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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

This image from NASA's Mars Odyssey is located west of Zephyria Planum. Surfaces in this region have undergone extensive erosion by the wind. Wind is one of the most active processes of erosion on the surface of Mars today.
This image from NASA's Mars Odyssey is located west of Zephyria Planum. Surfaces in this region have undergone extensive erosion by the wind. Wind is one of the most active processes of erosion on the surface of Mars today.

Wind and Rock

The ejecta of this unnamed crater in Amazonis Planitia is more resistant than the material around it in this image taken by NASA's Mars Odyssey.
The ejecta of this unnamed crater in Amazonis Planitia is more resistant than the material around it in this image taken by NASA's Mars Odyssey.

Crater Ejecta

This image from NASA's Mars Odyssey is of a doublet crater located in Utopia Planitia, near the Elysium Volcanic region. Doublet craters are formed by simultaneous impact of a meteor that broke into two pieces prior to hitting the surface.
This image from NASA's Mars Odyssey is of a doublet crater located in Utopia Planitia, near the Elysium Volcanic region. Doublet craters are formed by simultaneous impact of a meteor that broke into two pieces prior to hitting the surface.

Doublet Crater

A section of Nanedi Valles is shown in this image captured by NASA's 2001 Mars Odyssey.
A section of Nanedi Valles is shown in this image captured by NASA's 2001 Mars Odyssey.

Nanedi Valles

Taken by NASA's 2001 Mars Odyssey spacecraft, this image shows a small portion of the floor of Capri Chasma. Bright layered deposits and dunes are visible.
Taken by NASA's 2001 Mars Odyssey spacecraft, this image shows a small portion of the floor of Capri Chasma. Bright layered deposits and dunes are visible.

Capri Chasma

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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of the plains of 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Terra Sabaea.

Terra Sabaea - 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Coprates Chasma.
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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Coprates Chasma.

Coprates Chasma - False Color

The sinuous ridges in this image from NASA's Mars Reconnaissance Orbiter spacecraft display strong characteristics of ancient meandering riverbeds that are preserved as inverted topography.
The sinuous ridges in this image from NASA's Mars Reconnaissance Orbiter spacecraft display strong characteristics of ancient meandering riverbeds that are preserved as inverted topography.

Inverted Streams in the Aeolis Region

The depression crossing this image from NASA's 2001 Mars Odyssey spacecraft is a lava channel called Olympica Fossae. It is located on lava plains between Alba Mons and Olympus Mons.
The depression crossing this image from NASA's 2001 Mars Odyssey spacecraft is a lava channel called Olympica Fossae. It is located on lava plains between Alba Mons and Olympus Mons.

Olympica Fossae

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 Arabia Terra.
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 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 Gusev 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 Gusev Crater.

Gusev 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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the plains of Terra Cimmeria.
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 plains of Terra Cimmeria.

Terra Cimmeria - False Color

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the inner peak and floor of an unnamed crater in Terra Cimmeria.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the inner peak and floor of an unnamed crater in Terra Cimmeria.

Crater - False Color

This image from NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit within a complex crater (note the ejecta to the top and bottom of the image). There is a smaller complex crater on the ejecta to the north of the larger crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows a landslide deposit within a complex crater (note the ejecta to the top and bottom of the image). There is a smaller complex crater on the ejecta to the north of the larger crater.

Landslide

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Coloe Fossae, a series of linear depressions on the northeast margin of Terra Sabaea.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Coloe Fossae, a series of linear depressions on the northeast margin of Terra Sabaea.

Coloe Fossae

The linear depressions in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Memnonia Foassae.
The linear depressions in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Memnonia Foassae.

Memnonia Fossae

Continuing eastward, this image of Gale captured by NASA's 2001 Mars Odyssey spacecraft shows the reappearance of dunes on the crater floor near the margin of Mt. Sharp.
Continuing eastward, this image of Gale captured by NASA's 2001 Mars Odyssey spacecraft shows the reappearance of dunes on the crater floor near the margin of Mt. Sharp.

Images of Gale #6

This oblique view of Gale crater shows the landing site and the mound of layered rocks that NASA's Mars Science Laboratory will investigate. The landing site is in the smooth area in front of the mound.
This oblique view of Gale crater shows the landing site and the mound of layered rocks that NASA's Mars Science Laboratory will investigate. The landing site is in the smooth area in front of the mound.

Lower Portion of Mound Inside Gale Crater

This image from NASA's Mars Odyssey is of 'swiss cheese' terrain. Sometimes simple terms like these can accurately describe the appearance of a surface, but it does not relate at all to how that surface texture may have formed.
This image from NASA's Mars Odyssey is of 'swiss cheese' terrain. Sometimes simple terms like these can accurately describe the appearance of a surface, but it does not relate at all to how that surface texture may have formed.

South Polar Surface

The South Pole is receiving sun every day now as spring progresses. The surface texture visible in this image captured by NASA's Mars Odyssey was created by the effect of solar warming on the ice.
The South Pole is receiving sun every day now as spring progresses. The surface texture visible in this image captured by NASA's Mars Odyssey was created by the effect of solar warming on the ice.

South Polar Surface

This image from NASA's Mars Odyssey shows a portion of Avernus Colles. The term 'colles' means small hills, and the surface here is being fractured into many small hills and mesas.
This image from NASA's Mars Odyssey shows a portion of Avernus Colles. The term 'colles' means small hills, and the surface here is being fractured into many small hills and mesas.

Avernus Colles

Baetis Chasma is a chasmata near but not directly connected to Valles Marineris. Dunes are prevalent on the floor of this portion of Juventae Chasma in this image taken by NASA's 2001 Mars Odyssey.
Baetis Chasma is a chasmata near but not directly connected to Valles Marineris. Dunes are prevalent on the floor of this portion of Juventae Chasma in this image taken by NASA's 2001 Mars Odyssey.

Juventae Chasma

This image from the High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter shows gullies near the edge of Hale crater on southern Mars.
This image from the High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter shows gullies near the edge of Hale crater on southern Mars.

Gullies at the Edge of Hale Crater, Mars

This image from NASA's Mars Reconnaissance Orbiter shows one of these exotic locales at the South Pole. The polar cap is made from carbon dioxide (dry ice). The circular pits are holes in this dry ice layer that expand by a few meters each Martian year.
This image from NASA's Mars Reconnaissance Orbiter shows one of these exotic locales at the South Pole. The polar cap is made from carbon dioxide (dry ice). The circular pits are holes in this dry ice layer that expand by a few meters each Martian year.

The Coolest Landscape on Mars (or Earth)

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