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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a sand sheet with a surface dune form, which partly surrounds the central peak of this unnamed crater near the north pole.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a sand sheet with a surface dune form, which partly surrounds the central peak of this unnamed crater near the north pole.

Crater Dunes

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

Arda Valles

This image from NASA's Mars Odyssey spacecraft shows a small field of dunes and associated dust devil tracks located on the floor of this unnamed crater on the rim of Roddenberry Crater.
This image from NASA's Mars Odyssey spacecraft shows a small field of dunes and associated dust devil tracks located on the floor of this unnamed crater on the rim of Roddenberry Crater.

Dunes and Dust Devils

The lava channels in this image are located in the Tharsis plains as seen by NASA's 2001 Mars Odyssey spacecraft.
The lava channels in this image are located in the Tharsis plains as seen by NASA's 2001 Mars Odyssey spacecraft.

Lava Channels

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 part of Aureum Chaos.
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 part of Aureum Chaos.

Aureum Chaos - False Color

The graben and collapse features in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Ceraunius Fossae, which is located south of Alba Mons.
The graben and collapse features in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Ceraunius Fossae, which is located south of Alba Mons.

Tectonics

The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are located SE of Adams Crater.
The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are located SE of Adams Crater.

Lava Flows

This graph shows a spectrum recorded by the Chemistry and Camera instrument (ChemCam) in NASA's Curiosity Mars rover; it is is typical of Martian volcanic (basalt) material.
This graph shows a spectrum recorded by the Chemistry and Camera instrument (ChemCam) in NASA's Curiosity Mars rover; it is is typical of Martian volcanic (basalt) material.

ChemCam Spectrum from Martian Rock Target 'Ithaca'

Many dark slope streaks mark the rim of this unnamed crater in Terra Sabaea in this image from NASA's 2001 Mars Odyssey spacecraft.
Many dark slope streaks mark the rim of this unnamed crater in Terra Sabaea in this image from NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks in Terra Sabaea

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

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