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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

Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.
Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.

Overlapping Lobate Lava Flows in Daedalia Planum

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

This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows in Daedalia Planum.
This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows in Daedalia Planum.

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive field of lava flows that make up Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive field of lava flows that make up Daedalia Planum.

Daedalia Planum

This image from NASA's Mars Odyssey spacecraft shows the eastern part of Hydrae Chasma.
This image from NASA's Mars Odyssey spacecraft shows the eastern part of Hydrae Chasma.

Hydrae Chasma

The parallel ridges in this image captured by NASA's Mars Odyssey spacecraft are part of Arsia Sulci - a region west of Arsia Mons. How these features were formed is unknown.
The parallel ridges in this image captured by NASA's Mars Odyssey spacecraft are part of Arsia Sulci - a region west of Arsia Mons. How these features were formed is unknown.

Arsia Sulci

This graph compares a typical daily pattern of changing atmospheric pressure (blue) with the pattern during a regional dust storm hundreds of miles away (red). The data are by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.
This graph compares a typical daily pattern of changing atmospheric pressure (blue) with the pattern during a regional dust storm hundreds of miles away (red). The data are by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.

Atmospheric Pressure Patterns Before and During Dust Storm

Impact craters can have a variety of floor features. This image from NASA's Mars Odyssey is a central peak/pit combination crater in Terra Cimmeria.
Impact craters can have a variety of floor features. This image from NASA's Mars Odyssey is a central peak/pit combination crater in Terra Cimmeria.

Crater Centers

This image from NASA's Mars Odyssey caputured on July 23, 2010 off the northern flank of Arsia Mons shows collapse/vent features.
This image from NASA's Mars Odyssey caputured on July 23, 2010 off the northern flank of Arsia Mons shows collapse/vent features.

Arsia Mons

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