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The CRISM, a mineral mapping instrument on NASA's Mars Reconnaissance Orbiter, began observing Mars after its lens cover was opened on Sept. 27, 2006.
The CRISM, a mineral mapping instrument on NASA's Mars Reconnaissance Orbiter, began observing Mars after its lens cover was opened on Sept. 27, 2006.

New Spectrometer Begins its Global Map of Mars

NASA's Mars rover Opportunity edged closer to the top of the 'Duck Bay' alcove along the rim of 'Victoria Crater' (overnight Sept. 27 to Sept. 28), and gained this vista of the crater. 3D glasses are necessary to view this image.
NASA's Mars rover Opportunity edged closer to the top of the 'Duck Bay' alcove along the rim of 'Victoria Crater' (overnight Sept. 27 to Sept. 28), and gained this vista of the crater. 3D glasses are necessary to view this image.

'Victoria Crater' from 'Duck Bay' (Stereo)

On Feb. 19, 2005, NASA's Mars Exploration Rover Opportunity had completed a drive of 124 meters (407 feet) across the rippled flatland of the Meridiani Planum region. 3-D glasses are necessary to view this image.
On Feb. 19, 2005, NASA's Mars Exploration Rover Opportunity had completed a drive of 124 meters (407 feet) across the rippled flatland of the Meridiani Planum region. 3-D glasses are necessary to view this image.

Opportunity View on Sol 397 (3-D)

This anaglyph from the base of 'Burns Cliff' in the inner wall of 'Endurance Crater' combines several frames taken by Opportunity's navigation camera during the NASA rover's 280th martian day (Nov. 6, 2004). 3D glasses are necessary to view this image.
This anaglyph from the base of 'Burns Cliff' in the inner wall of 'Endurance Crater' combines several frames taken by Opportunity's navigation camera during the NASA rover's 280th martian day (Nov. 6, 2004). 3D glasses are necessary to view this image.

Along Endurance Crater's Inner Wall (3-D Anaglyph)

This 3-D cylindrical-perspective mosaic was created from navigation camera images that NASA's Mars Exploration Rover Spirit captured on on sol 100. 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 100. 3D glasses are necessary to view this image.

Spirit's View on Sol 100 (3-D)

This image taken by the microscopic imager on NASA's Mars Exploration Rover Spirit shows the powdery soil of Mars in 3-D. 3D glasses are necessary to view this image.
This image taken by the microscopic imager on NASA's Mars Exploration Rover Spirit shows the powdery soil of Mars in 3-D. 3D glasses are necessary to view this image.

Martian Soil in 3-D

This anaglyph from NASA's Mars Exploration Rover, Spirit, shows the rover's lander and, in the background, the surrounding martian terrain. 3D glasses are necessary to view this image.
This anaglyph from NASA's Mars Exploration Rover, Spirit, shows the rover's lander and, in the background, the surrounding martian terrain. 3D glasses are necessary to view this image.

Martian Landscape in 3-D

Dust-covered rocks can be seen in this portion of the 3D image taken by the panoramic camera on NASA's Mars Exploration Rover Spirit. 3D glasses are necessary to view this image.
Dust-covered rocks can be seen in this portion of the 3D image taken by the panoramic camera on NASA's Mars Exploration Rover Spirit. 3D glasses are necessary to view this image.

Shrouded in Dust

This image from NASA's Mars Odyssey spacecraft shows fractures within the volcanic plains south of Elysium Mons.
This image from NASA's Mars Odyssey spacecraft shows fractures within the volcanic plains south of Elysium Mons.

Cerberus Rupes

This image from NASA's Mars Odyssey of lava flows around the large scarp of Olympus Mons reveals textures characteristic of the variable surface roughness associated with different lava flows in this region.
This image from NASA's Mars Odyssey of lava flows around the large scarp of Olympus Mons reveals textures characteristic of the variable surface roughness associated with different lava flows in this region.

Lava Flows around Olympus Mons

Hills abound in this portion of Mars imaged by NASA's Mars Odyssey that shows the Vastitas Borealis region of the high northern plains. These hills are part of Scandia Colles.
Hills abound in this portion of Mars imaged by NASA's Mars Odyssey that shows the Vastitas Borealis region of the high northern plains. These hills are part of Scandia Colles.

Bumpy Terrain

This image is a mosaic of day and night infrared images of Melas Chasma taken by NASA's Mars Odyssey spacecraft. The daytime temperatures range from approximately -35 degrees Celsius (-31 degrees Fahrenheit) to -5 degrees Celsius (23 degrees Fahrenheit).
This image is a mosaic of day and night infrared images of Melas Chasma taken by NASA's Mars Odyssey spacecraft. The daytime temperatures range from approximately -35 degrees Celsius (-31 degrees Fahrenheit) to -5 degrees Celsius (23 degrees Fahrenheit).

Long Range View of Melas Chasma

The scoured grooves in the catastrophic outflow channels shown in this image from NASA's Mars Odyssey spacecraft formed hundreds of million of years ago and have the appearance of wood grain. They now host dune-like ripples of windblown material.
The scoured grooves in the catastrophic outflow channels shown in this image from NASA's Mars Odyssey spacecraft formed hundreds of million of years ago and have the appearance of wood grain. They now host dune-like ripples of windblown material.

Kasei Vallis

This image from NASA's Mars Odyssey is located in Meroe Patera, which is a small region within Syrtis Major Planitia. Syrtis Major is a low-relief shield volcano whose lava flows make up a plateau more than 1,000 km (about 620 miles) across.
This image from NASA's Mars Odyssey is located in Meroe Patera, which is a small region within Syrtis Major Planitia. Syrtis Major is a low-relief shield volcano whose lava flows make up a plateau more than 1,000 km (about 620 miles) across.

Meroe Patera

The jumbled, chaotic terrain in this NASA Mars Odyssey image may represent a source region for the Reull Vallis, one of the larger channel systems in the southern hemisphere of Mars.
The jumbled, chaotic terrain in this NASA Mars Odyssey image may represent a source region for the Reull Vallis, one of the larger channel systems in the southern hemisphere of Mars.

Reull Vallis Source Region

This image to the east of Tharsis Tholus from NASA's Mars Odyssey spacecraft shows one of many vast fields of lava flows produced by the great Tharsis volcanoes.
This image to the east of Tharsis Tholus from NASA's Mars Odyssey spacecraft shows one of many vast fields of lava flows produced by the great Tharsis volcanoes.

Lava Flows in Eastern Tharsis

This image of Tharsis Rise from NASA's Mars Odyssey shows a series of linear features called graben, which are associated with crustal extension resulting in up and down blocks of crust that run perpendicular to the direction of the extension.
This image of Tharsis Rise from NASA's Mars Odyssey shows a series of linear features called graben, which are associated with crustal extension resulting in up and down blocks of crust that run perpendicular to the direction of the extension.

Tharsis Rise Graben

The rugged, arcuate rim of the 90 km crater Reuyl dominates this NASA Mars Odyssey image. Reuyl crater is at the southern edge of a region known to be blanketed in thick dust based on its high albedo (brightness) and low thermal inertia values.
The rugged, arcuate rim of the 90 km crater Reuyl dominates this NASA Mars Odyssey image. Reuyl crater is at the southern edge of a region known to be blanketed in thick dust based on its high albedo (brightness) and low thermal inertia values.

Reuyl Crater Dust Avalanches

Observations by NASA's Mars Odyssey spacecraft show views of the polar regions of Mars in thermal neutrons (top) and epithermal neutrons (bottom). In these maps, deep blue indicates a low amount of neutrons and red indicates a high amount.
Observations by NASA's Mars Odyssey spacecraft show views of the polar regions of Mars in thermal neutrons (top) and epithermal neutrons (bottom). In these maps, deep blue indicates a low amount of neutrons and red indicates a high amount.

Polar Maps of Thermal and Epithermal Neutrons

The 'Mini Matterhorn' is a 3/4 meter rock immediately east-southeast of NASA's Mars Pathfinder lander. 3D glasses are necessary to identify surface detail.
The 'Mini Matterhorn' is a 3/4 meter rock immediately east-southeast of NASA's Mars Pathfinder lander. 3D glasses are necessary to identify surface detail.

Super Resolution Anaglyph of Mini-Matterhorn

NASA's Mars Reconnaissance Orbiter has detected widespread deposits of glacial ice in the mid-latitudes of Mars. This map of a region known as Deuteronilus Mensae, in the northern hemisphere, shows locations of the detected ice deposits in blue.
NASA's Mars Reconnaissance Orbiter has detected widespread deposits of glacial ice in the mid-latitudes of Mars. This map of a region known as Deuteronilus Mensae, in the northern hemisphere, shows locations of the detected ice deposits in blue.

Glacial Ice Deposits in Mid-Latitudes of Mars

This view of the American flag medallion on NASA's Mars rover Curiosity was taken by the rover's MAHLI camera during the 44th Martian sol on Sept. 19, 2012. The flag is one of four 'mobility logos' placed on the rover's mobility rocker arms.
This view of the American flag medallion on NASA's Mars rover Curiosity was taken by the rover's MAHLI camera during the 44th Martian sol on Sept. 19, 2012. The flag is one of four 'mobility logos' placed on the rover's mobility rocker arms.

Curiosity's Stars and Stripes

A sea of dark dunes, sculpted by the wind into long lines, surrounds the northern polar cap covering an area as big as Texas in this false-color image from NASA's Mars Odyssey, the longest-working Mars spacecraft in history.
A sea of dark dunes, sculpted by the wind into long lines, surrounds the northern polar cap covering an area as big as Texas in this false-color image from NASA's Mars Odyssey, the longest-working Mars spacecraft in history.

Mars Odyssey All Stars: Polar Dunes

As crater size increases, craters become more complex. This moderate size crater contains a central peak, created by rebound of molten material just following the impact. This image was captured by NASA's Mars Odyssey on Sept. 8, 2010.
As crater size increases, craters become more complex. This moderate size crater contains a central peak, created by rebound of molten material just following the impact. This image was captured by NASA's Mars Odyssey on Sept. 8, 2010.

Central Peak Crater

This wind eroded crater is located between Eumenides and Gordii Dorsa. The ejecta of the crater is more resistant to the wind than the surrounding materials in this image from NASA's Mars Odyssey.
This wind eroded crater is located between Eumenides and Gordii Dorsa. The ejecta of the crater is more resistant to the wind than the surrounding materials in this image from NASA's Mars Odyssey.

Wind Effects

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