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The landslide deposit in this image captured by NASA's 2001 Mars Odyssey spacecraft is located in Aurorae Chaos (distinctive area of broken terrain). Several regions of chaotic terrain are located on the eastern end of the Valles Marineris system.
The landslide deposit in this image captured by NASA's 2001 Mars Odyssey spacecraft is located in Aurorae Chaos (distinctive area of broken terrain). Several regions of chaotic terrain are located on the eastern end of the Valles Marineris system.

Aurorae Chaos

A network of large and small channels dissect this highland region in Terra Cimmeria, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
A network of large and small channels dissect this highland region in Terra Cimmeria, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Channels

This mosaic shows a north-facing outcrop, informally named 'Greeley Haven.' The site is near the northern tip of the
This mosaic shows a north-facing outcrop, informally named 'Greeley Haven.' The site is near the northern tip of the

'Greeley Haven' Site for Opportunity's Fifth Martian Winter

The channel at the top of this image captured by NASA's 2001 Mars Odyssey spacecraft runs between Galilaei Crater and the main channel on the northeastern side of Hydaspis Chaos.
The channel at the top of this image captured by NASA's 2001 Mars Odyssey spacecraft runs between Galilaei Crater and the main channel on the northeastern side of Hydaspis Chaos.

Hydaspis Chaos

This image shows dunes in and around a crater located on the floor of the much larger Herschel Crater as seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows dunes in and around a crater located on the floor of the much larger Herschel Crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Crater Dunes

The floor of Melsa Chasma contains a variety of landforms. This image from NASA's 2001 Mars Odyssey shows deposits of fine materials as well as layered deposits.
The floor of Melsa Chasma contains a variety of landforms. This image from NASA's 2001 Mars Odyssey shows deposits of fine materials as well as layered deposits.

Melas Chasma

Located near Amazonis Mensa, this region of Mars has undergone erosion by wind. Long linear hills being created by the wind are called yardangs in this image from NASA's 2001 Mars Odyssey.
Located near Amazonis Mensa, this region of Mars has undergone erosion by wind. Long linear hills being created by the wind are called yardangs in this image from NASA's 2001 Mars Odyssey.

Wind Effects

This image from NASA's Mars Odyssey shows the northern sidewall of Melas Chasma.
This image from NASA's Mars Odyssey shows the northern sidewall of Melas Chasma.

Melas Chasma

This image from NASA's 2001 Mars Odyssey shows a portion of Capri Chasma. Dunes are found on the floor of this chasma.
This image from NASA's 2001 Mars Odyssey shows a portion of Capri Chasma. Dunes are found on the floor of this chasma.

Capri Chasma

Large landslide deposits dominate this image of Ius Chasma captured by NASA's 2001 Mars Odyssey. Dunes are visible at the bottom of the frame.
Large landslide deposits dominate this image of Ius Chasma captured by NASA's 2001 Mars Odyssey. Dunes are visible at the bottom of the frame.

Ius Chasma

The mega gully in this image from NASA's 2001 Mars Odyssey spacecraft empties into Echus Chasma.
The mega gully in this image from NASA's 2001 Mars Odyssey spacecraft empties into Echus Chasma.

Mega Gully

This image from NASA's 2001 Mars Odyssey spacecraft shows part of Candor Chasma.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of Candor Chasma.

Candor Chasma

Dark slope streaks are common on the ridges of Lycus Sulci. These markings are thought to be formed by the removal of the brighter dust when material is shed from the top of the ridge. This image is from NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks are common on the ridges of Lycus Sulci. These markings are thought to be formed by the removal of the brighter dust when material is shed from the top of the ridge. This image is from NASA's 2001 Mars Odyssey spacecraft.

Lycus Sulci

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the northern flank of Hecates Tholus, which is located on the northern part of the Elysium Volcanic Complex.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the northern flank of Hecates Tholus, which is located on the northern part of the Elysium Volcanic Complex.

Hecates Tholus

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, which is mainly comprised of lava flows related to Arsia Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, which is mainly comprised of lava flows related to Arsia Mons.

Daedalia Planum

This small channel dissects the rim of an unnamed crater north of Terby Crater and Hellas Planitia as seen by NASA's 2001 Mars Odyssey spacecraft.
This small channel dissects the rim of an unnamed crater north of Terby Crater and Hellas Planitia as seen by NASA's 2001 Mars Odyssey spacecraft.

Channel

This unnamed channel is located in Arabia Terra, southwest of Meridiani Planum as seen by NASA's Mars Odyssey.
This unnamed channel is located in Arabia Terra, southwest of Meridiani Planum as seen by NASA's Mars Odyssey.

Channel in Arabia Terra

'Intrepid' crater on Mars carries the name of the lunar module of NASA's Apollo 12 mission, which landed on Earth's moon Nov. 19, 1969. NASA's Mars Exploration Rover Opportunity recorded this stereo view on Nov. 11, 2010. 3D glasses are necessary.
'Intrepid' crater on Mars carries the name of the lunar module of NASA's Apollo 12 mission, which landed on Earth's moon Nov. 19, 1969. NASA's Mars Exploration Rover Opportunity recorded this stereo view on Nov. 11, 2010. 3D glasses are necessary.

'Intrepid' Crater on Mars (Stereo)

This image from NASA's Mars Odyssey of part of Meridiani Planum contains windstreaks that formed in several directions around a single crater. This indicates that wind directions changed, forming new tails for each prevailing wind direction.
This image from NASA's Mars Odyssey of part of Meridiani Planum contains windstreaks that formed in several directions around a single crater. This indicates that wind directions changed, forming new tails for each prevailing wind direction.

Windstreaks on Meridiani Planum

Spurs and gullies form the cliff sides of the Vallis Marineris chasmata at top of this image captured by NASA's 2001 Mars Odyssey spacecraft. Sand dunes at the bottom of image are a common feature on the floors of the chasmata.
Spurs and gullies form the cliff sides of the Vallis Marineris chasmata at top of this image captured by NASA's 2001 Mars Odyssey spacecraft. Sand dunes at the bottom of image are a common feature on the floors of the chasmata.

Candor Chasma

This image from NASA's 2001 Mars Odyssey spacecraft shows dark slope streaks in an unnamed crater in Terra Sabaea. These features are believed to be formed by material moving downslope, removing the dust cover and revealing darker material.
This image from NASA's 2001 Mars Odyssey spacecraft shows dark slope streaks in an unnamed crater in Terra Sabaea. These features are believed to be formed by material moving downslope, removing the dust cover and revealing darker material.

Dark Slope Streaks

NASA's Mars Exploration Rover capturde this 360-degree view near the ridgeline of Endeavour Crater's western rim. The center is southeastward. Rocks on the slope to the right of center are in an outcrop area targeted for the rover to study.
NASA's Mars Exploration Rover capturde this 360-degree view near the ridgeline of Endeavour Crater's western rim. The center is southeastward. Rocks on the slope to the right of center are in an outcrop area targeted for the rover to study.

Approaching a Target Deposit on Mars Crater Rim

The flows in this image captured by NASA's 2001 Mars Odyssey spacecraft originated at Alba Mons.
The flows in this image captured by NASA's 2001 Mars Odyssey spacecraft originated at Alba Mons.

Alba Mons Flows

This image captured by NASA's 2001 Mars Odyssey spacecraft of Gale Crater shows the region of the crater that is 'home' to the Curiosity Rover.
This image captured by NASA's 2001 Mars Odyssey spacecraft of Gale Crater shows the region of the crater that is 'home' to the Curiosity Rover.

Gale Crater

Nirgal Vallis is one of the largest and longest valley networks on Mars as seen by NASA's Mars Reconnaissance Orbiter.
Nirgal Vallis is one of the largest and longest valley networks on Mars as seen by NASA's Mars Reconnaissance Orbiter.

Nirgal Vallis Tributaries

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