastitas Borealis, as seen in this image from NASA's Mars Odyssey spacecraft.

Ice Clouds

The relatively flat floor and terrace walls of this impact crater imaged by NASA's Mars Odyssey spacecraft suggest the crater was partly infilled with sediment and subsequently eroded to its present day form.
The relatively flat floor and terrace walls of this impact crater imaged by NASA's Mars Odyssey spacecraft suggest the crater was partly infilled with sediment and subsequently eroded to its present day form.

Impact Crater

This image from NASA's Mars Odyssey spacecraft shows the eastern portion of a region on Mars called Hesperia Planum. Immediately visible in the image is the dark barchan type dunes that are being blown against the southeast wall of the crater.
This image from NASA's Mars Odyssey spacecraft shows the eastern portion of a region on Mars called Hesperia Planum. Immediately visible in the image is the dark barchan type dunes that are being blown against the southeast wall of the crater.

Hesperia Planum

This image from NASA's Mars Odyssey spacecraft of the northern plains of Mars shows a surface texture of hundreds of small mounds and numerous small impact craters.
This image from NASA's Mars Odyssey spacecraft of the northern plains of Mars shows a surface texture of hundreds of small mounds and numerous small impact craters.

Late Afternoon Sun

This image from NASA's Mars Odyssey spacecraft was acquired of Candor Chasma within Valles Marineris and shows the effects of erosion on a sequence of dramatically layered rocks.
This image from NASA's Mars Odyssey spacecraft was acquired of Candor Chasma within Valles Marineris and shows the effects of erosion on a sequence of dramatically layered rocks.

Candor Chasma on Mars, in Color

The force of moving water from a flood carved these teardrop-shaped islands within Granicus Valles, imaged here by NASA's Mars Odyssey spacecraft. The orientation of the islands can be used as an indicator of the direction the water flowed.
The force of moving water from a flood carved these teardrop-shaped islands within Granicus Valles, imaged here by NASA's Mars Odyssey spacecraft. The orientation of the islands can be used as an indicator of the direction the water flowed.

Granicus Valles

The channels and impact crater rim shown in this NASA Mars Odyssey image provide insight to the forces that have sculpted the surface within the extensive Reull Vallis network.
The channels and impact crater rim shown in this NASA Mars Odyssey image provide insight to the forces that have sculpted the surface within the extensive Reull Vallis network.

Reull Vallis

This nighttime temperature image from NASA's Mars Odyssey spacecraft shows the ancient, heavily cratered surface of the highlands between Isidis and Elysium Planitia.
This nighttime temperature image from NASA's Mars Odyssey spacecraft shows the ancient, heavily cratered surface of the highlands between Isidis and Elysium Planitia.

Martian Highlands at Night in Infrared

With a location roughly equidistant between two of the largest volcanic constructs on the planet, the fate of the approximately 50 km (31 mile) impact crater in this image from NASA's Mars Odyssey was sealed. It has been buried to the rim by lava flows.
With a location roughly equidistant between two of the largest volcanic constructs on the planet, the fate of the approximately 50 km (31 mile) impact crater in this image from NASA's Mars Odyssey was sealed. It has been buried to the rim by lava flows.

Buried Crater

Kasei Valles is one of the largest outflow channels on Mars. This NASA Mars Odyssey image is of the northern branch of Kasei Valles and shows the channel floor and northern channel wall.
Kasei Valles is one of the largest outflow channels on Mars. This NASA Mars Odyssey image is of the northern branch of Kasei Valles and shows the channel floor and northern channel wall.

Kasei Valles

This image from NASA's Mars Odyssey shows Noctis Labyrinthus, a large valley system at the western end of the Valles Marineris canyon system notable for a pattern of intersecting valleys, which give it a maze-like appearance when viewed from above.
This image from NASA's Mars Odyssey shows Noctis Labyrinthus, a large valley system at the western end of the Valles Marineris canyon system notable for a pattern of intersecting valleys, which give it a maze-like appearance when viewed from above.

Noctis Labyrinthus

Dark streaks mark the inner rim of this unnamed crater in Terra Sabaea as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark streaks mark the inner rim of this unnamed crater in Terra Sabaea as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

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