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This image from NASA's Mars Reconnaissance Orbiter (MRO) is part of simulated flyover showing rhythmic layers of sedimentary rock inside Becquerel crater on Mars.
This image from NASA's Mars Reconnaissance Orbiter (MRO) is part of simulated flyover showing rhythmic layers of sedimentary rock inside Becquerel crater on Mars.

Flyover Animation of Becquerel Crater on Mars

The numerous valleys in this image captured by NASA's 2001 Mars Odyssey spacecra are dissecting part of Aonia Terra.
The numerous valleys in this image captured by NASA's 2001 Mars Odyssey spacecra are dissecting part of Aonia Terra.

Valley Networks

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the dune field on the floor of Nili Patera.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the dune field on the floor of Nili Patera.

Nili Patera Dunes

A large pile of sand with dune features on its surface is located on the floor of Matara Crater as seen by NASA's 2001 Mars Odyssey spacecraft.
A large pile of sand with dune features on its surface is located on the floor of Matara Crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Matara Crater

This mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 122.2-meter (401-foot) drive on Oct. 25, 2010. 3D glasses are necessary.
This mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 122.2-meter (401-foot) drive on Oct. 25, 2010. 3D glasses are necessary.

Opportunity's Eastward View After Sol 2401 Drive (Stereo)

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the eastern part of Coprates Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the eastern part of Coprates Chasma.

Coprates Chasma

This image captured by NASA's 2001 Mars Odyssey of Elator Vallis shows where a crater has deflected flow and created a streamlined island.
This image captured by NASA's 2001 Mars Odyssey of Elator Vallis shows where a crater has deflected flow and created a streamlined island.

Elator Vallis

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Hussey Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Hussey Crater.

Hussey Crater Dunes

The dunes in this unnamed crater in Aonia Terra are coalescing into a sand sheet in this image from NASA's 2001 Mars Odyssey spacecraft.
The dunes in this unnamed crater in Aonia Terra are coalescing into a sand sheet in this image from NASA's 2001 Mars Odyssey spacecraft.

V43209003

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Ares Vallis.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Ares Vallis.

Ares Vallis

This image captured by NASA's 2001 Mars Odyssey spacecraft shows more north polar dunes.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows more north polar dunes.

More Polar Dunes

This daytime IR image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the patera (summit depression) and eroded flank of Hadriacus Mons at the top of the image and a section of Dao Vallis at the bottom of the image.
This daytime IR image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the patera (summit depression) and eroded flank of Hadriacus Mons at the top of the image and a section of Dao Vallis at the bottom of the image.

Hadriaca and Dao

The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on Olympus Mons, the largest volcano in the solar system.
The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on Olympus Mons, the largest volcano in the solar system.

Olympus Mons Flows

The Rover Environmental Monitoring Station (REMS) on NASA's Curiosity Mars rover has detected dozens of whirlwinds, or vortex events, causing brief dips in atmospheric pressure, and sometimes other measurable effects.
The Rover Environmental Monitoring Station (REMS) on NASA's Curiosity Mars rover has detected dozens of whirlwinds, or vortex events, causing brief dips in atmospheric pressure, and sometimes other measurable effects.

Whirlwind Detection by Curiosity in Gale Crater

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a field of dunes on the floor of an unnamed crater in Terra Cimmeria.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a field of dunes on the floor of an unnamed crater in Terra Cimmeria.

Crater Dunes

A rippled patch of sand in Becquerel Crater on Mars moved about two meters (about two yards) between November 24, 2006 and September 5, 2010, in one of two images taken by NASA's Mars Reconnaissance Orbiter.
A rippled patch of sand in Becquerel Crater on Mars moved about two meters (about two yards) between November 24, 2006 and September 5, 2010, in one of two images taken by NASA's Mars Reconnaissance Orbiter.

Blowing in the Martian Wind

This image from NASA's 2001 Mars Odyssey spacecraft shows several large channels emptying into the eastern Hellas Basin. These southern channels are filled with material today. Whether the material contains volitiles (like ice) is unknown.
This image from NASA's 2001 Mars Odyssey spacecraft shows several large channels emptying into the eastern Hellas Basin. These southern channels are filled with material today. Whether the material contains volitiles (like ice) is unknown.

Reull Vallis

Centuries of wind action have sculpted the surface materials shown this image from NASA's 2001 Mars Odyssey.
Centuries of wind action have sculpted the surface materials shown this image from NASA's 2001 Mars Odyssey.

Wind Erosion

This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the vast lava flow fields between Echus Chasma and the main Tharsis volcanoes.
This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the vast lava flow fields between Echus Chasma and the main Tharsis volcanoes.

Tharsis Volcanics

A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 (3,300 feet) wide. This image is from NASA's Mars Odyssey.
A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 (3,300 feet) wide. This image is from NASA's Mars Odyssey.

Mars Odyssey All Stars: Dunes Engulf Crater

Most of the hills in this image from NASA's 2001 Mars Odyssey spacecraft have dark streaks thought to be where bright dust has been removed by sliding down the hillside.
Most of the hills in this image from NASA's 2001 Mars Odyssey spacecraft have dark streaks thought to be where bright dust has been removed by sliding down the hillside.

Down the Hill

The unusual surface texture seen in the image from NASA's 2001 Mars Odyssey spacecraft reflects the resistance of the surface rocks to erosion by the wind. This image shows part of the northern end of Gordii Dorsum.
The unusual surface texture seen in the image from NASA's 2001 Mars Odyssey spacecraft reflects the resistance of the surface rocks to erosion by the wind. This image shows part of the northern end of Gordii Dorsum.

Wind Erosion

This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the lava flows located east of the large Tharsis volcanoes.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the lava flows located east of the large Tharsis volcanoes.

Lava Flows

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in an unnamed crater on the eastern margin of Tempe Terra.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in an unnamed crater on the eastern margin of Tempe Terra.

Dunes

Now that summer has arrived in the northern hemisphere of Mars, the dunes near the polar cap have shed all their winter frost, as shown in this image from NASA's 2001 Mars Odyssey spacecraft.
Now that summer has arrived in the northern hemisphere of Mars, the dunes near the polar cap have shed all their winter frost, as shown in this image from NASA's 2001 Mars Odyssey spacecraft.

North Polar Dunes

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