3711 images found
Currently displaying images 1976-2000 of 3711
78 79 80 81 82

Wallpaper Categories

Choose from the categories below. Click on the thumbnail image to preview and download the JPL wallpaper.

Featured (209)
Sun (73)
Mercury (65)
Venus (102)
Earth (1170)
Mars (3711)
Jupiter (141)
Saturn (933)
Uranus (58)
Neptune (82)
Dwarf Planets (454)
Asteroids & Comets (636)
The Universe (917)
Spacecraft & Technology (912)
These ridges near the south polar cap are called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
These ridges near the south polar cap are called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Polar Ridges

The windstreaks in this image captured by NASA's Mars Odyssey are located on lava flows from Arsia Mons.
The windstreaks in this image captured by NASA's Mars Odyssey are located on lava flows from Arsia Mons.

Windstreaks on Arsia Mons

This image from NASA's 2001 Mars Odyssey shows a portion of the floor of Ganges Chasma. Eroded deposits and sand dune forms are common features of Ganges Chasma.
This image from NASA's 2001 Mars Odyssey shows a portion of the floor of Ganges Chasma. Eroded deposits and sand dune forms are common features of Ganges Chasma.

Ganges Chasma

This image shows fine sand from Mars that was filtered by NASA's Curiosity rover as part of its first 'decontamination' exercise.
This image shows fine sand from Mars that was filtered by NASA's Curiosity rover as part of its first 'decontamination' exercise.

Sand Filtered through Curiosity's Sieve

This image from NASA's Mars Reconnaissance Orbiter shows the funnel-shaped terminus of Lethe Vallis, a winding channel in the Elysium Planitia region of Mars; the floor is covered in solidified lava and blanketed by a thin layer of light-toned dust.
This image from NASA's Mars Reconnaissance Orbiter shows the funnel-shaped terminus of Lethe Vallis, a winding channel in the Elysium Planitia region of Mars; the floor is covered in solidified lava and blanketed by a thin layer of light-toned dust.

End of Lethe Vallis

Illumination in this image comes from MAHLI's two ultraviolet LEDs, which emit light in a waveband centered at a wavelength of 365 nanometers in this image of a calibration target on NASA's Mars rover Curiosity.
Illumination in this image comes from MAHLI's two ultraviolet LEDs, which emit light in a waveband centered at a wavelength of 365 nanometers in this image of a calibration target on NASA's Mars rover Curiosity.

First Night Image of MAHLI Calibration Target Under Ultraviolet Lights

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a series of low, concentric ridges is located to the west of Arsia Mons. The origin of these features is unknown, and there are no similar features at the other Tharsis volcanoes.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a series of low, concentric ridges is located to the west of Arsia Mons. The origin of these features is unknown, and there are no similar features at the other Tharsis volcanoes.

Arsia Mons 'Ripples'

This image from NASA's 2001 Mars Odyssey spacecraft shows dune forms on the floor of Orson Welles Crater, an impact crater in the Coprates quadrangle named for the actor.
This image from NASA's 2001 Mars Odyssey spacecraft shows dune forms on the floor of Orson Welles Crater, an impact crater in the Coprates quadrangle named for the actor.

Orson Welles Dunes

Layering of Arabia Terra is evident in this image from NASA's 2001 Mars Odyssey spacecraft.
Layering of Arabia Terra is evident in this image from NASA's 2001 Mars Odyssey spacecraft.

Layers

This image from NASA's Mars Odyssey shows part of the summit of Ceraunius Tholus.
This image from NASA's Mars Odyssey shows part of the summit of Ceraunius Tholus.

Ceraunius Tholus

A view from NASA's Mars Reconnaissance Orbiter on April 8, 2015, catches sight of NASA's Curiosity Mars rover passing through a valley called 'Artist's Drive' on the lower slope of Mount Sharp.
A view from NASA's Mars Reconnaissance Orbiter on April 8, 2015, catches sight of NASA's Curiosity Mars rover passing through a valley called 'Artist's Drive' on the lower slope of Mount Sharp.

Mars Orbiter Sees Curiosity Rover in 'Artist's Drive'

This frame from an animation from NASA's Mars rover Curiosity shows the rover drilling into rock target 'Cumberland.' The drilling was performed during the 279th Martian day, or sol, of the Curiosity's work on Mars (May 19, 2013).
This frame from an animation from NASA's Mars rover Curiosity shows the rover drilling into rock target 'Cumberland.' The drilling was performed during the 279th Martian day, or sol, of the Curiosity's work on Mars (May 19, 2013).

Curiosity Mars Rover Drilling Into Its Second Rock

This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes in located on the floor of Lyot Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes in located on the floor of Lyot Crater.

Lyot Crater Dunes

This image, taken by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is of a gully on a south-facing slope in middle southern latitudes of Mars.
This image, taken by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is of a gully on a south-facing slope in middle southern latitudes of Mars.

Changes in a Gully in a Mars Crater (Two-Image Comparison)

This windstreak is located on the volcanic plains of Daedalia Planum as seen by NASA's Mars Odyssey. The dark outer margin is the region of dust being removed from the surface. The inner bright part is where dust is being deposited.
This windstreak is located on the volcanic plains of Daedalia Planum as seen by NASA's Mars Odyssey. The dark outer margin is the region of dust being removed from the surface. The inner bright part is where dust is being deposited.

Windstreak on Daedalia Planum

These dunes in Richardson Crater are still frost covered in this image captured by NASA's Mars Odyssey. As spring deepens the frost will sublimate and the dark dunes will appear.
These dunes in Richardson Crater are still frost covered in this image captured by NASA's Mars Odyssey. As spring deepens the frost will sublimate and the dark dunes will appear.

Richardson Crater Dunes

NASA's Curiosity Mars rover targeted the laser of the ChemCam instrument with remarkable accuracy for assessing the composition of the wall of a drilled hole and tailings that resulted from the drilling.
NASA's Curiosity Mars rover targeted the laser of the ChemCam instrument with remarkable accuracy for assessing the composition of the wall of a drilled hole and tailings that resulted from the drilling.

Accurate Pointing by Curiosity

This map of Mars from NASA's Mars Odyssey orbiter shows relative locations of three types of findings related to salt or frozen water, plus a new type of finding that may be related to both salt and water.
This map of Mars from NASA's Mars Odyssey orbiter shows relative locations of three types of findings related to salt or frozen water, plus a new type of finding that may be related to both salt and water.

Ice, Salt and Warm-Season Flows on Mars

This image captured by NASA's 2001 Mars Odyssey shows a landslide deposit located in an unnamed crater in Syrtis Planum.
This image captured by NASA's 2001 Mars Odyssey shows a landslide deposit located in an unnamed crater in Syrtis Planum.

Syrtis Planum Landslide

This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows from Alba Mons. The depression and collapse features within it are part of the large system of tectonic features created by the apparent collapse of the volcano.
This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows from Alba Mons. The depression and collapse features within it are part of the large system of tectonic features created by the apparent collapse of the volcano.

Alba Mons Flows

A volcanic vent has created a small construct (a volcano) in this region of Tharsis east of Arsia Mons. This image is from NASA's 2001 Mars Odyssey spacecraft.
A volcanic vent has created a small construct (a volcano) in this region of Tharsis east of Arsia Mons. This image is from NASA's 2001 Mars Odyssey spacecraft.

Tharsis Volcanics

The wind etched region in this image captured by NASA's Mars Odyssey on July 23, 2010 is called Zephyria Planum.
The wind etched region in this image captured by NASA's Mars Odyssey on July 23, 2010 is called Zephyria Planum.

Zephyria Planum

Dark slope streaks mark the rim of this unnamed crater near Schiaparelli Crater as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks mark the rim of this unnamed crater near Schiaparelli Crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

This unnamed as seen by NASA's 2001 Mars Odyssey spacecraft channel drains part of Margaritifer Terra.
This unnamed as seen by NASA's 2001 Mars Odyssey spacecraft channel drains part of Margaritifer Terra.

Channel

This image from NASA's Mars Reconnaissance Orbiter shows a number of unusual, quasi-circular structures that apparently formed within bright flows in Meridiani Planum.
This image from NASA's Mars Reconnaissance Orbiter shows a number of unusual, quasi-circular structures that apparently formed within bright flows in Meridiani Planum.

Concentric Structures in Meridiani Planum

Currently displaying images 1976-2000 of 3711
78 79 80 81 82