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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 plains of Terra Sirenum.
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 plains of Terra Sirenum.

Terra Sirenum - False Color

This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed crater in Chryse Planitia. There are several concentric ridges visible on the right side of this image.
This image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed crater in Chryse Planitia. There are several concentric ridges visible on the right side of this image.

Rim Complexities

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows sand dunes and sand materials in depressions near the south pole.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows sand dunes and sand materials in depressions near the south pole.

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 part of the region near Nili Fossae.
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 part of the region near Nili Fossae.

False Color Surface

This image from NASA's 2001 Mars Odyssey spacecraft shows a region near Memnonia Sulci, which has been eroded by the wind to form linear ridges called yardangs. The two prominent directions of wind are recorded by the two directions of the ridges.
This image from NASA's 2001 Mars Odyssey spacecraft shows a region near Memnonia Sulci, which has been eroded by the wind to form linear ridges called yardangs. The two prominent directions of wind are recorded by the two directions of the ridges.

Yardangs

This image shows some bright layered deposits exposed within a linear trough along the floor of the Ladon Basin as seen by NASA's Mars Reconnaissance Orbiter.
This image shows some bright layered deposits exposed within a linear trough along the floor of the Ladon Basin as seen by NASA's Mars Reconnaissance Orbiter.

Bright Sediments on the Floor of Ladon Basin

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Athabasca Valles.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Athabasca Valles.

Athabasca Valles

This image from NASA's Mars Odyssey spacecraft shows an unnamed channel located in Terra Sabaea, near Hellas Planitia.
This image from NASA's Mars Odyssey spacecraft shows an unnamed channel located in Terra Sabaea, near Hellas Planitia.

Channel

An arc of dunes covers part of the floor of this unnamed crater in Aonia Terra, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
An arc of dunes covers part of the floor of this unnamed crater in Aonia Terra, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Dunes

The channel feature in this image captured by NASA's Mars Odyssey spacecraft is part of Tyrrhena Fossae, a large depression that dissects Tyrrhena Mons.
The channel feature in this image captured by NASA's Mars Odyssey spacecraft is part of Tyrrhena Fossae, a large depression that dissects Tyrrhena Mons.

Tyrrhena Fossae

The surface in this image captured by NASA's 2001 Mars Odyssey spacecraft has been scoured by the wind, producing the linear ridges/valleys.
The surface in this image captured by NASA's 2001 Mars Odyssey spacecraft has been scoured by the wind, producing the linear ridges/valleys.

Wind Erosion

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are dissecting a slope near Huygens Crater.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are dissecting a slope near Huygens Crater.

Channels

The collapse valleys in this portion of the floor of Bernard Crater were likely caused by the formation of Memnonia Fossae, a system of tectonic graben, that passes through the region. This image was captured by NASA's Mars Odyssey.
The collapse valleys in this portion of the floor of Bernard Crater were likely caused by the formation of Memnonia Fossae, a system of tectonic graben, that passes through the region. This image was captured by NASA's Mars Odyssey.

Tectonic Collapse

This observation from NASA's Mars Reconnaissance Orbiter covers a portion of the Martian equatorial plains called Elysium Planitia. In this location, lava that was once flowing across the surface interacted with multiple obstructions.
This observation from NASA's Mars Reconnaissance Orbiter covers a portion of the Martian equatorial plains called Elysium Planitia. In this location, lava that was once flowing across the surface interacted with multiple obstructions.

Flow Obstructions and Wakes Southeast of Elysium Planitia

Dunes of sand-sized materials have been trapped on the floors of many Martian craters, as seen in this view captured by NASA's Mars Reconnaissance Orbiter. This is one example, from a crater in Noachis Terra, west of the giant Hellas impact basin.
Dunes of sand-sized materials have been trapped on the floors of many Martian craters, as seen in this view captured by NASA's Mars Reconnaissance Orbiter. This is one example, from a crater in Noachis Terra, west of the giant Hellas impact basin.

Dune Symmetry Inside Martian Crater

This image from NASA's Mars Reconnaissance Orbiter shows the southern latitude Hale Crater, a rather large, pristine elliptical crater possessing sharp features, impact melt bodies ponded throughout the structure and few overprinting impact craters.
This image from NASA's Mars Reconnaissance Orbiter shows the southern latitude Hale Crater, a rather large, pristine elliptical crater possessing sharp features, impact melt bodies ponded throughout the structure and few overprinting impact craters.

Light-Toned Gully Materials on Hale Crater Wall

This image from NASA's 2001 Mars Odyssey shows a complex tributary channel and its entry to the main channel of Shalbatana Vallis.
This image from NASA's 2001 Mars Odyssey shows a complex tributary channel and its entry to the main channel of Shalbatana Vallis.

Shalbatana Vallis

This view from the Mars Hand Lens Imager (MAHLI) on the arm of NASA's Curiosity Mars rover shows a combination of dark and light material within a mineral vein at a site called 'Garden City' on lower Mount Sharp.
This view from the Mars Hand Lens Imager (MAHLI) on the arm of NASA's Curiosity Mars rover shows a combination of dark and light material within a mineral vein at a site called 'Garden City' on lower Mount Sharp.

Light Material Ripped Up Older Dark Vein Material

A view from NASA's Mars Reconnaissance Orbiter on April 8, 2015, catches sight of NASA's Curiosity Mars rover passing through a valley called 'Artist's Drive' on the lower slope of Mount Sharp.
A view from NASA's Mars Reconnaissance Orbiter on April 8, 2015, catches sight of NASA's Curiosity Mars rover passing through a valley called 'Artist's Drive' on the lower slope of Mount Sharp.

Mars Orbiter Sees Curiosity Rover in 'Artist's Drive'

This image from NASA's Mars Reconnaissance Orbiter is one of the rare examples of a fresh 'lunar-like' crater on Mars. The impact crater formed in the Tharsis region.
This image from NASA's Mars Reconnaissance Orbiter is one of the rare examples of a fresh 'lunar-like' crater on Mars. The impact crater formed in the Tharsis region.

A Fresh, Lunar-Like Crater on Mars

If a meteorite breaks in two shortly before hitting the ground, the typical bowl shape of a single impact crater becomes doubled. This image is from NASA's Mars Odyssey, one of an 'All Star' set.
If a meteorite breaks in two shortly before hitting the ground, the typical bowl shape of a single impact crater becomes doubled. This image is from NASA's Mars Odyssey, one of an 'All Star' set.

Mars Odyssey All Stars: Dual Crater

This 3-D scene shows the view from where NASA's Mars Exploration Rover Opportunity first arrived on the rim of Endeavour crater, an impact crater about 14 miles (22 kilometers) in diameter. You will need 3D glasses to view this image.
This 3-D scene shows the view from where NASA's Mars Exploration Rover Opportunity first arrived on the rim of Endeavour crater, an impact crater about 14 miles (22 kilometers) in diameter. You will need 3D glasses to view this image.

'Spirit Point' Vista from Opportunity, in Stereo

This mosaic of images from the navigation camera on NASA's Mars Exploration Rover Opportunity shows a terrain that includes light-toned bedrock and darker ripples of wind-blown sand.
This mosaic of images from the navigation camera on NASA's Mars Exploration Rover Opportunity shows a terrain that includes light-toned bedrock and darker ripples of wind-blown sand.

Opportunity's Eastward View After Sol 2382 Drive

On this image of the rock target 'Knorr,' color coding maps the amount of mineral hydration indicated by a ratio of near-infrared reflectance intensities measured by the Mastcam on NASA's Mars rover Curiosity.
On this image of the rock target 'Knorr,' color coding maps the amount of mineral hydration indicated by a ratio of near-infrared reflectance intensities measured by the Mastcam on NASA's Mars rover Curiosity.

Hydration Map, Based on Mastcam Spectra, for 'Knorr' Rock Target

The finely ridged material in this image captured by NASA's 2001 Mars Odyssey spacecraft are huge landslide deposits called Coprates Labes. These landslide deposits are located on the floor of Coprates Chasma.
The finely ridged material in this image captured by NASA's 2001 Mars Odyssey spacecraft are huge landslide deposits called Coprates Labes. These landslide deposits are located on the floor of Coprates Chasma.

Coprates Labes

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