2471 images found for "Mars" Wallpaper
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This is a picture of 'Block Island' an odd-shaped, dark rock, which may be a meteorite.
This is a picture of 'Block Island' an odd-shaped, dark rock, which may be a meteorite.

Block Island Close-up

This image of 'Block Island' was taken on July 28, 2009, with the front hazard-identification camera on NASA’s Mars Exploration Rover Opportunity.
This image of 'Block Island' was taken on July 28, 2009, with the front hazard-identification camera on NASA’s Mars Exploration Rover Opportunity.

Block Island in Sight

This scene combines seven frames taken by the navigation camera on NASA's Mars Exploration Rover Spirit during the 1,891st Martian day, or sol, of Spirit's mission on Mars (April 28, 2009).
This scene combines seven frames taken by the navigation camera on NASA's Mars Exploration Rover Spirit during the 1,891st Martian day, or sol, of Spirit's mission on Mars (April 28, 2009).

Spirit's View from "Troy"

This stereo scene combines frames taken by the navigation camera on NASA's Mars Exploration Rover Spirit during the 1,866th Martian day, or sol, of  Spirit's mission on Mars (April 3, 2009). You will need 3-D glasses to view this image.
This stereo scene combines frames taken by the navigation camera on NASA's Mars Exploration Rover Spirit during the 1,866th Martian day, or sol, of  Spirit's mission on Mars (April 3, 2009). You will need 3-D glasses to view this image.

Spirit's Look Ahead After Sol 1866 Drive (Stereo)

The robotic arm on NASA's Phoenix Mars Lander enlarged a trench beside a rock called 'Headless' on Sept. 20, 2008 in preparation for sliding the rock into the trench. 3D glasses are necessary to view this image.
The robotic arm on NASA's Phoenix Mars Lander enlarged a trench beside a rock called 'Headless' on Sept. 20, 2008 in preparation for sliding the rock into the trench. 3D glasses are necessary to view this image.

Preparation for Moving a Rock on Mars, Stereo View

This anaglyph, acquired by NASA's Phoenix Lander's Surface Stereo Imager on June 19, 2008, shows a view of the Martian surface near the lander. The trench shown here is informally called 'Snow White 1.' 3D glasses are necessary.
This anaglyph, acquired by NASA's Phoenix Lander's Surface Stereo Imager on June 19, 2008, shows a view of the Martian surface near the lander. The trench shown here is informally called 'Snow White 1.' 3D glasses are necessary.

Martian Surface as Seen by Phoenix

Images taken by NASA's Phoenix Mars Lander's Surface Stereo Imager, combined into a panoramic view looking north from the lander.
Images taken by NASA's Phoenix Mars Lander's Surface Stereo Imager, combined into a panoramic view looking north from the lander.

Phoenix Animation Looking North

This image taken by the Stereo Surface Imager aboard NASA's Phoenix Mars Lander focuses on items on the deck rather than the workspace or horizon on Sol 8.
This image taken by the Stereo Surface Imager aboard NASA's Phoenix Mars Lander focuses on items on the deck rather than the workspace or horizon on Sol 8.

Telltale Animation (Sol 8)

This image from NASA's Phoenix Mars Lander shows the spacecraft's robotic arm in its stowed configuration, with its biobarrier unpeeled. The arm is still folded up, with its
This image from NASA's Phoenix Mars Lander shows the spacecraft's robotic arm in its stowed configuration, with its biobarrier unpeeled. The arm is still folded up, with its

Ready to Unfurl

NASA's Mars Exploration Rover Opportunity used its navigation camera to take the images combined into this stereo view of the rover's surroundings. 3D glasses are necessary to identify surface detail.
NASA's Mars Exploration Rover Opportunity used its navigation camera to take the images combined into this stereo view of the rover's surroundings. 3D glasses are necessary to identify surface detail.

Opportunity's View, Sol 958 (Stereo)

Northern Impact

This stereo view shows the landscape surrounding NASA's Mars Exploration Rover Opportunity at the edge of 'Erebus Crater.' 3D glasses are necessary to view this image.
This stereo view shows the landscape surrounding NASA's Mars Exploration Rover Opportunity at the edge of 'Erebus Crater.' 3D glasses are necessary to view this image.

Erebus Panorama in Stereo

NASA's Mars Exploration Rover Spirit captured this view uphill toward 'Cumberland Ridge' on 'Husband Hill.' 3-D glasses are necessary to view this image.
NASA's Mars Exploration Rover Spirit captured this view uphill toward 'Cumberland Ridge' on 'Husband Hill.' 3-D glasses are necessary to view this image.

Spirit's View on Sol 390 (3-D)

This stereo view is from NASA's Mars Exploration Rover Spirit as it was investigating a rock called 'Mazatzal' on the rim of 'Bonneville Crater.' 3D glasses are necessary to view this image.
This stereo view is from NASA's Mars Exploration Rover Spirit as it was investigating a rock called 'Mazatzal' on the rim of 'Bonneville Crater.' 3D glasses are necessary to view this image.

A Rocky Rim Around 'Bonneville' in 3-D

This is the 3-D version of NASA's Mars Exploration Rover Opportunity's view on its 56th sol on Mars, before it left 'Eagle Crater.' 3D glasses are necessary to view this image.
This is the 3-D version of NASA's Mars Exploration Rover Opportunity's view on its 56th sol on Mars, before it left 'Eagle Crater.' 3D glasses are necessary to view this image.

A Well-Traveled 'Eagle Crater'

The slumping of materials in the walls of this impact crater imaged by NASA's Mars Odyssey spacecraft illustrates the continued erosion of the Martian surface. Small fans of debris as well as larger landslides are observed throughout the image.
The slumping of materials in the walls of this impact crater imaged by NASA's Mars Odyssey spacecraft illustrates the continued erosion of the Martian surface. Small fans of debris as well as larger landslides are observed throughout the image.

Landslides

The fluidized impact crater ejecta and flat crater floors observed in this image from NASA's Mars Odyssey spacecraft suggest near-surface volatiles once played an important role in modifying the Martian surface.
The fluidized impact crater ejecta and flat crater floors observed in this image from NASA's Mars Odyssey spacecraft suggest near-surface volatiles once played an important role in modifying the Martian surface.

Impact Craters

In this image from NASA's Mars Odyssey spacecraft, numerous lava flows and fossae (cracks) are visible in a region of Mars located southeast of Olympus Mons. There is also a hint that water may have possibly flowed in the region.
In this image from NASA's Mars Odyssey spacecraft, numerous lava flows and fossae (cracks) are visible in a region of Mars located southeast of Olympus Mons. There is also a hint that water may have possibly flowed in the region.

Gordii Fossae

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

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

Bumpy Terrain

Extensional forces in the volcanic province of Tharsis, shown in this image from NASA's Mars Odyssey spacecraft, have produced a fractured terrain that resembles wrinkled skin.
Extensional forces in the volcanic province of Tharsis, shown in this image from NASA's Mars Odyssey spacecraft, have produced a fractured terrain that resembles wrinkled skin.

Ulysses Fossae in Tharsis

This image from NASA's Mars Odyssey spacecraft shows a region of Mars called Ophir Planum. The Valles Marineris system of canyons that stretch for thousands of kilometers across Mars are located just south of the area covered in the image.
This image from NASA's Mars Odyssey spacecraft shows a region of Mars called Ophir Planum. The Valles Marineris system of canyons that stretch for thousands of kilometers across Mars are located just south of the area covered in the image.

Ophir Planum

This image from NASA's Mars Odyssey shows a region of Mars' northern hemisphere called Ismenia Fossae. Most of the landforms are the degraded remains of impact crater rim and ejecta from an unnamed crater (75 km diameter) just north of this scene.
This image from NASA's Mars Odyssey shows a region of Mars' northern hemisphere called Ismenia Fossae. Most of the landforms are the degraded remains of impact crater rim and ejecta from an unnamed crater (75 km diameter) just north of this scene.

Ismenia Fossae

This image from NASA's Mars Odyssey shows a portion of Aureum Chaos located just south of the Martian equator. This fractured landscape contains canyons and mesas with two large impact craters in the upper left.
This image from NASA's Mars Odyssey shows a portion of Aureum Chaos located just south of the Martian equator. This fractured landscape contains canyons and mesas with two large impact craters in the upper left.

Canyons and Mesas of Aureum Chaos

This image from NASA's Mars Odyssey spacecraft captures two channels (Nirgal Vallis is the smaller sinuous channel on the left and Uzboi Vallis is the larger channel located in the lower right) and Luki Crater located in the upper right.
This image from NASA's Mars Odyssey spacecraft captures two channels (Nirgal Vallis is the smaller sinuous channel on the left and Uzboi Vallis is the larger channel located in the lower right) and Luki Crater located in the upper right.

Uzboi Vallis, Nirgal Vallis, and Luki Crater

Currently displaying images 2151-2175 of 2471
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