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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

Located at 64 degrees south latitude, the dunes in Wegener Crater are just beginning to lose their frost cover. The 'salt and pepper' appearance is bright frost and dark dune on the crater floor in this image from NASA's Mars Odyssey.
Located at 64 degrees south latitude, the dunes in Wegener Crater are just beginning to lose their frost cover. The 'salt and pepper' appearance is bright frost and dark dune on the crater floor in this image from NASA's Mars Odyssey.

Wegener Crater Dunes

Dunes are found on the floor of this unnamed crater located on the margin between Arabia Terra and Terra Sabaea in this image from NASA's 2001 Mars Odyssey spacecraft.
Dunes are found on the floor of this unnamed crater located on the margin between Arabia Terra and Terra Sabaea in this image from NASA's 2001 Mars Odyssey spacecraft.

Crater Dunes

This infrared image, taken by NASA's 2001 Mars Odyssey spacecraft, shows the feature called 'White Rock.' The feature is dark, indicating that it is cooler than the surroundings.
This infrared image, taken by NASA's 2001 Mars Odyssey spacecraft, shows the feature called 'White Rock.' The feature is dark, indicating that it is cooler than the surroundings.

Pollack Crater

Small channels dissect the rim of Bakhuysen Crater in Noachis Terra as seen by NASA's 2001 Mars Odyssey.
Small channels dissect the rim of Bakhuysen Crater in Noachis Terra as seen by NASA's 2001 Mars Odyssey.

Channels in Noachis Terra

This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows terminating at the foot of canyon walls in Echus Chasma. These lava flows are also fractured into large plates in this region.
This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows terminating at the foot of canyon walls in Echus Chasma. These lava flows are also fractured into large plates in this region.

Echus Chasma

This image from NASA's 2001 Mars Odyssey spacecraf shows part of Aspledon Undae, one of several dune fields near the north pole. The term Undae means dunes.
This image from NASA's 2001 Mars Odyssey spacecraf shows part of Aspledon Undae, one of several dune fields near the north pole. The term Undae means dunes.

Polar Dunes

This image shows a different part of Utopia Planitia than yesterday's image. Both are marked with hundreds of dust devil tracks as seen by by NASA's 2001 Mars Odyssey spacecraft.
This image shows a different part of Utopia Planitia than yesterday's image. Both are marked with hundreds of dust devil tracks as seen by by NASA's 2001 Mars Odyssey spacecraft.

More Dust Devils

This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a portion of the lava flows associated with Arsia Mons.
This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a portion of the lava flows associated with Arsia Mons.

Arsia Mons Flows

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the margin of Olympia Undae.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the margin of Olympia Undae.

Olympia Undae

This image shows the location (green) where scientists estimate NASA's Curiosity rover landed on Mars within Gale Crater, based on images from the Mars Descent Imager (MARDI).
This image shows the location (green) where scientists estimate NASA's Curiosity rover landed on Mars within Gale Crater, based on images from the Mars Descent Imager (MARDI).

Narrowing in on Curiosity's Landing Site

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in an unnamed crater in Sisyphi Planum.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in an unnamed crater in Sisyphi Planum.

Dunes in Sisyphi Planum

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