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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

The complex channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympica Fossae, and was most likely formed by the flow of lava.
The complex channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympica Fossae, and was most likely formed by the flow of lava.

Olympica Fossae

Oti Fossae are paired fractures with a downdropped block [called graben] located on the eastern flank of Arsia Mons as seen by NASA's 2001 Mars Odyssey spacecraft.
Oti Fossae are paired fractures with a downdropped block [called graben] located on the eastern flank of Arsia Mons as seen by NASA's 2001 Mars Odyssey spacecraft.

Oti Fossae

These lava flows in Elysium Planitia captured by NASA's Mars Odyssey are called platy flows. The surface of the lava flow cooled and solidified, while liquid lava beneath kept flowing.
These lava flows in Elysium Planitia captured by NASA's Mars Odyssey are called platy flows. The surface of the lava flow cooled and solidified, while liquid lava beneath kept flowing.

Platy Flows

This image from NASA's 2001 Mars Odyssey shows a landslide deposit in Ophir Chasma.
This image from NASA's 2001 Mars Odyssey shows a landslide deposit in Ophir Chasma.

Ophir Chasma

A stereo landscape scene from NASA's Curiosity Mars rover shows rock rows at 'Junda' forming striations in the foreground, with Mount Sharp on the horizon. You need 3D glasses to view this image.
A stereo landscape scene from NASA's Curiosity Mars rover shows rock rows at 'Junda' forming striations in the foreground, with Mount Sharp on the horizon. You need 3D glasses to view this image.

Martian Landscape With Rock Rows and Mount Sharp (Stereo)

NASA's Mars rover Curiosity drove 6.2 feet (1.9 meters) during the 100th Martian day, or sol, of the mission (Nov. 16, 2012). The view spans from north at the left to south-southeast at the right. It is presented in a cylindrical projection.
NASA's Mars rover Curiosity drove 6.2 feet (1.9 meters) during the 100th Martian day, or sol, of the mission (Nov. 16, 2012). The view spans from north at the left to south-southeast at the right. It is presented in a cylindrical projection.

Curiosity's Eastward View After Sol 100 Drive

The wide channel in this image captured by NASA's Mars Odyssey is Tinto Vallis.
The wide channel in this image captured by NASA's Mars Odyssey is Tinto Vallis.

Tinto Vallis

This image captured by NASA's 2001 Mars Odyssey shows a small portion of the large fracture called Cerberus Fossae.
This image captured by NASA's 2001 Mars Odyssey shows a small portion of the large fracture called Cerberus Fossae.

Cerberus Fossae

This image from NASA's Curiosity rover shows the great diversity of grains found on the surface of a Martian rock.
This image from NASA's Curiosity rover shows the great diversity of grains found on the surface of a Martian rock.

Texture of 'Gillespie Lake' Rock

Dunes cover the floor of this unnamed crater in the northern lowlands in this image captured by NASA's Mars Odyssey.
Dunes cover the floor of this unnamed crater in the northern lowlands in this image captured by NASA's Mars Odyssey.

Northern Dunes

This image taken by NASA's 2001 Mars Odyssey shows secondary channeling on a terrace of the huge Kasei Valles outflow system.
This image taken by NASA's 2001 Mars Odyssey shows secondary channeling on a terrace of the huge Kasei Valles outflow system.

Kasei Valles

This image from NASA's Mars Odyssey shows the southeast flank of Olympus Mons. This huge volcano is surrounded by an escarpment, a large cliff at the volcano margin; a landslide lies alongside the escarpment.
This image from NASA's Mars Odyssey shows the southeast flank of Olympus Mons. This huge volcano is surrounded by an escarpment, a large cliff at the volcano margin; a landslide lies alongside the escarpment.

Olympus Mons

The depressions in this image from NASA's Mars Odyssey likely formed due to both volcanic and tectonic forces. Tectonic forces likely account for some of the depressions, while collapse into lava tubes and lava flow erosion account for the remainder.
The depressions in this image from NASA's Mars Odyssey likely formed due to both volcanic and tectonic forces. Tectonic forces likely account for some of the depressions, while collapse into lava tubes and lava flow erosion account for the remainder.

Collapse Features

The sand dunes in this image are part of Olympia Undae, a huge sand sea located near the north polar cap as seen by NASA's 2001 Mars Odyssey spacecraft.
The sand dunes in this image are part of Olympia Undae, a huge sand sea located near the north polar cap as seen by NASA's 2001 Mars Odyssey spacecraft.

Olympia Undae

This image shows a portion of Samara Valles as seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows a portion of Samara Valles as seen by NASA's 2001 Mars Odyssey spacecraft.

Samara Valles

The linear ridges in this image captured by NASA's 2001 Mars Odyssey spacecraft are located near the south polar cap.
The linear ridges in this image captured by NASA's 2001 Mars Odyssey spacecraft are located near the south polar cap.

Linear Ridges

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