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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

NASA's 2001 Mars Odyssey captured this image of individual dunes located on the floor of Briault Crater.
NASA's 2001 Mars Odyssey captured this image of individual dunes located on the floor of Briault Crater.

Briault Crater Dunes

Several landslide deposits are visible in this image of Coprates Chasma taken by NASA's 2001 Mars Odyssey spacecraft.
Several landslide deposits are visible in this image of Coprates Chasma taken by NASA's 2001 Mars Odyssey spacecraft.

Several Landslides on Coprates Chasma

The mitten-shaped feature in Candor Chasma is a landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft.
The mitten-shaped feature in Candor Chasma is a landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft.

Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Sulci Gordii, a complexly fractured region east of Olympus Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Sulci Gordii, a complexly fractured region east of Olympus Mons.

Sulci Gordii

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Siton Undae, one of the dune fields near the north polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Siton Undae, one of the dune fields near the north polar cap.

Siton Undae

The dunes seen in this view from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Brashear Crater.
The dunes seen in this view from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Brashear Crater.

Brashear Crater Dunes

The graben in this image from NASA's 2001 Mars Odyssey spacecraft is Cyane Fossae. The lava flows are part of the extensive Tharsis volcanic flows.
The graben in this image from NASA's 2001 Mars Odyssey spacecraft is Cyane Fossae. The lava flows are part of the extensive Tharsis volcanic flows.

Cyane Fossae

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Elysium Planitia and were likely created by lava flow.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Elysium Planitia and were likely created by lava flow.

Channels

This pair of graphs shows about one-fourth of a Martian year's record of temperatures (in degrees Celsius) measured by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.
This pair of graphs shows about one-fourth of a Martian year's record of temperatures (in degrees Celsius) measured by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.

Steady Temperatures at Mars' Gale Crater

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

Brashear Dunes

This image from NASA's 2001 Mars Odyssey spacecraft of a ridge in the Tharsis region (called Uranius Dorsum) reminds one of a skeletal spine.
This image from NASA's 2001 Mars Odyssey spacecraft of a ridge in the Tharsis region (called Uranius Dorsum) reminds one of a skeletal spine.

Uranius Dorsum

The channel-like features in image captured by NASA's 2001 Mars Odyssey spacecraft are fracture sets related to the formation of Iani Chaos, which occurs directly north of the image.
The channel-like features in image captured by NASA's 2001 Mars Odyssey spacecraft are fracture sets related to the formation of Iani Chaos, which occurs directly north of the image.

Iani Chaos

This image from NASA's Mars Odyssey shows a portion of a large landslide deposit in Ius Chasma.
This image from NASA's Mars Odyssey shows a portion of a large landslide deposit in Ius Chasma.

Ius Chasma Landslide

As northern summer approaches on Mars, dunes near the pole defrost and become darker appearing as shown in this image from NASA's Mars Odyssey captured on July 8, 2010.
As northern summer approaches on Mars, dunes near the pole defrost and become darker appearing as shown in this image from NASA's Mars Odyssey captured on July 8, 2010.

Polar Dunes

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