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Ophir Chasma forms the northern portion of Valles Marineris, and this image from NASA's Mars Reconnaissance Orbiter spacecraft features a small part of its wall and floor.
Ophir Chasma forms the northern portion of Valles Marineris, and this image from NASA's Mars Reconnaissance Orbiter spacecraft features a small part of its wall and floor.

Layers and Fractures in Ophir Chasma

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed crater on the floor of Molesworth Carter.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed crater on the floor of Molesworth Carter.

Crater Dunes - False Color

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 windstreaks on the floor of Gusev Crater.
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 windstreaks on the floor of Gusev Crater.

Gusev Crater - False Color

This April 6, 2014, image from NASA's Mars Reconnaissance Orbiter shows numerous landslides in the vicinity of where an impact crater was excavated in March 2012.
This April 6, 2014, image from NASA's Mars Reconnaissance Orbiter shows numerous landslides in the vicinity of where an impact crater was excavated in March 2012.

Landslides Near Fresh Crater on Mars

The southern Amazonis Planitia shows two craters with ejecta that stand out above the surrounding surface. The ejecta has remained in place while the surrounding material was removed. This image is from NASA's 2001 Mars Odyssey spacecraft.
The southern Amazonis Planitia shows two craters with ejecta that stand out above the surrounding surface. The ejecta has remained in place while the surrounding material was removed. This image is from NASA's 2001 Mars Odyssey spacecraft.

Resistent Ejecta

This VIS image from NASA's 2001 Mars Odyssey spacecraft shows Tinto Vallis (middle of image) and Palos Crater (top of image).
This VIS image from NASA's 2001 Mars Odyssey spacecraft shows Tinto Vallis (middle of image) and Palos Crater (top of image).

Tinto and Palos

This image maps the traverse of NASA's Mars rover Curiosity from 'Bradbury Landing' to 'Yellowknife Bay,' with an inset documenting a change in the ground's thermal properties with arrival at a different type of terrain.
This image maps the traverse of NASA's Mars rover Curiosity from 'Bradbury Landing' to 'Yellowknife Bay,' with an inset documenting a change in the ground's thermal properties with arrival at a different type of terrain.

Curiosity's Traverse into Different Terrain

The dark dunes in this image from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Escalante Crater.
The dark dunes in this image from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Escalante Crater.

Sand Dunes

This region of chaos, as seen by NASA's 2001 Mars Odyssey spacecraft, is located southeast of Tempe Terra.
This region of chaos, as seen by NASA's 2001 Mars Odyssey spacecraft, is located southeast of Tempe Terra.

Chaos

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 map shows the route driven by NASA's Curiosity Mars rover, from the location where it landed in August 2012 to its location in July 2017, and its planned path to additional geological layers of lower Mount Sharp.
This map shows the route driven by NASA's Curiosity Mars rover, from the location where it landed in August 2012 to its location in July 2017, and its planned path to additional geological layers of lower Mount Sharp.

Mid-2017 Map of NASA's Curiosity Mars Rover Mission

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large dune form on the floor of Russell Crater.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large dune form on the floor of Russell Crater.

Russell Crater Dunes - False Color

'Perseverance Valley' lies just on the other side of the dip in the crater rim visible in the left half of this 360-degree panorama from NASA's Mars Exploration Rover Opportunity.
'Perseverance Valley' lies just on the other side of the dip in the crater rim visible in the left half of this 360-degree panorama from NASA's Mars Exploration Rover Opportunity.

Crater Rim and Plain at Head of 'Perseverance Valley,' Mars

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the canyon wall of Melas Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the canyon wall of Melas Chasma.

Melas Chasma

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

This stereo vista from the panoramic camera (Pancam) of NASA's Mars Exploration Rover Opportunity catches 'Pillinger Point,' on the western rim of Endeavour Crater, in the foreground. You need 3-D glasses to view this image.
This stereo vista from the panoramic camera (Pancam) of NASA's Mars Exploration Rover Opportunity catches 'Pillinger Point,' on the western rim of Endeavour Crater, in the foreground. You need 3-D glasses to view this image.

'Pillinger Point' Overlooking Endeavour Crater on Mars (Stereo)

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

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