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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large deposit on the floor of Nicholson Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large deposit on the floor of Nicholson Crater.

Nicholson Crater

This image from NASA's 2001 Mars Odyssey spacecraf shows part of the southern flank of Ascraeus Mons. Large collapse features are common in this area.
This image from NASA's 2001 Mars Odyssey spacecraf shows part of the southern flank of Ascraeus Mons. Large collapse features are common in this area.

Ascraeus Mons Collapse Pits

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large sand sheet and surface dune forms on the floor of Proctor Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large sand sheet and surface dune forms on the floor of Proctor Crater.

Proctor Crater Dunes

A rippled dune front in Herschel Crater on Mars moved an average of about one meter (about one yard) between March 3, 2007 and December 1, 2010, as seen in one of two images from NASA's Mars Reconnaissance Orbiter.
A rippled dune front in Herschel Crater on Mars moved an average of about one meter (about one yard) between March 3, 2007 and December 1, 2010, as seen in one of two images from NASA's Mars Reconnaissance Orbiter.

Rippling Dune Front in Herschel Crater on Mars

NASA's Mars Odyssey spacecraft shows that gullies have formed on the side of this ridge in northwestern Argyre Planitia.
NASA's Mars Odyssey spacecraft shows that gullies have formed on the side of this ridge in northwestern Argyre Planitia.

Gullies in Argyre Planitia

This NASA 2001 Mars Odyssey spacecraft image shows the western edge of the summit caldera of Ceranus Tholus, one of the smaller volcanic constructs of the Tharsis region. Several channels dissect the western flank of the volcano.
This NASA 2001 Mars Odyssey spacecraft image shows the western edge of the summit caldera of Ceranus Tholus, one of the smaller volcanic constructs of the Tharsis region. Several channels dissect the western flank of the volcano.

Ceranus Tholus

This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a small section of Nirgal Vallis.
This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a small section of Nirgal Vallis.

Nirgal Vallis

This image from NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks on the surface of Sisyphi Planum.
This image from NASA's 2001 Mars Odyssey spacecraft shows dust devil tracks on the surface of Sisyphi Planum.

Dust Devil Tracks

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 Nili Patera.
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 Nili Patera.

Nili Patera - 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 of Eos Chasma.
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 of Eos Chasma.

Eos Chasma - False Color

This frame from an animation simulates a flyover of a portion of a Martian canyon detailed in a geological map produced by the U.S. Geological Survey and based on observations by the HiRISE camera on NASA's Mars Reconnaissance Orbiter.
This frame from an animation simulates a flyover of a portion of a Martian canyon detailed in a geological map produced by the U.S. Geological Survey and based on observations by the HiRISE camera on NASA's Mars Reconnaissance Orbiter.

Simulated Flyover of Mars Canyon Map (Animation)

NASA's Mars Reconnaissance Orbiter acquired this image to aid in the search for the missing lander, Mars 2. If the debris field is found, it could serve as a future landing location to study the effects of crash landing on the Martian surface.
NASA's Mars Reconnaissance Orbiter acquired this image to aid in the search for the missing lander, Mars 2. If the debris field is found, it could serve as a future landing location to study the effects of crash landing on the Martian surface.

Search for the Mars 2 Debris Field

At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.
At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.

The Icy Surface of the North Polar Cap

The objective of this observation from NASA's Mars Reconnaissance Orbiter is to determine the nature of a group of what appears to be channels that trend in a west-east direction.
The objective of this observation from NASA's Mars Reconnaissance Orbiter is to determine the nature of a group of what appears to be channels that trend in a west-east direction.

Channels in Phlegra Montes

Small impact craters usually have simple bowl shapes; however, when the target material has different layers of different strength, then more complicated crater shapes can emerge as shown in image captured by NASA's Mars Reconnaissance Orbiter.
Small impact craters usually have simple bowl shapes; however, when the target material has different layers of different strength, then more complicated crater shapes can emerge as shown in image captured by NASA's Mars Reconnaissance Orbiter.

Terraced Craters and Layered Targets

The different layers of material in this occur in Aram Chaos as seen in this image from NASA's 2001 Mars Odyssey spacecraft.
The different layers of material in this occur in Aram Chaos as seen in this image from NASA's 2001 Mars Odyssey spacecraft.

Aram Chaos

This image from NASA's Mars Odyssey spacecraft shows some of the extensive lava flows that originate at Arsia Mons.
This image from NASA's Mars Odyssey spacecraft shows some of the extensive lava flows that originate at Arsia Mons.

Arsia Mons Flows

This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that make up Daedalia Planum.
This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that make up Daedalia Planum.

Daedalia Planum

This image from NASA's Mars Odyssey shows a short section of Naktong Vallis.
This image from NASA's Mars Odyssey shows a short section of Naktong Vallis.

Naktong Vallis

This image from NASA's 2001 Mars Odyssey highlights individual dunes located on the floor of Moreaux Crater.
This image from NASA's 2001 Mars Odyssey highlights individual dunes located on the floor of Moreaux Crater.

Moreaux Crater Dunes

Many dark slope streaks are visible in this image of an unnamed crater in Terra Sabaea taken by NASA's 2001 Mars Odyssey spacecraft.
Many dark slope streaks are visible in this image of an unnamed crater in Terra Sabaea taken by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

This NASA 2001 Mars Odyssey spacecraft image shows two different types of linear depressions. The wide depression at the top of the frame is Elysium Fossae, which most likely formed due to tectonic activity.
This NASA 2001 Mars Odyssey spacecraft image shows two different types of linear depressions. The wide depression at the top of the frame is Elysium Fossae, which most likely formed due to tectonic activity.

Patapsco Vallis

This 3-D, microscopic imager mosaic of a target area on a rock called 'Diamond Jenness' was taken after NASA's Mars Exploration Rover Opportunity ground into the surface with its rock abrasion tool for a second time. 3D glasses are necessary.
This 3-D, microscopic imager mosaic of a target area on a rock called 'Diamond Jenness' was taken after NASA's Mars Exploration Rover Opportunity ground into the surface with its rock abrasion tool for a second time. 3D glasses are necessary.

'Diamond' in 3-D

This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the interior of Ganges Chasma.
This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the interior of Ganges Chasma.

Ganges Chasma - 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Hebes Chasma.
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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Hebes Chasma.

Hebes Chasma - False Color

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