2877 images found
Currently displaying images 2376-2400 of 2877
94 95 96 97 98

Wallpaper Categories

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

Featured (164)
Sun (48)
Mercury (65)
Venus (101)
Earth (969)
Mars (2877)
Jupiter (133)
Saturn (773)
Uranus (58)
Neptune (82)
Dwarf Planets (14)
Asteroids & Comets (542)
The Universe (781)
Spacecraft & Technology (0)
This image from NASA's Mars Odyssey covers a region in western Arabia Terra, which contains two interesting craters. The eastern floor of the largest crater seen in most of this image is bumpy and ridged in places and relatively smooth in regions.
This image from NASA's Mars Odyssey covers a region in western Arabia Terra, which contains two interesting craters. The eastern floor of the largest crater seen in most of this image is bumpy and ridged in places and relatively smooth in regions.

Western Arabia Terra

The ejecta blanket of the crater in this image from NASA's Mars Odyssey spacecraft does not resemble the blocky, discontinuous ejecta associated with most fresh craters on Mars.
The ejecta blanket of the crater in this image from NASA's Mars Odyssey spacecraft does not resemble the blocky, discontinuous ejecta associated with most fresh craters on Mars.

Fluidized crater ejecta

This set of images from NASA's Mars Odyssey spacecraft shows the so-called 'face on Mars' landform located in the northern plains of Mars.
This set of images from NASA's Mars Odyssey spacecraft shows the so-called 'face on Mars' landform located in the northern plains of Mars.

The So-Called "Face on Mars" in Infrared

Hrad Valles, seen in this image from NASA's Mars Odyssey spacecraft, is located north-northwest of the large Elysium Mons volcanic complex and is yet another example of a channel that likely carried fluids.
Hrad Valles, seen in this image from NASA's Mars Odyssey spacecraft, is located north-northwest of the large Elysium Mons volcanic complex and is yet another example of a channel that likely carried fluids.

Hrad Valles

White Rock' is the unofficial name for this unusual landform which was first observed during NASA's Mariner 9 mission in the early 1970's and is now shown here in an image from NASA's Mars Odyssey spacecraft.
White Rock' is the unofficial name for this unusual landform which was first observed during NASA's Mariner 9 mission in the early 1970's and is now shown here in an image from NASA's Mars Odyssey spacecraft.

White Rock

This image is a single frame from a computer animation, which begins with a global view of the planet Mars created from images by NASA's Mars Odyssey. Color is used to emphasize the Martian topographic, andesite, and basalt compositional differences.
This image is a single frame from a computer animation, which begins with a global view of the planet Mars created from images by NASA's Mars Odyssey. Color is used to emphasize the Martian topographic, andesite, and basalt compositional differences.

Still From Odyssey Clip 2

This anaglyph view of 'Shark' was produced by NASA's Mars Pathfinder's Imager camera. 3D glasses are necessary to identify surface detail.
This anaglyph view of 'Shark' was produced by NASA's Mars Pathfinder's Imager camera. 3D glasses are necessary to identify surface detail.

Shark in Super Resolution from Super Panorama

This view of 'Bookshelf Two' was produced by combining the 'Super Panorama' frames from the IMP camera from NASA's Mars Pathfinder lander. 3D glasses are necessary to identify surface detail.
This view of 'Bookshelf Two' was produced by combining the 'Super Panorama' frames from the IMP camera from NASA's Mars Pathfinder lander. 3D glasses are necessary to identify surface detail.

Bookshelf Two in Super Resolution from Super Panorama

This panoramic view taken by NASA's Mars Pathfinder is a controlled mosaic of approximately 300 IMP images. 3D glasses are necessary to identify surface detail.
This panoramic view taken by NASA's Mars Pathfinder is a controlled mosaic of approximately 300 IMP images. 3D glasses are necessary to identify surface detail.

Panoramic Views of the Landing site from Sagan Memorial Station

'Barnacle Bill' is a small rock immediately west-northwest of NASA's Mars Pathfinder lander and was the first rock visited by the rover Sojourner. 3D glasses are necessary to identify surface detail.
'Barnacle Bill' is a small rock immediately west-northwest of NASA's Mars Pathfinder lander and was the first rock visited by the rover Sojourner. 3D glasses are necessary to identify surface detail.

Super Resolution Anaglyph of Barnacle Bill

At right, NASA's Sojourner has traveled off the lander's rear ramp and onto the surface of Mars. The rock 'Barnacle Bill' and the rear ramp is to the left of Sojourner. 3-D glasses are necessary to identify surface detail.
At right, NASA's Sojourner has traveled off the lander's rear ramp and onto the surface of Mars. The rock 'Barnacle Bill' and the rear ramp is to the left of Sojourner. 3-D glasses are necessary to identify surface detail.

Sojourner near Barnacle Bill - 3-D

Many prominent rocks near the Sagan Memorial Station are featured in this image, from NASA's Mars Pathfinder. Wedge is at lower left; Shark, Half-Dome, and Pumpkin are at center. 3D glasses are necessary to identify surface detail.
Many prominent rocks near the Sagan Memorial Station are featured in this image, from NASA's Mars Pathfinder. Wedge is at lower left; Shark, Half-Dome, and Pumpkin are at center. 3D glasses are necessary to identify surface detail.

Sojourner's Favorite Rocks - in 3-D

Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars. This image is from NASA's Mars Reconnaissance Orbiter.
Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars. This image is from NASA's Mars Reconnaissance Orbiter.

Water-Bearing Rocks in Noctis Labyrinthus

Ancient lava flow in Cerberus Planitia is observed here by NASA's Mars Reconnaissance Orbiter.
Ancient lava flow in Cerberus Planitia is observed here by NASA's Mars Reconnaissance Orbiter.

Chevrons on a Flow Surface in Marte Vallis

This observation from NASA's Mars Reconnaissance Orbiter shows a beautiful example of gullies in a massif in Nereidum Montes, located in Argyre Planitia, one of the largest impact basins on Mars.
This observation from NASA's Mars Reconnaissance Orbiter shows a beautiful example of gullies in a massif in Nereidum Montes, located in Argyre Planitia, one of the largest impact basins on Mars.

Gullied Massif in the Nereidum Montes

In this image from NASA's Mars Reconnaissance Orbiter, we can see a small notch in a crater rim with a well-formed channel. Lava appears to have flowed through this notch and filled in this crater.
In this image from NASA's Mars Reconnaissance Orbiter, we can see a small notch in a crater rim with a well-formed channel. Lava appears to have flowed through this notch and filled in this crater.

Breaching a Crater Rim in Tartarus Montes

This image captured by NASA's Mars Reconnaissance Orbiter was intended to search for surface changes after three Mars years in a dust-covered region west of the Alba Mons volcano.
This image captured by NASA's Mars Reconnaissance Orbiter was intended to search for surface changes after three Mars years in a dust-covered region west of the Alba Mons volcano.

Looking for Changes in Dust Drifts West of Alba Mons

This image from NASA's Mars Reconnaissance Orbiter covers many shallow irregular pits with raised rims, concentrated along ridges and other topographic features.
This image from NASA's Mars Reconnaissance Orbiter covers many shallow irregular pits with raised rims, concentrated along ridges and other topographic features.

Mystery Martian Morphology of the Month

In this image from NASA's Mars Reconnaissance Orbiter, lower wall rock spurs are found that spread dark materials onto a dune field, suggesting local wall materials are a nearby sediment source for dunes.
In this image from NASA's Mars Reconnaissance Orbiter, lower wall rock spurs are found that spread dark materials onto a dune field, suggesting local wall materials are a nearby sediment source for dunes.

Olivine-Bearing Dune Fields and Wall Rock in Coprates Chasma

'Megabreccia' is a term used to describe jumbled, fragmented blocks of rock larger than 1 meter (1.09 yard) across. This image was observed by NASA's Mars Reconnaissance Orbiter.
'Megabreccia' is a term used to describe jumbled, fragmented blocks of rock larger than 1 meter (1.09 yard) across. This image was observed by NASA's Mars Reconnaissance Orbiter.

Megabreccia on the Floor of an Impact Crater

A beautiful delta deposit in Harris Crater is the highlighted feature in this image captured by NASA's 2001 Mars Odyssey.
A beautiful delta deposit in Harris Crater is the highlighted feature in this image captured by NASA's 2001 Mars Odyssey.

Harris Crater Delta

This image from NASA's Mars Odyssey of the south pole shows a surface texture called 'thumbprint,' for its uncanny resemblance to human fingerprints.
This image from NASA's Mars Odyssey of the south pole shows a surface texture called 'thumbprint,' for its uncanny resemblance to human fingerprints.

South Polar Surface

This daytime infrared image taken by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field located on the floor of Proctor Crater.
This daytime infrared image taken by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field located on the floor of Proctor Crater.

Proctor Crater Dunes

This image, taken by NASA's Mars Odyssey, shows dunes of several sizes in Terra Cimmeria.
This image, taken by NASA's Mars Odyssey, shows dunes of several sizes in Terra Cimmeria.

Terra Cimmeria Dunes

This view, taken by NASA's Mars Reconnaissance Orbiter from Martian orbit, shows a pale circular shape in the center is a low plateau called
This view, taken by NASA's Mars Reconnaissance Orbiter from Martian orbit, shows a pale circular shape in the center is a low plateau called

Orbital View of Spirit at 'Troy'

Currently displaying images 2376-2400 of 2877
94 95 96 97 98