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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 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 of Aureum Chaos.

Aureum Chaos - False Color

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows the rim and ejecta of an unnamed crater northwest of Hesperia Planum.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows the rim and ejecta of an unnamed crater northwest of Hesperia Planum.

Hesperia Planum - False Color

The THEMIS VIS camera contains 5 filters. The data from different filters can create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Schaeberle Crater, including small dunes.
The THEMIS VIS camera contains 5 filters. The data from different filters can create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Schaeberle Crater, including small dunes.

Schaeberle Crater - False Color

This image from NASA's Mars Mars Reconnaissance Orbiter shows a triple impact crater in Elysium Planitia near Tartarus Montes, which probably formed when a binary-or even triple-asteroid struck the surface.
This image from NASA's Mars Mars Reconnaissance Orbiter shows a triple impact crater in Elysium Planitia near Tartarus Montes, which probably formed when a binary-or even triple-asteroid struck the surface.

Triple-Crater in Elysium Planitia

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 Calahorra Crater in Chryse Planitia.
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 Calahorra Crater in Chryse Planitia.

Calahorra Crater - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a graben cutting through a plateau. The graben is part of Sirenum Fossae.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a graben cutting through a plateau. The graben is part of Sirenum Fossae.

Sirenum Fossae

The small channels in this image from NASA's 2001 Mars Odyssey spacecraft are located within the much larger Kasei Valles channel.
The small channels in this image from NASA's 2001 Mars Odyssey spacecraft are located within the much larger Kasei Valles channel.

Kasei Valles

The channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is a portion of Hrad Vallis.
The channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is a portion of Hrad Vallis.

Hrad Vallis

Looking at yet another portion of Utopia Planitia, NASA's 2001 Mars Odyssey spacecraft still find hundreds of dust devil tracks.
Looking at yet another portion of Utopia Planitia, NASA's 2001 Mars Odyssey spacecraft still find hundreds of dust devil tracks.

More Dust Devils

Numerous channels dissect both sides of this high spot south of Solis Planum in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Numerous channels dissect both sides of this high spot south of Solis Planum in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Channels

This graph compares the elemental composition of typical soils at three landing regions on Mars: Gusev Crater, from Spirit; Meridiani Planum, from Opportunity; and now Gale Crater, where NASA's newest Curiosity rover is currently investigating.
This graph compares the elemental composition of typical soils at three landing regions on Mars: Gusev Crater, from Spirit; Meridiani Planum, from Opportunity; and now Gale Crater, where NASA's newest Curiosity rover is currently investigating.

Inspecting Soils Across Mars

The lava channels in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern flank of Ascraeus Mons.
The lava channels in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern flank of Ascraeus Mons.

Lava Channels

This image shows a portion of Utopia Planitia that is covered by dust devil tracks as seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows a portion of Utopia Planitia that is covered by dust devil tracks as seen by NASA's 2001 Mars Odyssey spacecraft.

Utopia Planitia

This view of channels on Mars came from NASA's Mariner 9 orbiter. In 1971, Mariner 9 became the first spacecraft to enter orbit around Mars.
This view of channels on Mars came from NASA's Mariner 9 orbiter. In 1971, Mariner 9 became the first spacecraft to enter orbit around Mars.

Mariner 9 View of Nirgal Vallis

Dunes on the floor of Russell Crater vary from individual dunes, to a large hook shaped, towering sand sheet as seen by NASA's Mars Odyssey.
Dunes on the floor of Russell Crater vary from individual dunes, to a large hook shaped, towering sand sheet as seen by NASA's Mars Odyssey.

Russell Crater Dunes

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 the plains between Hale Crater and Argyre Planitia.
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 the plains between Hale Crater and Argyre Planitia.

Argyre Basin Margin - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a region of small isolated dunes on the floor of an unnamed crater in Terra Cimmeria.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a region of small isolated dunes on the floor of an unnamed crater in Terra Cimmeria.

Crater Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows several linear depressions that cross an unnamed crater. The depressions are tectonic fractures that are hundreds of km long.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows several linear depressions that cross an unnamed crater. The depressions are tectonic fractures that are hundreds of km long.

Sirenum Fossae

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

Daedalia Planum

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 Candor Labes.
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 Candor Labes.

Candor Labes - 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 floor of Antoniadi 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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Antoniadi Crater.

Antoniadi Crater - False Color

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae.

Olympia Undae

These two images come from the HiRISE camera on NASA's Mars Reconnaissance Orbiter. Images of locations in Gale Crater taken from orbit around Mars reveal evidence of erosion in recent geological times and development of small scarps, or vertical surfaces
These two images come from the HiRISE camera on NASA's Mars Reconnaissance Orbiter. Images of locations in Gale Crater taken from orbit around Mars reveal evidence of erosion in recent geological times and development of small scarps, or vertical surfaces

Erosion Patterns May Guide Mars Rover to Rocks Recently Exposed

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that comprise Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that comprise Daedalia Planum.

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Proctor Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Proctor Crater.

Proctor Crater Dunes

Currently displaying images 2151-2175 of 3747
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