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This image, captured by NASA's Mars Odyssey on May 23, 2010 of Daedalia Planum, shows various lava flows from Arsia Mons.
This image, captured by NASA's Mars Odyssey on May 23, 2010 of Daedalia Planum, shows various lava flows from Arsia Mons.

Daedalia Planum

Richardson Crater is home to this sea of sand dunes. It was fall in the Southern hemisphere when NASA's MRO acquired this image of the dunes frosted with the first bit of carbon dioxide ice condensed from the atmosphere.
Richardson Crater is home to this sea of sand dunes. It was fall in the Southern hemisphere when NASA's MRO acquired this image of the dunes frosted with the first bit of carbon dioxide ice condensed from the atmosphere.

Fall Frosting

This diagram shows how materials analyzed by the ChemCam instrument on NASA's Curiosity Mars rover during the first 100 Martian days of the mission differed with regard to hydrogen content (horizontal axis) and alkali (vertical axis).
This diagram shows how materials analyzed by the ChemCam instrument on NASA's Curiosity Mars rover during the first 100 Martian days of the mission differed with regard to hydrogen content (horizontal axis) and alkali (vertical axis).

Curiosity's ChemCam Analyzes Rocks, Soils and Dust

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows of Solis Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows of Solis Planum.

Solis Planum

The complex channels in this image from NASA's 2001 Mars Odyssey spacecraft are part of Granicus Valles, located on the western margin of the Elysium volcanic region.
The complex channels in this image from NASA's 2001 Mars Odyssey spacecraft are part of Granicus Valles, located on the western margin of the Elysium volcanic region.

Granicus Valles

This image captured by NASA's Mars Odyssey shows the layers of a polar trough and several different surface textures.
This image captured by NASA's Mars Odyssey shows the layers of a polar trough and several different surface textures.

South Polar Surface

This image of Utopia Planitia, NASA's 2001 Mars Odyssey, is covered with the tracks of dust devils.
This image of Utopia Planitia, NASA's 2001 Mars Odyssey, is covered with the tracks of dust devils.

Utopia Planitia

This full-circle view from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit shows the terrain surrounding the location called 'Troy,' where Spirit became embedded in soft soil during the spring of 2009. 3D glasses are necessary.
This full-circle view from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit shows the terrain surrounding the location called 'Troy,' where Spirit became embedded in soft soil during the spring of 2009. 3D glasses are necessary.

'Calypso' Panorama of Spirit's View from 'Troy' (Stereo)

This image from NASA's Mars Exploration Rover, Opportunity, shows the lower reaches of 'Murray Ridge,' informally named to honor the late Bruce Murray, who led NASA's Jet Propulsion Laboratory through a period of great challenge and achievement.
This image from NASA's Mars Exploration Rover, Opportunity, shows the lower reaches of 'Murray Ridge,' informally named to honor the late Bruce Murray, who led NASA's Jet Propulsion Laboratory through a period of great challenge and achievement.

Opportunity's View Climbing 'Murray Ridge'

This is only one of four impact craters on Mars known that possesses intact layers exposed in the central uplift in this image from NASA's Mars Reconnaissance Orbiter.
This is only one of four impact craters on Mars known that possesses intact layers exposed in the central uplift in this image from NASA's Mars Reconnaissance Orbiter.

Beautiful Layers in the Central Uplift of Mazamba Crater

The sand dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lyot Crater.
The sand dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lyot Crater.

Lyot Crater Dunes

Small dunes are located on the floor of this unnamed crater in Terra Cimmeria as seen by NASA's 2001 Mars Odyssey spacecraft.
Small dunes are located on the floor of this unnamed crater in Terra Cimmeria as seen by NASA's 2001 Mars Odyssey spacecraft.

V43188001

'Yankee Clipper' crater on Mars carries the name of the command and service module of NASA's 1969 Apollo 12 mission to the moon. NASA's Mars Exploration Rover Opportunity recorded this stereo view on Nov. 4, 2010. 3D glasses are necessary.
'Yankee Clipper' crater on Mars carries the name of the command and service module of NASA's 1969 Apollo 12 mission to the moon. NASA's Mars Exploration Rover Opportunity recorded this stereo view on Nov. 4, 2010. 3D glasses are necessary.

'Yankee Clipper' Crater on Mars (Stereo)

This image from NASA's 2001 Mars Odyssey spacecraft shows sand dunes of the floor of Trouvelot Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows sand dunes of the floor of Trouvelot Crater.

Trouvelot Crater Dunes

This image taken by NASA's 2001 Mars Odyssey shows a portion of the floor of Melsa Chasma. Wind blown material is located in lows between layered floor materials.
This image taken by NASA's 2001 Mars Odyssey shows a portion of the floor of Melsa Chasma. Wind blown material is located in lows between layered floor materials.

Melas Chasma

This image from NASA's 2001 Mars Odyssey spacecraft shows the margin between materials being sculpted by the wind into long, narrow hills and a surface not visibly affected by the wind.
This image from NASA's 2001 Mars Odyssey spacecraft shows the margin between materials being sculpted by the wind into long, narrow hills and a surface not visibly affected by the wind.

Wind Erosion

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field located on the floor of Rabe Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field located on the floor of Rabe Crater.

Rabe Crater Dunes

Several fractures cross through Gorgonum Chaos in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Several fractures cross through Gorgonum Chaos in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Gorgonum Chaos

This global map of Mars was acquired on Aug. 5, 2012, by the Mars Color Imager instrument on NASA's MRO. One global map is generated each day to forecast weather conditions for the entry, descent and landing of NASA's Curiosity rover.
This global map of Mars was acquired on Aug. 5, 2012, by the Mars Color Imager instrument on NASA's MRO. One global map is generated each day to forecast weather conditions for the entry, descent and landing of NASA's Curiosity rover.

Mars Weather Map, Aug. 5

Sirenum Fossae is comprised of long, parallel fracture systems, some of which are seen in this image from NASA's 2001 Mars Odyssey spacecraft.
Sirenum Fossae is comprised of long, parallel fracture systems, some of which are seen in this image from NASA's 2001 Mars Odyssey spacecraft.

Sirenum Fossae

The pale rocks in the foreground of this Aug. 14, 2014, image from NASA's Curiosity Mars rover include the 'Bonanza King' target under consideration to become the fourth rock drilled by the rover.
The pale rocks in the foreground of this Aug. 14, 2014, image from NASA's Curiosity Mars rover include the 'Bonanza King' target under consideration to become the fourth rock drilled by the rover.

View Down 'Hidden Valley' Ramp at 'Bonanza King' on Mars

Gravity has caused materials to move down the rim of this crater in Terra Sabaea. In this image from NASA's 2001 Mars Odyssey, thinner dark slope streaks are less common than broader, lighter markings of downslope movement of materials.
Gravity has caused materials to move down the rim of this crater in Terra Sabaea. In this image from NASA's 2001 Mars Odyssey, thinner dark slope streaks are less common than broader, lighter markings of downslope movement of materials.

Terra Sabaea

This image from NASA's 2001 Mars Odyssey spacecraft shows a wind eroded surface located between the lava flows of Olympus Mons and the wind eroded ridge called Gordii Dorsum.
This image from NASA's 2001 Mars Odyssey spacecraft shows a wind eroded surface located between the lava flows of Olympus Mons and the wind eroded ridge called Gordii Dorsum.

Wind Erosion

This image from NASA's 2001 Mars Odyssey spacecraft shows some of the depressions in the material that fills Asimov Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows some of the depressions in the material that fills Asimov Crater.

Asimov Crater

The narrow volcanic flows in this image from NASA's 2001 Mars Odyssey spacecraft are located on Olympus Mons, the largest volcano in the solar system.
The narrow volcanic flows in this image from NASA's 2001 Mars Odyssey spacecraft are located on Olympus Mons, the largest volcano in the solar system.

Olympus Mons

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