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This image captured by NASA's 2001 Mars Odyssey shows a small channel emptying into a deeper crater to the west.
This image captured by NASA's 2001 Mars Odyssey shows a small channel emptying into a deeper crater to the west.

Channel

This image from NASA's 2001 Mars Odyssey spacecraft shows the Tharsis plains contains numerous channels, which were likely created by the flow of lava.
This image from NASA's 2001 Mars Odyssey spacecraft shows the Tharsis plains contains numerous channels, which were likely created by the flow of lava.

Lava Channels

The fractures, collapse features and lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are all located on the northern flank of Ascraeus Mons.
The fractures, collapse features and lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are all located on the northern flank of Ascraeus Mons.

Ascraeus Mons

This large landslide deposit is located in an unnamed crater southwest of Holden Crater. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
This large landslide deposit is located in an unnamed crater southwest of Holden Crater. This image was captured by NASA's 2001 Mars Odyssey spacecraft.

Landslide

This image shows from NASA's 2001 Mars Odyssey spacecraft some of the layered deposits in Terby Crater.
This image shows from NASA's 2001 Mars Odyssey spacecraft some of the layered deposits in Terby Crater.

Terby Crater

This panorama taken by NASA's Mars Exploration Rover Opportunity includes an outcrop informally called
This panorama taken by NASA's Mars Exploration Rover Opportunity includes an outcrop informally called

'Cambridge Bay' Outcrop Examined by Opportunity

The region of this image captured by NASA's 2001 Mars Odyssey spacecraft shows several different flow surfaces, including platy and lobate. These flows are part of Daedalia Planum.
The region of this image captured by NASA's 2001 Mars Odyssey spacecraft shows several different flow surfaces, including platy and lobate. These flows are part of Daedalia Planum.

Volcanic Flow Surfaces

The ejecta pattern around this northern plains crater is termed 'butterfly' for its similarity to butterfly wings, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
The ejecta pattern around this northern plains crater is termed 'butterfly' for its similarity to butterfly wings, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

'Butterfly' Crater

This 360-degree panorama from NASA's Mars rover Curiosity shows the rocky terrain of 'Rocknest' surrounding it as of its 55th Martian day, or sol, of the mission (Oct. 1, 2012).
This 360-degree panorama from NASA's Mars rover Curiosity shows the rocky terrain of 'Rocknest' surrounding it as of its 55th Martian day, or sol, of the mission (Oct. 1, 2012).

View on the Way to 'Glenelg'

The floor of the crater at the top of this image from NASA's 2001 Mars Odyssey spacecraft is completely covered by a large sand sheet with surface dune forms. Now that is it near the end of northern spring all the frost has disappeared from the sand.
The floor of the crater at the top of this image from NASA's 2001 Mars Odyssey spacecraft is completely covered by a large sand sheet with surface dune forms. Now that is it near the end of northern spring all the frost has disappeared from the sand.

Crater Dune

This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.
This image from NASA's 2001 Mars Odyssey spacecraft is of the south pole and shows a surface with numerous oval depressions. This texture has been described as looking like swiss cheese.

South Polar Textures

This topography map shows a portion of the Gale Crater region on Mars, where NASA's Mars Curiosity rover landed on August 6, 2014. The rover (marked with a star) is currently headed toward 'Pahrump Hills.'
This topography map shows a portion of the Gale Crater region on Mars, where NASA's Mars Curiosity rover landed on August 6, 2014. The rover (marked with a star) is currently headed toward 'Pahrump Hills.'

Slopes of Mount Sharp

This image from NASA's 2001 Mars Odyssey spacecraft shows this unnamed crater has gullies along the inner rim and dunes on the crater floor.
This image from NASA's 2001 Mars Odyssey spacecraft shows this unnamed crater has gullies along the inner rim and dunes on the crater floor.

Crater Dunes and Gullies

Showing the area just slightly west of the previous image, the large region of sand and sand dunes are the dark area that dominates this image captured by NASA's 2001 Mars Odyssey spacecraft.
Showing the area just slightly west of the previous image, the large region of sand and sand dunes are the dark area that dominates this image captured by NASA's 2001 Mars Odyssey spacecraft.

Images of Gale #20

The highest elevations of Mt. Sharp are just outside this image (to the east). In the center of this image from NASA's Mars Odyssey spacecraft is a channel, indicating that fluids played a part in eroding Mt. Sharp.
The highest elevations of Mt. Sharp are just outside this image (to the east). In the center of this image from NASA's Mars Odyssey spacecraft is a channel, indicating that fluids played a part in eroding Mt. Sharp.

Images of Gale #15

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lohse Crater.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Lohse Crater.

Lohse Crater Dunes

This image from NASA's 2001 Mars Odyssey shows channels dissecting the northwestern rim of Holden Crater.
This image from NASA's 2001 Mars Odyssey shows channels dissecting the northwestern rim of Holden Crater.

Holden Crater Rim

The channel in this image from NASA's 2001 Mars Odyssey spacecraft is located in Terra Sabaea. At some time after the channel was carved, the impact event occurred, forever blocking the channel.
The channel in this image from NASA's 2001 Mars Odyssey spacecraft is located in Terra Sabaea. At some time after the channel was carved, the impact event occurred, forever blocking the channel.

Blocked Channel

Today's image from NASA's Mars Odyssey spacecraft shows a portion of Tempe Fossae, a region of parallel to subparallel paired fractures called graben.
Today's image from NASA's Mars Odyssey spacecraft shows a portion of Tempe Fossae, a region of parallel to subparallel paired fractures called graben.

Tempe Fossae

It is early springtime in the southern hemisphere of Mars in this image from NASA's Mars Odyssey. The south polar cap is now illuminated by the sun and the surface can be studied as it changes with the passage of spring.
It is early springtime in the southern hemisphere of Mars in this image from NASA's Mars Odyssey. The south polar cap is now illuminated by the sun and the surface can be studied as it changes with the passage of spring.

South Pole

Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike. This image is part of an 'All Star' set marking the occasion of NASA's Mars Odyssey as the longest-working Mars spacecraft in history.
Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike. This image is part of an 'All Star' set marking the occasion of NASA's Mars Odyssey as the longest-working Mars spacecraft in history.

Mars Odyssey All Stars: Cerberus Crack

This image from NASA's Mars Odyssey of the floor of Ganges Chasma shows eroded fill material and extensive sand deposits.
This image from NASA's Mars Odyssey of the floor of Ganges Chasma shows eroded fill material and extensive sand deposits.

Ganges Chasma

This image taken by NASA's 2001 Mars Odyssey of the eastern end of Coprates Chasma contains a landslide deposit and sand dunes. Both features are typical for the chasmata that make up Valles Marineris.
This image taken by NASA's 2001 Mars Odyssey of the eastern end of Coprates Chasma contains a landslide deposit and sand dunes. Both features are typical for the chasmata that make up Valles Marineris.

Eastern Coprates Chasma

On Earth, these wind-derived features are called 'blowouts,' where the force of the wind has carved out a crescent-shaped depression in soft, uncemented material like glacial loess. This image is from NASA's Mars Odyssey.
On Earth, these wind-derived features are called 'blowouts,' where the force of the wind has carved out a crescent-shaped depression in soft, uncemented material like glacial loess. This image is from NASA's Mars Odyssey.

Wind Texture

The collapse features in this image captured by NASA's Mars Odyssey are located in the volcanic flows south of Alba Mons.
The collapse features in this image captured by NASA's Mars Odyssey are located in the volcanic flows south of Alba Mons.

Collapse Features

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