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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 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

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 Iani 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 of Iani Chaos.

Iani Chaos - False Color

This image from NASA's Mars Reconnaissance Orbiter spacecraft shows numerous branching ridges with various degrees of sinuosity. These branching forms resemble tributaries funneling and draining into larger channel trunks towards the upper portion.
This image from NASA's Mars Reconnaissance Orbiter spacecraft shows numerous branching ridges with various degrees of sinuosity. These branching forms resemble tributaries funneling and draining into larger channel trunks towards the upper portion.

Fine-Branched Ridges

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Hebes Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Hebes Chasma.

Hebes Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft very clearly shows the layering that is found in both polar caps. This image is of the north polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft very clearly shows the layering that is found in both polar caps. This image is of the north polar cap.

Polar Layers

The view from NASA's Mars rover Curiosity covers a full 360 degrees, centered toward the south, with north at both the left and right ends. Nearer the horizon is a sand dune at a location called 'Dingo Gap'.
The view from NASA's Mars rover Curiosity covers a full 360 degrees, centered toward the south, with north at both the left and right ends. Nearer the horizon is a sand dune at a location called 'Dingo Gap'.

Full-Circle Vista During Curiosity's Approach to 'Dingo Gap'

Winds have scoured this region south of Olympus Mons as seen in this image from NASA's 2001 Mars Odyssey spacecraft.
Winds have scoured this region south of Olympus Mons as seen in this image from NASA's 2001 Mars Odyssey spacecraft.

Wind Erosion

Imaged by MRO's NASA's Mars Reconnaissance Orbiter Context Camera, this observation shows one of two odd, rounded mesas with a knobby, pitted texture.
Imaged by MRO's NASA's Mars Reconnaissance Orbiter Context Camera, this observation shows one of two odd, rounded mesas with a knobby, pitted texture.

A Textured Mesa

On ancient Mars, water carved channels and transported sediments to form fans and deltas within lake basins. Spectral data acquired by NASA's Mars Reconnaissance Orbiter, indicate chemical alteration by water.
On ancient Mars, water carved channels and transported sediments to form fans and deltas within lake basins. Spectral data acquired by NASA's Mars Reconnaissance Orbiter, indicate chemical alteration by water.

Chemical Alteration by Water, Jezero Crater Delta

Today's image from NASA's 2001 Mars Odyssey spacecraft shows part of the Valles Marineris canyon system -- a mega gully enters Capri Chasma.
Today's image from NASA's 2001 Mars Odyssey spacecraft shows part of the Valles Marineris canyon system -- a mega gully enters Capri Chasma.

Valles Marineris Canyon

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