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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

The dunes in this daytime IR image from NASA's 2001 Mars Odyssey spacecraft appear bright because they are warmer than the surrounding crater materials. These dunes are located on the floor of Proctor Crater.
The dunes in this daytime IR image from NASA's 2001 Mars Odyssey spacecraft appear bright because they are warmer than the surrounding crater materials. These dunes are located on the floor of Proctor Crater.

Proctor Crater Dunes

The small channel in this image from NASA's 2001 Mars Odyssey spacecraft runs semi-parallel to Shalbatana Vallis in Xanthe Terra.
The small channel in this image from NASA's 2001 Mars Odyssey spacecraft runs semi-parallel to Shalbatana Vallis in Xanthe Terra.

Channel

The volcanic flows that comprise Daedalia Planum arose from Arsia Mons. This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, including a channel-fed lava flow.
The volcanic flows that comprise Daedalia Planum arose from Arsia Mons. This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, including a channel-fed lava flow.

Daedalia Planum

As the sun warms the surface and more frost is removed, the dunes and other features near the north pole of Mars are revealed. This image from NASA's Mars Odyssey shows that the inter-dune areas are complex.
As the sun warms the surface and more frost is removed, the dunes and other features near the north pole of Mars are revealed. This image from NASA's Mars Odyssey shows that the inter-dune areas are complex.

North Polar Dunes

This image from NASA's Mars Odyssey is an unnamed crater in the far northern lowlands containing a sand sheet with dune forms on its floor. Many craters this close to the pole contain similar dune fields.
This image from NASA's Mars Odyssey is an unnamed crater in the far northern lowlands containing a sand sheet with dune forms on its floor. Many craters this close to the pole contain similar dune fields.

Dunes

This stereo view from the Navigation Camera (Navcam) on NASA's Curiosity Mars rover shows the terrain ahead of the rover as it makes its way westward through a valley called
This stereo view from the Navigation Camera (Navcam) on NASA's Curiosity Mars rover shows the terrain ahead of the rover as it makes its way westward through a valley called

Curiosity View Ahead Through 'Artist's Drive' (Stereo)

This observation from NASA's Mars Reconnaissance Orbiter shows the nature of large fissures in a smooth apron around a mound in the Phlegra region.
This observation from NASA's Mars Reconnaissance Orbiter shows the nature of large fissures in a smooth apron around a mound in the Phlegra region.

Cracks in a Debris Apron

This image shows a possible landing site for the 2020 Mission: Jezero Crater, as seen by NASA's Mars Reconnaissance Orbiter.
This image shows a possible landing site for the 2020 Mission: Jezero Crater, as seen by NASA's Mars Reconnaissance Orbiter.

A Possible Landing Site for the 2020 Mission: Jezero Crater

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the flank of Hecates Tholus.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the flank of Hecates Tholus.

Hecates Tholus - False Color

The depression in the center of this image captured by NASA's 2001 Mars Odyssey spacecraft is a graben (fault bounded block of material). This graben is called Mangala Fossa.
The depression in the center of this image captured by NASA's 2001 Mars Odyssey spacecraft is a graben (fault bounded block of material). This graben is called Mangala Fossa.

Mangala Fossa

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the layering of the north polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the layering of the north polar cap.

Polar Layers

Eridania Basin, located at the head of Ma'adim Vallis, has mounting geomorphic and spectral evidence that it may have been the site of an ancient inland sea. This image is from NASA's Mars Reconnaissance Orbiter.
Eridania Basin, located at the head of Ma'adim Vallis, has mounting geomorphic and spectral evidence that it may have been the site of an ancient inland sea. This image is from NASA's Mars Reconnaissance Orbiter.

Ridges in Eridania Basin

This complex channel is located in the Nili Fossae region as seen by NASA's 2001 Mars Odyssey spacecraft.
This complex channel is located in the Nili Fossae region as seen by NASA's 2001 Mars Odyssey spacecraft.

Channel

With summer fast approaching, the frost has sublimated away and the layers that make up the north polar cap are easily discernable, as seen by NASA's 2001 Mars Odyssey spacecraft.
With summer fast approaching, the frost has sublimated away and the layers that make up the north polar cap are easily discernable, as seen by NASA's 2001 Mars Odyssey spacecraft.

Spring at the North Pole

Following the dunes eastward, we find several channels dissecting the crater rim in this image from NASA's Mars Odyssey spacecraft. These channels may be the source of material for the sand dunes.
Following the dunes eastward, we find several channels dissecting the crater rim in this image from NASA's Mars Odyssey spacecraft. These channels may be the source of material for the sand dunes.

Images of Gale #30

A network of small channels is visible in image from NASA's 2001 Mars Odyssey spacecraft.
A network of small channels is visible in image from NASA's 2001 Mars Odyssey spacecraft.

Channels

The triple tails of windstreaks behind these small craters in Arabia Terra indicate multiple wind directions in the area in this image from NASA's Mars Odyssey.
The triple tails of windstreaks behind these small craters in Arabia Terra indicate multiple wind directions in the area in this image from NASA's Mars Odyssey.

Triple Tails of Windstreaks

Sample material from the fourth scoop of Martian soil collected by NASA's Mars rover Curiosity is on the rover's observation tray in this image taken during the mission's 78th Martian sol, (Oct. 24, 2012) by Curiosity's left Navigation Camera.
Sample material from the fourth scoop of Martian soil collected by NASA's Mars rover Curiosity is on the rover's observation tray in this image taken during the mission's 78th Martian sol, (Oct. 24, 2012) by Curiosity's left Navigation Camera.

Scooped Material on Rover's Observation Tray

This image from NASA's 2001 Mars Odyssey spacecraft shows a small landslide chute and deposit. This feature is located on the easternmost end of Candor Chasma.
This image from NASA's 2001 Mars Odyssey spacecraft shows a small landslide chute and deposit. This feature is located on the easternmost end of Candor Chasma.

Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft crosses the summit of Uranius Tholus, as well as the western flank of Ceraunius Tholus.
This image captured by NASA's 2001 Mars Odyssey spacecraft crosses the summit of Uranius Tholus, as well as the western flank of Ceraunius Tholus.

Uranius Tholus

The fractures in this image are part of a large system of fractures called Cerberus Fossae. Athabasca Valles is visible in the lower right corner of the image as seen by NASA's 2001 Mars Odyssey spacecraft.
The fractures in this image are part of a large system of fractures called Cerberus Fossae. Athabasca Valles is visible in the lower right corner of the image as seen by NASA's 2001 Mars Odyssey spacecraft.

Cerberus Fossae

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern flank of Elysium Mons. The small channels were likely created due to the flow of lava, rather than water.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern flank of Elysium Mons. The small channels were likely created due to the flow of lava, rather than water.

Elysium Mons

This small landslide deposit is located in an unnamed crater in Margaritifer Terra in this image captured by NASA's 2001 Mars Odyssey spacecraft.
This small landslide deposit is located in an unnamed crater in Margaritifer Terra in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Landslide

Multiple layers of material are located in Terby Crater in this image from NASA's 2001 Mars Odyssey.
Multiple layers of material are located in Terby Crater in this image from NASA's 2001 Mars Odyssey.

Terby Crater

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