2472 images found for "Mars" Wallpaper
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The Surface Stereo Imager on NASA's Phoenix Mars Lander caught this dust devil in action west of the lander on Sol 104, or the 104th Martian day of the mission, Sept. 9, 2008.
The Surface Stereo Imager on NASA's Phoenix Mars Lander caught this dust devil in action west of the lander on Sol 104, or the 104th Martian day of the mission, Sept. 9, 2008.

Martian Dust Devil Movie, Phoenix Sol 104

NASA's Phoenix Mars Lander's telltale catches a breeze as clouds move over the landing site on Sol 103 (Sept. 7, 2008), the 103rd Martian day since landing.
NASA's Phoenix Mars Lander's telltale catches a breeze as clouds move over the landing site on Sol 103 (Sept. 7, 2008), the 103rd Martian day since landing.

Phoenix Telltale Movie with Clouds, Sol 103

An angry looking sky is captured in this frame from a movie clip consisting of 10 frames taken by the Surface Stereo Imager on NASA's Phoenix Mars Lander.
An angry looking sky is captured in this frame from a movie clip consisting of 10 frames taken by the Surface Stereo Imager on NASA's Phoenix Mars Lander.

Nighttime Clouds in Martian Arctic (Accelerated Movie)

Clouds scoot across the Martian sky in a frame from a movie clip consisting of 10 frames taken by the Surface Stereo Imager on NASA's Phoenix Mars Lander.
Clouds scoot across the Martian sky in a frame from a movie clip consisting of 10 frames taken by the Surface Stereo Imager on NASA's Phoenix Mars Lander.

Ice Clouds in Martian Arctic (Accelerated Movie)

This stereo, 180-degree panorama shows the southward vista from the location where Spirit is spending its third Martian winter inside Mars' Gusev Crater on July 2, 2008. 3D glasses are necessary to view this image.
This stereo, 180-degree panorama shows the southward vista from the location where Spirit is spending its third Martian winter inside Mars' Gusev Crater on July 2, 2008. 3D glasses are necessary to view this image.

Southern Half of Spirit's 'Bonestell' Panorama (Anaglyph)

This image shows the evolution of the trench called 'Snow White' that NASA's Phoenix Mars Lander began digging on the 22nd Martian day of the mission after the May 25, 2008, landing.
This image shows the evolution of the trench called 'Snow White' that NASA's Phoenix Mars Lander began digging on the 22nd Martian day of the mission after the May 25, 2008, landing.

Snow White Trench (Animation)

A laser beam from the Canadian-built lidar instrument on NASA's Phoenix Mars Lander can be seen in this contrast-enhanced image taken by Phoenix's Surface Stereo Imager on July 26, 2008, during early Martian morning hours of the 61st Martian day.
A laser beam from the Canadian-built lidar instrument on NASA's Phoenix Mars Lander can be seen in this contrast-enhanced image taken by Phoenix's Surface Stereo Imager on July 26, 2008, during early Martian morning hours of the 61st Martian day.

Zenith Movie showing Phoenix's Lidar Beam (Animation)

This image shows NASA's Phoenix Lander's Robotic Arm scoop delivering a sample to the Thermal and Evolved-Gas Analyzer (TEGA) and how samples are analyzed within the instrument.
This image shows NASA's Phoenix Lander's Robotic Arm scoop delivering a sample to the Thermal and Evolved-Gas Analyzer (TEGA) and how samples are analyzed within the instrument.

TEGA Sample Delivery and Analysis (Animation)

NASA's Mars Exploration Rover Spirit obtained this stereo panorama of the surrounding Martian terrain in Gusev Crater . 3D glasses are necessary to view this image.
NASA's Mars Exploration Rover Spirit obtained this stereo panorama of the surrounding Martian terrain in Gusev Crater . 3D glasses are necessary to view this image.

Sweeping View of the "Columbia Hills" and Gusev Crater (3-D)

This stereo view was taken by the panoramic camera on NASA's Mars Exploration Rover Spirit on the rover's 87th martian day, or sol (April 1, 2004), just after Spirit left 'Bonneville Crater.' 3D glasses are necessary to view this image.
This stereo view was taken by the panoramic camera on NASA's Mars Exploration Rover Spirit on the rover's 87th martian day, or sol (April 1, 2004), just after Spirit left 'Bonneville Crater.' 3D glasses are necessary to view this image.

Eyeing the Drive Ahead After 'Bonneville' (3-D)

This 360-degree view combines frames taken by the navigation camera on NASA's Mars Exploration Rover Spirit during the rover's 271st martian day, or sol, on Oct. 7, 2004. 3-D glasses are necessary to view this image.
This 360-degree view combines frames taken by the navigation camera on NASA's Mars Exploration Rover Spirit during the rover's 271st martian day, or sol, on Oct. 7, 2004. 3-D glasses are necessary to view this image.

Full-Circle View from Near 'Tetl' (3-D)

This image from NASA's Mars Odyssey spacecraft shows several lava flows in Lycus Sulci. Notice the streamlined features near the bottom of the image indicating the flow direction.
This image from NASA's Mars Odyssey spacecraft shows several lava flows in Lycus Sulci. Notice the streamlined features near the bottom of the image indicating the flow direction.

Lycus Sulci

Embayment relationship is displayed where mottled plains material laps up against higher standing plains material in this image from NASA's Mars Odyssey spacecraft. The embaying material could be lava or possibly mud.
Embayment relationship is displayed where mottled plains material laps up against higher standing plains material in this image from NASA's Mars Odyssey spacecraft. The embaying material could be lava or possibly mud.

Embayment

The element potassium, shown on this NASA Mars Odyssey gamma ray spectrometer map of the mid-latitude region of Mars, is a naturally radioactive element and is a minor constituent of rocks on the surface of both Mars and Earth.
The element potassium, shown on this NASA Mars Odyssey gamma ray spectrometer map of the mid-latitude region of Mars, is a naturally radioactive element and is a minor constituent of rocks on the surface of both Mars and Earth.

Map of Martian Potassium at Mid-Latitudes

The floors of these craters imaged by NASA's Mars Odyssey contain very interesting and enigmatic materials that may hold shallow subsurface ground ice with varying amounts of a sediment covering (mantle).
The floors of these craters imaged by NASA's Mars Odyssey contain very interesting and enigmatic materials that may hold shallow subsurface ground ice with varying amounts of a sediment covering (mantle).

Nilosyrtis Mensae

In this image from NASA's Mars Odyssey, the late afternoon sun casts a shadow over a rim of Huygens Crater that's 700 meters (nearly 2,300 feet) high.
In this image from NASA's Mars Odyssey, the late afternoon sun casts a shadow over a rim of Huygens Crater that's 700 meters (nearly 2,300 feet) high.

Crater Rim

A variegated mottled texture located NW of the volcano Elysium Monsis is readily apparent in the terrain imaged here by NASA's Mars Odyssey spacecraft. The Hrad Vallis channel system can be seen sauntering across the bumpy landscape of Utopia Planitia.
A variegated mottled texture located NW of the volcano Elysium Monsis is readily apparent in the terrain imaged here by NASA's Mars Odyssey spacecraft. The Hrad Vallis channel system can be seen sauntering across the bumpy landscape of Utopia Planitia.

Complex and Perplexing Mars

One of the many branches of the Mangala Vallis channel system is seen in this image from NASA's Mars Odyssey spacecraft. The water that likely carved the channels emerged from a huge graben or fracture almost 1000 km to the south.
One of the many branches of the Mangala Vallis channel system is seen in this image from NASA's Mars Odyssey spacecraft. The water that likely carved the channels emerged from a huge graben or fracture almost 1000 km to the south.

Northwestern Branch of Mangala Vallis

The fractured surface shown in this image from NASA's Mars Odyssey spacecraft belongs to a portion of a region called Gorgonum Chaos located in the southern hemisphere of Mars.
The fractured surface shown in this image from NASA's Mars Odyssey spacecraft belongs to a portion of a region called Gorgonum Chaos located in the southern hemisphere of Mars.

Gullies of Gorgonus Chaos

Hebrus Valles is located in the Elysium Planitia region of the northern lowlands of Mars. This image from NASA's Mars Odyssey spacecraft shows three sinuous tributaries of the channel system which carved up the surrounding plains.
Hebrus Valles is located in the Elysium Planitia region of the northern lowlands of Mars. This image from NASA's Mars Odyssey spacecraft shows three sinuous tributaries of the channel system which carved up the surrounding plains.

Hebrus Valles

This NASA Mars Odyssey image shows a portion of a volcano called Alba Patera. This region has many unique valley features that at first glance look much like the patterns formed by rivers and tributaries on Earth, but are actually quite discontinuous.
This NASA Mars Odyssey image shows a portion of a volcano called Alba Patera. This region has many unique valley features that at first glance look much like the patterns formed by rivers and tributaries on Earth, but are actually quite discontinuous.

Alba Patera

Layering is visible in these deposits on the floor of Juventae Chasma in this image captured by NASA's 2001 Mars Odyssey.
Layering is visible in these deposits on the floor of Juventae Chasma in this image captured by NASA's 2001 Mars Odyssey.

Juventae Chasma

The muted terrain of northern Acidalia Planitia, as seen in this image from NASA's Mars Odyssey spacecraft, testifies to the fact that the region is heavily mantled with dust.
The muted terrain of northern Acidalia Planitia, as seen in this image from NASA's Mars Odyssey spacecraft, testifies to the fact that the region is heavily mantled with dust.

Ridges swimming in a sea of dust

NASA's Mars Exploration Rover Spirit welcomed the beginning of 2006 on Earth by taking this striking panorama of intricately rippled sand deposits in Gusev Crater on Mars.
NASA's Mars Exploration Rover Spirit welcomed the beginning of 2006 on Earth by taking this striking panorama of intricately rippled sand deposits in Gusev Crater on Mars.

Intricately Rippled Sand Deposits

This image from NASA's Mars Reconnaissance Rover shows the north polar region of Mars is surrounded by a large sea of dark sand dunes that become covered by seasonal carbon dioxide frost.
This image from NASA's Mars Reconnaissance Rover shows the north polar region of Mars is surrounded by a large sea of dark sand dunes that become covered by seasonal carbon dioxide frost.

Polygons, Crater Layers, and Defrosting Dunes

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