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Just as on Earth, volcanism and tectonism are found together on Mars. In this image from NASA's 2001 Mars Odyssey spacecraft the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Planum.
Just as on Earth, volcanism and tectonism are found together on Mars. In this image from NASA's 2001 Mars Odyssey spacecraft the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Planum.

Volcanism & Tectonism

NASA's Mars Reconnaissance Orbiter reveals underground ice exposed by impact cratering. The impact that dug the crater excavated water ice from beneath the surface.
NASA's Mars Reconnaissance Orbiter reveals underground ice exposed by impact cratering. The impact that dug the crater excavated water ice from beneath the surface.

Underground Ice on Mars Exposed by Impact Cratering

A surprise landslump in Melas Chasma was observed by NASA's Mars Reconnaissance Orbiter.
A surprise landslump in Melas Chasma was observed by NASA's Mars Reconnaissance Orbiter.

A Surprise Landslump in Melas Chasma

Multiple channels dissect the rim of this unnamed crater in Noachis Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
Multiple channels dissect the rim of this unnamed crater in Noachis Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Rim Channels

This image from NASA's Mars Odyssey spacecraft shows Gale crater, which is east of the landing site. It shows the northern extent of the dunes, and the layers in Mt. Sharp are visible at the bottom of the image.
This image from NASA's Mars Odyssey spacecraft shows Gale crater, which is east of the landing site. It shows the northern extent of the dunes, and the layers in Mt. Sharp are visible at the bottom of the image.

Images of Gale #3

Channels are a common feature on the margin of Terra Cimmeria where the elevation changes from highland to northern lowlands in this image captured by NASA's Mars Odyssey.
Channels are a common feature on the margin of Terra Cimmeria where the elevation changes from highland to northern lowlands in this image captured by NASA's Mars Odyssey.

Channels on Terra Cimmeria

NASA's Mars Odyssey captured this image of Ulysses Fossae, located in the Tharsis Volcanic region. Cross cutting tectonic fractures indicate that this region underwent stresses in multiple directions.
NASA's Mars Odyssey captured this image of Ulysses Fossae, located in the Tharsis Volcanic region. Cross cutting tectonic fractures indicate that this region underwent stresses in multiple directions.

Ulysses Fossae

This observation from NASA's Mars Reconnaissance Orbiter covers an outcrop of possible cyclic bedding within a crater in Arabia Terra.
This observation from NASA's Mars Reconnaissance Orbiter covers an outcrop of possible cyclic bedding within a crater in Arabia Terra.

Possible Cyclic Bedding within a Crater in Arabia Terra

This image shows a portion of the dunes on the floor of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft.
This image shows a portion of the dunes on the floor of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft.

Rabe Crater Dunes

The channels in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are called Hephaestus Fossae and were most likely formed by lava flow and erosion rather than being eroded by water.
The channels in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are called Hephaestus Fossae and were most likely formed by lava flow and erosion rather than being eroded by water.

Hephaestus Fossae

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 image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a small portion of the lava flows associated with Arsia Mons.
This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a small portion of the lava flows associated with Arsia Mons.

Arsia Mons Flows

This NASA 2001 Mars Odyssey image shows part of the floor of Coprates Chasma.
This NASA 2001 Mars Odyssey image shows part of the floor of Coprates Chasma.

Coprates Chasma Floor

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

This image maps out the travels of NASA's Mars Exploration Rover Opportunity, from is landing site at Eagle Crater to the rim of Victoria Crater about six miles (9.7 kilometers) away in September of 2006.
This image maps out the travels of NASA's Mars Exploration Rover Opportunity, from is landing site at Eagle Crater to the rim of Victoria Crater about six miles (9.7 kilometers) away in September of 2006.

Opportunity's Long Road to Victoria (Animation)

On sol 1120 (February 26, 2007), the navigation camera aboard NASA's Mars Exploration Rover Spirit captured one of the best dust devils it's seen in its three-plus year mission.
On sol 1120 (February 26, 2007), the navigation camera aboard NASA's Mars Exploration Rover Spirit captured one of the best dust devils it's seen in its three-plus year mission.

Dust Devils Whip by Spirit

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 larger craters in this image from NASA's Mars Odyssey spacecraft showing a region north of Elysium Mons are buried and distorted almost beyond recognition.
The larger craters in this image from NASA's Mars Odyssey spacecraft showing a region north of Elysium Mons are buried and distorted almost beyond recognition.

Degraded Craters in Phlegra Montes

This anaglyph from NASA's Mars Global Surveyor shows a circular feature in northern Terra Meridiani. The circular feature was once an impact crater. 3D glasses are necessary to view this image.
This anaglyph from NASA's Mars Global Surveyor shows a circular feature in northern Terra Meridiani. The circular feature was once an impact crater. 3D glasses are necessary to view this image.

Partially-Exhumed Crater in Northern Terra Meridiani: Stereo Anaglyph of overlapping coverage in M04-01289 and E17-01676

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

Currently displaying images 2201-2225 of 2951
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