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This NASA 2001 Mars Odyssey image of the southwestern flank of Alba Mons shows lava flows and collapse features.
This NASA 2001 Mars Odyssey image of the southwestern flank of Alba Mons shows lava flows and collapse features.

Alba Mons

Streamlined islands indicate the direction of flow in this image of Shalbatana Vallis. taken by NASA's 2001 Mars Odyssey spacecraft.
Streamlined islands indicate the direction of flow in this image of Shalbatana Vallis. taken by NASA's 2001 Mars Odyssey spacecraft.

Shalbatana Vallis

Several gullies located on the rim of this unnamed crater in Terra Sirenum are seen in this image taken by NASA's 2001 Mars Odyssey spacecraft.
Several gullies located on the rim of this unnamed crater in Terra Sirenum are seen in this image taken by NASA's 2001 Mars Odyssey spacecraft.

Gullies in Terra Sirenum

This series of images spanning a period of 15 weeks shows a pair of fresh craters taken by NASA's Mars Reconnaissance Orbiter. Bright, bluish material apparent in the earliest images disappears by the later ones.
This series of images spanning a period of 15 weeks shows a pair of fresh craters taken by NASA's Mars Reconnaissance Orbiter. Bright, bluish material apparent in the earliest images disappears by the later ones.

Ice in Pair of Fresh Craters on Mars Fades with Time

NASA's Mars Exploration Rover Opportunity combined images into this stereo, 360-degree view on March 28-30, 2009. In this view, the western edge of Home Plate is on the portion of the horizon farthest to the left. 3D glasses are necessary.
NASA's Mars Exploration Rover Opportunity combined images into this stereo, 360-degree view on March 28-30, 2009. In this view, the western edge of Home Plate is on the portion of the horizon farthest to the left. 3D glasses are necessary.

View Ahead After Spirit's Sol 1861 Drive (Stereo)

This anaglyph, acquired by NASA's Phoenix Lander on Jun. 23, 2008, shows a stereoscopic 3D view of the Martian surface near the lander. 3D glasses are necessary to view this image.
This anaglyph, acquired by NASA's Phoenix Lander on Jun. 23, 2008, shows a stereoscopic 3D view of the Martian surface near the lander. 3D glasses are necessary to view this image.

Martian Surface as Seen by Phoenix

NASA's Mars Exploration Rover Spirit used its panoramic camera (Pancam) to record a 360-degree vista, dubbed the 'Thanksgiving' panorama, from the northwestern side of 'Husband Hill' in late 2004. 3D glasses are necessary to view this image.
NASA's Mars Exploration Rover Spirit used its panoramic camera (Pancam) to record a 360-degree vista, dubbed the 'Thanksgiving' panorama, from the northwestern side of 'Husband Hill' in late 2004. 3D glasses are necessary to view this image.

Stereo Version of Spirit's 'Thanksgiving' Panorama

Much of the northern lowlands of Mars are thought to be relatively young volcanic flows with varying amounts of windblown dust cover. The lack of impact craters in this image from NASA's Mars Odyssey spacecraft indicate the young age of the surface.
Much of the northern lowlands of Mars are thought to be relatively young volcanic flows with varying amounts of windblown dust cover. The lack of impact craters in this image from NASA's Mars Odyssey spacecraft indicate the young age of the surface.

Acidalia Planitia

The ancient sinuous river channel shown in this image by NASA's Mars Odyssey spacecraft was likely carved by water early in Mars history. Auqakuh Valles cuts through a remarkable series of rock layers that were deposited and then subsequently eroded.
The ancient sinuous river channel shown in this image by NASA's Mars Odyssey spacecraft was likely carved by water early in Mars history. Auqakuh Valles cuts through a remarkable series of rock layers that were deposited and then subsequently eroded.

Auqakuh Valles

This image is a single frame from a computer animation, which begins with a global view of the planet Mars compiled with images from NASA's Mars Odyssey spacecraft.
This image is a single frame from a computer animation, which begins with a global view of the planet Mars compiled with images from NASA's Mars Odyssey spacecraft.

Still From Odyssey Clip 3

In this Mars Reconnaissance Orbiter view of the Curiosity rover mission's waypoint called 'the Kimberley,' the red dot indicates the location of a sandstone target, 'Windjana,' selected for close-up inspection.
In this Mars Reconnaissance Orbiter view of the Curiosity rover mission's waypoint called 'the Kimberley,' the red dot indicates the location of a sandstone target, 'Windjana,' selected for close-up inspection.

Location of Mars Sandstone Target 'Windjana'

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the dunes on the floor of Bogia Crater, a crater in Hellas Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the dunes on the floor of Bogia Crater, a crater in Hellas Planitia.

Bogia Crater Dunes

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? The hills in this image are surrounded by strange radial ridges, creating a group of jellyfish.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? The hills in this image are surrounded by strange radial ridges, creating a group of jellyfish.

THEMIS Art #119

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft sare located in the depressions of Sisyphi Cavi.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft sare located in the depressions of Sisyphi Cavi.

Dunes in Sisyphi Cavi

Sand is abundant of this portion of the floor of Ganges Chasma as captured by NASA's 2001 Mars Odyssey.
Sand is abundant of this portion of the floor of Ganges Chasma as captured by NASA's 2001 Mars Odyssey.

Ganges Chasma

NASA's Mars Exploration Rover Opportunity observed this outcrop on the 'Murray Ridge' portion of the rim of Endeavour Crater as the rover approached the 10th anniversary of its landing on Mars.
NASA's Mars Exploration Rover Opportunity observed this outcrop on the 'Murray Ridge' portion of the rim of Endeavour Crater as the rover approached the 10th anniversary of its landing on Mars.

Outcrop on 'Murray Ridge' Section of Martian Crater Rim

The yellow line on this map shows where NASA's Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, at the upper left end of the track, to a point approaching the rim of Endeavour crater.
The yellow line on this map shows where NASA's Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, at the upper left end of the track, to a point approaching the rim of Endeavour crater.

Opportunity's Route to Endeavour Crater

The landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft is located in an unnamed crater in Xanthe Terra.
The landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft is located in an unnamed crater in Xanthe Terra.

Landslide

This image from NASA's Mars Odyssey is of the south polar cap shows the tip of a trough and the surface surrounding it.
This image from NASA's Mars Odyssey is of the south polar cap shows the tip of a trough and the surface surrounding it.

V40448004

This image from NASA's Mars Odyssey shows a small channel entering the south side of Balvicar Crater.
This image from NASA's Mars Odyssey shows a small channel entering the south side of Balvicar Crater.

Balvicar Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows the southern margin of Pavonis Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows the southern margin of Pavonis Mons.

Pavonis Mons

Sand is common in the region of Juventae Chasma as shown in this image from NASA's Mars Odyssey.
Sand is common in the region of Juventae Chasma as shown in this image from NASA's Mars Odyssey.

Juventae Chasma

Component images for this stereo, 360-degree scene were taken byNASA's Mars Exploration Rover Opportunity after a drive of about 97 feet southeastward on April 22, 2014. You need 3D glasses to view this image.
Component images for this stereo, 360-degree scene were taken byNASA's Mars Exploration Rover Opportunity after a drive of about 97 feet southeastward on April 22, 2014. You need 3D glasses to view this image.

Opportunity's Tracks Near Crater Rim Ridgeline (Stereo)

The different features of the sand and sand dune field are readily visible in this image captured by NASA's 2001 Mars Odyssey spacecraft of the western floor of Gale Crater.
The different features of the sand and sand dune field are readily visible in this image captured by NASA's 2001 Mars Odyssey spacecraft of the western floor of Gale Crater.

V38546002

The dunes in Richardson crater, located at 72 degrees south latitude, are still covered in frost as seen by NASA's Mars Odyssey. The small dark spots are where the sun is beginning to remove the ice and reveal the darker dune materials below.
The dunes in Richardson crater, located at 72 degrees south latitude, are still covered in frost as seen by NASA's Mars Odyssey. The small dark spots are where the sun is beginning to remove the ice and reveal the darker dune materials below.

Richardson Crater Dunes

Currently displaying images 1951-1975 of 2612
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