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This image taken by the Mars Hand Lens Imager (MAHLI) on NASA's Mars rover Curiosity shows the texture of the patch of flat-lying bedrock called 'Cumberland,' which was the mission's second target for use of the rover's sample-collecting drill.
This image taken by the Mars Hand Lens Imager (MAHLI) on NASA's Mars rover Curiosity shows the texture of the patch of flat-lying bedrock called 'Cumberland,' which was the mission's second target for use of the rover's sample-collecting drill.

Concretions at 'Cumberland'

The network of channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Arda Valles.
The network of channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Arda Valles.

Arda Valles

This wide view of the 'John Klein' location selected for the first rock drilling by NASA's Mars rover Curiosity is a mosaic taken by Curiosity's right Mast Camera (Mastcam).
This wide view of the 'John Klein' location selected for the first rock drilling by NASA's Mars rover Curiosity is a mosaic taken by Curiosity's right Mast Camera (Mastcam).

Neighborhood for Curiosity's First Drilling Campaign

Fractures mark the surface in this region of Margaritifer Terra in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Fractures mark the surface in this region of Margaritifer Terra in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Margaritifer Terra

Lava channels and tectonic fractures are both found in the Tharsis region as shown in this image from NASA's Mars Odyssey.
Lava channels and tectonic fractures are both found in the Tharsis region as shown in this image from NASA's Mars Odyssey.

Tharsis Features

The gravity driven motion of material downhill has swept away some of the bright dust on the rim of this unnamed crater in Terra Sabaea as seen by NASA's Mars Odyssey.
The gravity driven motion of material downhill has swept away some of the bright dust on the rim of this unnamed crater in Terra Sabaea as seen by NASA's Mars Odyssey.

Dark Slope Streaks

NASA's Mars Odyssey captured this unnamed channel is west of Flammarion Crater in Terra Sabaea on July 23, 2010.
NASA's Mars Odyssey captured this unnamed channel is west of Flammarion Crater in Terra Sabaea on July 23, 2010.

Channel in Terra Sabaea

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 Martin 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 Martin Crater.

Martin Crater - 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 image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the floor of Huygens 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 image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the floor of Huygens Crater.

Huygens Crater - False Color

This channelized area is near the source region of the huge outflow channel, Ares Vallis. It was at the distal end or 'long-ways down-river-area' where the Pathfinder/Sojourner mission landed on 4 July 1997.
This channelized area is near the source region of the huge outflow channel, Ares Vallis. It was at the distal end or 'long-ways down-river-area' where the Pathfinder/Sojourner mission landed on 4 July 1997.

A Plateau in Ares Vallis

Details of hilly terrain within a large Martian canyon are shown on a geological map based on observations from NASA's Mars Reconnaissance Orbiter and produced by the U.S. Geological Survey.
Details of hilly terrain within a large Martian canyon are shown on a geological map based on observations from NASA's Mars Reconnaissance Orbiter and produced by the U.S. Geological Survey.

Geological Mapping of Hills in Martian Canyon

This map shows the route driven by NASA's Curiosity Mars rover from the 'Bradbury Landing' location where it landed in August 2012 to the 'Pahrump Hills' outcrop where it drilled into the lowest part of Mount Sharp.
This map shows the route driven by NASA's Curiosity Mars rover from the 'Bradbury Landing' location where it landed in August 2012 to the 'Pahrump Hills' outcrop where it drilled into the lowest part of Mount Sharp.

Curiosity Mars Rover's Route from Landing to 'Pahrump Hills'

Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars, as seen by NASA's Mars Reconnaissance Orbiter.
Many of the depressions in Noctis Labyrinthus contain water-bearing minerals, suggesting that water was available and persistent in this region during the Late Hesperian to Amazonian epochs on Mars, as seen by NASA's Mars Reconnaissance Orbiter.

Water-Bearing Rocks in Noctis Labyrinthus

The narrow lava flows in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northeastern flank of Olympus Mons.
The narrow lava flows in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northeastern flank of Olympus Mons.

Olympus Mons

The gray area in center of this image is where the Dust Removal Tool on NASA's Mars rover Curiosity brushed a rock target called 'Wernecke.' The brushing revealed dark nodules and white veins crisscrossing the light gray rock.
The gray area in center of this image is where the Dust Removal Tool on NASA's Mars rover Curiosity brushed a rock target called 'Wernecke.' The brushing revealed dark nodules and white veins crisscrossing the light gray rock.

Target 'Wernecke' After Brushing by Curiosity

This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the extensive lava flows in Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the extensive lava flows in Daedalia Planum.

Daedalia Planum

Isolated hills and a small channel are visible in this image of Gigas Sulci captured by NASA's 2001 Mars Odyssey spacecraft . Gigas Sulci is located southeast of Olympus Mons.
Isolated hills and a small channel are visible in this image of Gigas Sulci captured by NASA's 2001 Mars Odyssey spacecraft . Gigas Sulci is located southeast of Olympus Mons.

Gigas Sulci

Clouds are common feature over the north polar dunes in spring. This image captured by NASA's 2001 Mars Odyssey spacecraft shows line after line of puffy clouds, with hints of dark sand dunes below.
Clouds are common feature over the north polar dunes in spring. This image captured by NASA's 2001 Mars Odyssey spacecraft shows line after line of puffy clouds, with hints of dark sand dunes below.

Cloudy Day

This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows that cover the steep embankment called Olympus Rupes on the margin of Olympus Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows that cover the steep embankment called Olympus Rupes on the margin of Olympus Mons.

Olympus Rupes

With the extensive amount of dust and sandy materials on Mars, dunes are a pervasive feature. Many dunes are small, like the ones in this image from NASA's 2001 Mars Odyssey spacecraft. The bright 'squiggles' in this image are small dunes.
With the extensive amount of dust and sandy materials on Mars, dunes are a pervasive feature. Many dunes are small, like the ones in this image from NASA's 2001 Mars Odyssey spacecraft. The bright 'squiggles' in this image are small dunes.

Small Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft show windstreaks found on Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft show windstreaks found on Daedalia Planum.

Windstreaks

NASA's Mars Reconnaissance Orbiter took these images of an area near Mars' south pole where coalescing or elongated pits are interpreted as signs of an underlying deposit of frozen carbon dioxide, or 'dry ice.'
NASA's Mars Reconnaissance Orbiter took these images of an area near Mars' south pole where coalescing or elongated pits are interpreted as signs of an underlying deposit of frozen carbon dioxide, or 'dry ice.'

Pitting from Sublimation of Underlying Dry-Ice Layer

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 Cimmeria.
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 Cimmeria.

Terra Cimmeria - False Color

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 in Arabia Terra.
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 in Arabia Terra.

Arabia Terra - 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 image from NASA's 2001 Mars Odyssey spacecraft shows part of the rim of Tyndall 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 image from NASA's 2001 Mars Odyssey spacecraft shows part of the rim of Tyndall Crater.

Tyndall Crater - False Color

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