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The windstreak is this image from NASA's 2001 Mars Odyssey spacecraft is located on the volcanic flows of Daedalia Planum.
The windstreak is this image from NASA's 2001 Mars Odyssey spacecraft is located on the volcanic flows of Daedalia Planum.

Windstreak

This image taken by NASA's 2001 Mars Odyssey shows the southeastern flank of Hecates Tholus, the northernmost volcano of the Elysium Volcanic complex.
This image taken by NASA's 2001 Mars Odyssey shows the southeastern flank of Hecates Tholus, the northernmost volcano of the Elysium Volcanic complex.

Hecates Tholus

This image captured by NASA's 2001 Mars Odyssey spacecraft show part of the ejecta of Bacolor Crater. The ejecta is layered and grooved, all radial to the crater itself. Bacolor Crater is located in Utopia Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft show part of the ejecta of Bacolor Crater. The ejecta is layered and grooved, all radial to the crater itself. Bacolor Crater is located in Utopia Planitia.

Bacolor Crater Ejecta

This series of images from NASA's Mars Reconnaissance Orbiter successively zooms into 'spider' features, or channels carved in the surface in radial patterns, in the south polar region of Mars.
This series of images from NASA's Mars Reconnaissance Orbiter successively zooms into 'spider' features, or channels carved in the surface in radial patterns, in the south polar region of Mars.

Volunteers Help Decide Where to Point Mars Camera

This image captured by NASA's Mars Reconnaissance Orbiter shows a small channel cutting into young volcanic lavas in a region where massive catastrophic flooding took place in the relatively recent past in the Athabasca Valles region.
This image captured by NASA's Mars Reconnaissance Orbiter shows a small channel cutting into young volcanic lavas in a region where massive catastrophic flooding took place in the relatively recent past in the Athabasca Valles region.

Sand Sources Near Athabasca Valles

The linear depression in the center of this image captured by NASA's Mars Odyssey spacecraft is a graben - a fault bounded block of material. The graben crosses the crater and ejecta in the middle of the image.
The linear depression in the center of this image captured by NASA's Mars Odyssey spacecraft is a graben - a fault bounded block of material. The graben crosses the crater and ejecta in the middle of the image.

Sirenum Fossae

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the caldera at the summit of Arsia Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the caldera at the summit of Arsia Mons.

Arsia Mons

Eridania is the name of topographically enclosed basin located in the Southern highlands of Mars that has been suggested to be the site of a large ancient lake or inland sea. This image is from NASA's Mars Reconnaissance Orbiter.
Eridania is the name of topographically enclosed basin located in the Southern highlands of Mars that has been suggested to be the site of a large ancient lake or inland sea. This image is from NASA's Mars Reconnaissance Orbiter.

Chaos in Eridania Basin

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rubicon Valles, a complex region of channels found on the northwestern flank of Alba Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rubicon Valles, a complex region of channels found on the northwestern flank of Alba Mons.

Rubicon Valles

The pits, fractures and channel-like features captured by NASA's 2001 Mars Odyssey spacecraft are located on the northern flank of Ascraeus Mons. Most of these features were created by collapse into lava tubes that existed below the surface.
The pits, fractures and channel-like features captured by NASA's 2001 Mars Odyssey spacecraft are located on the northern flank of Ascraeus Mons. Most of these features were created by collapse into lava tubes that existed below the surface.

Ascraeus Mons

This image captured by NASA's Mars Reconnaissance Orbiter shows Tharsis Tholus, one of the smaller shield volcanoes on Mars' massive 'Tharsis Rise.'
This image captured by NASA's Mars Reconnaissance Orbiter shows Tharsis Tholus, one of the smaller shield volcanoes on Mars' massive 'Tharsis Rise.'

Dust Covered Channels on Tharsis Tholus

This graphic presents results from APXS onboard NASA's rover Curiosity, with the comparisons simplified across diverse elements by dividing the amount of each element measured in the rocks by the amount of the same element in a local soil.
This graphic presents results from APXS onboard NASA's rover Curiosity, with the comparisons simplified across diverse elements by dividing the amount of each element measured in the rocks by the amount of the same element in a local soil.

Elemental Compositions of 'Yellowknife Bay' Rocks

This unnamed channel is located in Terra Cimmeria as seen by NASA's 2001 Mars Odyssey spacecraft.
This unnamed channel is located in Terra Cimmeria as seen by NASA's 2001 Mars Odyssey spacecraft.

Channel

The isolated mesas in this image from NASA's 2001 Mars Odyssey spacecraft are part of Arsinoes Chaos. There is a material that differs from the rest of the chaos visible at the bottom of the image.
The isolated mesas in this image from NASA's 2001 Mars Odyssey spacecraft are part of Arsinoes Chaos. There is a material that differs from the rest of the chaos visible at the bottom of the image.

Arsinoes Chaos

The red 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 where it reached on Nov. 30, 2010.
The red 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 where it reached on Nov. 30, 2010.

Opportunity's Path on Mars Through Sol 2436

These dunes are located on the floor of an unnamed crater in Terra Cimmeria in this image captured by NASA's Mars Odyssey spacecraft.
These dunes are located on the floor of an unnamed crater in Terra Cimmeria in this image captured by NASA's Mars Odyssey spacecraft.

Terra Cimmeria Dunes

This stereo mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 93.3-meter (306-foot) drive east-northeastward on Oct. 6, 2010. 3D glasses are necessary to view this image.
This stereo mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 93.3-meter (306-foot) drive east-northeastward on Oct. 6, 2010. 3D glasses are necessary to view this image.

Opportunity's Eastward View After Sol 2382 Drive (Stereo)

This small unnamed channel is located in southern Tyrrhena Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
This small unnamed channel is located in southern Tyrrhena Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Channel

The interconnected collapse pits at the top of this image, taken by NASA's 2001 Mars Odyssey spacecraft, are part of Coprates Catena. Notice the dunes in the bottom of each pit.
The interconnected collapse pits at the top of this image, taken by NASA's 2001 Mars Odyssey spacecraft, are part of Coprates Catena. Notice the dunes in the bottom of each pit.

Coprates Catena

The streamlined islands in this image from NASA's Mars Odyssey are located in Maja Valles.
The streamlined islands in this image from NASA's Mars Odyssey are located in Maja Valles.

Maja Valles

This mosaic of images from NASA's Mars Exploration Rover Opportunity shows terrain that includes light-toned bedrock and darker ripples of wind-blown sand. Portions of Endeavour Crater's rim are visible in the horizon of this scene.
This mosaic of images from NASA's Mars Exploration Rover Opportunity shows terrain that includes light-toned bedrock and darker ripples of wind-blown sand. Portions of Endeavour Crater's rim are visible in the horizon of this scene.

Opportunity's Eastward View After Sol 2401 Drive

The tectonic fractures in this image captured by NASA's Mars Odyssey on July 8, 2010 are part of Aram Chaos.
The tectonic fractures in this image captured by NASA's Mars Odyssey on July 8, 2010 are part of Aram Chaos.

Aram Chaos

By repeated measurements of the concentration of methane in the atmosphere at Gale Crater, NASA's Curiosity Mars rover has detected long-term variation in background levels below one part per billion.
By repeated measurements of the concentration of methane in the atmosphere at Gale Crater, NASA's Curiosity Mars rover has detected long-term variation in background levels below one part per billion.

Methane Background Levels at Gale Crater, Mars

This mosaic of four images from NASA's Mars rover Curiosity shows detailed texture in a ridge that stands higher than surrounding rock. The rock is at a location called 'Darwin,' inside Gale Crater.
This mosaic of four images from NASA's Mars rover Curiosity shows detailed texture in a ridge that stands higher than surrounding rock. The rock is at a location called 'Darwin,' inside Gale Crater.

Close-up of Ridge in Rock Outcrop at Curiosity's 'Waypoint 1'

This image from NASA's 2001 Mars Odyssey spacecraft is of Lismore Crater. This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.
This image from NASA's 2001 Mars Odyssey spacecraft is of Lismore Crater. This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.

Lismore Crater

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