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This 360-degree panorama from NASA's Mars rover Curiosity shows the rocky terrain of 'Rocknest' surrounding it as of its 55th Martian day, or sol, of the mission (Oct. 1, 2012).
This 360-degree panorama from NASA's Mars rover Curiosity shows the rocky terrain of 'Rocknest' surrounding it as of its 55th Martian day, or sol, of the mission (Oct. 1, 2012).

View on the Way to 'Glenelg'

The floor of the crater at the top of this image from NASA's 2001 Mars Odyssey spacecraft is completely covered by a large sand sheet with surface dune forms. Now that is it near the end of northern spring all the frost has disappeared from the sand.
The floor of the crater at the top of this image from NASA's 2001 Mars Odyssey spacecraft is completely covered by a large sand sheet with surface dune forms. Now that is it near the end of northern spring all the frost has disappeared from the sand.

Crater Dune

Alluvial fans are piles of debris dumped by rivers when they emerge from the mountains and enter a mostly dry valley as seen by NASA's Mars Reconnaissance Orbiter.
Alluvial fans are piles of debris dumped by rivers when they emerge from the mountains and enter a mostly dry valley as seen by NASA's Mars Reconnaissance Orbiter.

Sinuous Ridge on the Orson Welles Bajada

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows some of the plains of Arabia Terra.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows some of the plains of Arabia Terra.

Arabia Terra - False Color

This was the first image to be acquired by NASA's Mars Reconnaissance Orbiter after the sun rose on Inca City, marking the end to polar night. A few fans are visible emerging from the araneiforms.
This was the first image to be acquired by NASA's Mars Reconnaissance Orbiter after the sun rose on Inca City, marking the end to polar night. A few fans are visible emerging from the araneiforms.

Spring in Inca City I

The hills and depressions in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Cavi Angusti.
The hills and depressions in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Cavi Angusti.

Cavi Angusti

This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.
This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.

South Polar Textures

This topography map shows a portion of the Gale Crater region on Mars, where NASA's Mars Curiosity rover landed on August 6, 2014. The rover (marked with a star) is currently headed toward 'Pahrump Hills.'
This topography map shows a portion of the Gale Crater region on Mars, where NASA's Mars Curiosity rover landed on August 6, 2014. The rover (marked with a star) is currently headed toward 'Pahrump Hills.'

Slopes of Mount Sharp

This image from NASA's 2001 Mars Odyssey spacecraft shows this unnamed crater has gullies along the inner rim and dunes on the crater floor.
This image from NASA's 2001 Mars Odyssey spacecraft shows this unnamed crater has gullies along the inner rim and dunes on the crater floor.

Crater Dunes and Gullies

Showing the area just slightly west of the previous image, the large region of sand and sand dunes are the dark area that dominates this image captured by NASA's 2001 Mars Odyssey spacecraft.
Showing the area just slightly west of the previous image, the large region of sand and sand dunes are the dark area that dominates this image captured by NASA's 2001 Mars Odyssey spacecraft.

Images of Gale #20

The highest elevations of Mt. Sharp are just outside this image (to the east). In the center of this image from NASA's Mars Odyssey spacecraft is a channel, indicating that fluids played a part in eroding Mt. Sharp.
The highest elevations of Mt. Sharp are just outside this image (to the east). In the center of this image from NASA's Mars Odyssey spacecraft is a channel, indicating that fluids played a part in eroding Mt. Sharp.

Images of Gale #15

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

Lohse Crater Dunes

This image from NASA's 2001 Mars Odyssey shows channels dissecting the northwestern rim of Holden Crater.
This image from NASA's 2001 Mars Odyssey shows channels dissecting the northwestern rim of Holden Crater.

Holden Crater Rim

The channel in this image from NASA's 2001 Mars Odyssey spacecraft is located in Terra Sabaea. At some time after the channel was carved, the impact event occurred, forever blocking the channel.
The channel in this image from NASA's 2001 Mars Odyssey spacecraft is located in Terra Sabaea. At some time after the channel was carved, the impact event occurred, forever blocking the channel.

Blocked Channel

Today's image from NASA's Mars Odyssey spacecraft shows a portion of Tempe Fossae, a region of parallel to subparallel paired fractures called graben.
Today's image from NASA's Mars Odyssey spacecraft shows a portion of Tempe Fossae, a region of parallel to subparallel paired fractures called graben.

Tempe Fossae

It is early springtime in the southern hemisphere of Mars in this image from NASA's Mars Odyssey. The south polar cap is now illuminated by the sun and the surface can be studied as it changes with the passage of spring.
It is early springtime in the southern hemisphere of Mars in this image from NASA's Mars Odyssey. The south polar cap is now illuminated by the sun and the surface can be studied as it changes with the passage of spring.

South Pole

Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike. This image is part of an 'All Star' set marking the occasion of NASA's Mars Odyssey as the longest-working Mars spacecraft in history.
Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike. This image is part of an 'All Star' set marking the occasion of NASA's Mars Odyssey as the longest-working Mars spacecraft in history.

Mars Odyssey All Stars: Cerberus Crack

This image from NASA's Mars Odyssey of the floor of Ganges Chasma shows eroded fill material and extensive sand deposits.
This image from NASA's Mars Odyssey of the floor of Ganges Chasma shows eroded fill material and extensive sand deposits.

Ganges Chasma

This image taken by NASA's 2001 Mars Odyssey of the eastern end of Coprates Chasma contains a landslide deposit and sand dunes. Both features are typical for the chasmata that make up Valles Marineris.
This image taken by NASA's 2001 Mars Odyssey of the eastern end of Coprates Chasma contains a landslide deposit and sand dunes. Both features are typical for the chasmata that make up Valles Marineris.

Eastern Coprates Chasma

On Earth, these wind-derived features are called 'blowouts,' where the force of the wind has carved out a crescent-shaped depression in soft, uncemented material like glacial loess. This image is from NASA's Mars Odyssey.
On Earth, these wind-derived features are called 'blowouts,' where the force of the wind has carved out a crescent-shaped depression in soft, uncemented material like glacial loess. This image is from NASA's Mars Odyssey.

Wind Texture

The collapse features in this image captured by NASA's Mars Odyssey are located in the volcanic flows south of Alba Mons.
The collapse features in this image captured by NASA's Mars Odyssey are located in the volcanic flows south of Alba Mons.

Collapse Features

This annotated image, taken in 2014, shows where features seen in an observation by NASA's Mars Reconnaissance Orbiter have been interpreted as hardware from the Dec. 25, 2003, arrival at Mars of the United Kingdom's Beagle 2 Lander.
This annotated image, taken in 2014, shows where features seen in an observation by NASA's Mars Reconnaissance Orbiter have been interpreted as hardware from the Dec. 25, 2003, arrival at Mars of the United Kingdom's Beagle 2 Lander.

Components of Beagle 2 Flight System on Mars

This graphic depicts what Mars' atmosphere would have looked like to a viewer with ultraviolet-seeing eyes after a meteor shower on Oct. 19, 2014.
This graphic depicts what Mars' atmosphere would have looked like to a viewer with ultraviolet-seeing eyes after a meteor shower on Oct. 19, 2014.

Emission from Ionized Magnesium in Mars' Atmosphere After Comet Flyby

The hills and ridges at the top of this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Nilus Mensae, which is part of the complex Kasei Valles channels.
The hills and ridges at the top of this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Nilus Mensae, which is part of the complex Kasei Valles channels.

Nilus Mensae

The complex channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympica Fossae, and was most likely formed by the flow of lava.
The complex channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympica Fossae, and was most likely formed by the flow of lava.

Olympica Fossae

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