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This image from NASA's 2001 Mars Odyssey spacecraft shows small sets of dunes on the plains of Aonia Terra.
This image from NASA's 2001 Mars Odyssey spacecraft shows small sets of dunes on the plains of Aonia Terra.

Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the weathering of the eastern side of Mt. Sharp.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the weathering of the eastern side of Mt. Sharp.

Images of Gale #10

This image, taken NASA's Mars Reconnaissance Orbiter, shows distinct bands of alternating tone and brightness within the 'Murray Formation' on Mars. Outcrops like this are common throughout the formation.
This image, taken NASA's Mars Reconnaissance Orbiter, shows distinct bands of alternating tone and brightness within the 'Murray Formation' on Mars. Outcrops like this are common throughout the formation.

Bands on the 'Murray Formation'

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 image from NASA's Mars Reconnaissance Orbiter captures light-toned ridges found in a large fracture located east of Holden Crater forming a curious box-like pattern.
This image from NASA's Mars Reconnaissance Orbiter captures light-toned ridges found in a large fracture located east of Holden Crater forming a curious box-like pattern.

Many Small Interesting Ridges in Erythraea Fossa

This image shows part of the sand sheet and dunes on the floor of Rabe Crater as seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows part of the sand sheet and dunes on the floor of Rabe Crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Rabe Crater Dunes

The complex channel and streamlined islands are part of Maja Valles as seen by NASA's 2001 Mars Odyssey spacecraft.
The complex channel and streamlined islands are part of Maja Valles as seen by NASA's 2001 Mars Odyssey spacecraft.

Maja Valles

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft were most likely created by lava flows from Alba Mons, located in the northern Tharsis region.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft were most likely created by lava flows from Alba Mons, located in the northern Tharsis region.

Channels

More dunes are encountered surrounding the north polar cap by NASA's 2001 Mars Odyssey spacecraft.
More dunes are encountered surrounding the north polar cap by NASA's 2001 Mars Odyssey spacecraft.

More Polar Dunes

This artist's impression Mars' Gale Crater depicts a cross section through the mountain in the middle of the crater, from a viewpoint looking toward the southeast. NASA's rover Curiosity will land in Gale Crater in August 2012.
This artist's impression Mars' Gale Crater depicts a cross section through the mountain in the middle of the crater, from a viewpoint looking toward the southeast. NASA's rover Curiosity will land in Gale Crater in August 2012.

Cross Section of Gale Crater, Mars

The region shown in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Gigas Sulci.
The region shown in this image captured by NASA's 2001 Mars Odyssey spacecraft is part of Gigas Sulci.

Gigas Sulci

This set of images illustrates how the science filters of the Mast Camera (Mastcam) on NASA's Mars rover Curiosity can be used to investigate aspects of the composition and mineralogy of materials on Mars.
This set of images illustrates how the science filters of the Mast Camera (Mastcam) on NASA's Mars rover Curiosity can be used to investigate aspects of the composition and mineralogy of materials on Mars.

Drill Hole Image and Spectra Acquired by Mastcam

The unnamed channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is located on the northeastern margin of Tempe Terra.
The unnamed channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is located on the northeastern margin of Tempe Terra.

Tempe Terra

Just as on Earth, volcanism and tectonism are found together on Mars. In this image from NASA's 2001 Mars Odyssey spacecraft the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Planum.
Just as on Earth, volcanism and tectonism are found together on Mars. In this image from NASA's 2001 Mars Odyssey spacecraft the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Planum.

Volcanism & Tectonism

NASA's Mars Reconnaissance Orbiter reveals underground ice exposed by impact cratering. The impact that dug the crater excavated water ice from beneath the surface.
NASA's Mars Reconnaissance Orbiter reveals underground ice exposed by impact cratering. The impact that dug the crater excavated water ice from beneath the surface.

Underground Ice on Mars Exposed by Impact Cratering

A surprise landslump in Melas Chasma was observed by NASA's Mars Reconnaissance Orbiter.
A surprise landslump in Melas Chasma was observed by NASA's Mars Reconnaissance Orbiter.

A Surprise Landslump in Melas Chasma

Multiple channels dissect the rim of this unnamed crater in Noachis Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
Multiple channels dissect the rim of this unnamed crater in Noachis Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Rim Channels

This image from NASA's Mars Odyssey spacecraft shows Gale crater, which is east of the landing site. It shows the northern extent of the dunes, and the layers in Mt. Sharp are visible at the bottom of the image.
This image from NASA's Mars Odyssey spacecraft shows Gale crater, which is east of the landing site. It shows the northern extent of the dunes, and the layers in Mt. Sharp are visible at the bottom of the image.

Images of Gale #3

Channels are a common feature on the margin of Terra Cimmeria where the elevation changes from highland to northern lowlands in this image captured by NASA's Mars Odyssey.
Channels are a common feature on the margin of Terra Cimmeria where the elevation changes from highland to northern lowlands in this image captured by NASA's Mars Odyssey.

Channels on Terra Cimmeria

NASA's Mars Odyssey captured this image of Ulysses Fossae, located in the Tharsis Volcanic region. Cross cutting tectonic fractures indicate that this region underwent stresses in multiple directions.
NASA's Mars Odyssey captured this image of Ulysses Fossae, located in the Tharsis Volcanic region. Cross cutting tectonic fractures indicate that this region underwent stresses in multiple directions.

Ulysses Fossae

This observation from NASA's Mars Reconnaissance Orbiter covers an outcrop of possible cyclic bedding within a crater in Arabia Terra.
This observation from NASA's Mars Reconnaissance Orbiter covers an outcrop of possible cyclic bedding within a crater in Arabia Terra.

Possible Cyclic Bedding within a Crater in Arabia Terra

This image shows a portion of the dunes on the floor of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft.
This image shows a portion of the dunes on the floor of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft.

Rabe Crater Dunes

The channels in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are called Hephaestus Fossae and were most likely formed by lava flow and erosion rather than being eroded by water.
The channels in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are called Hephaestus Fossae and were most likely formed by lava flow and erosion rather than being eroded by water.

Hephaestus Fossae

This NASA 2001 Mars Odyssey image of the southwestern flank of Alba Mons shows lava flows and collapse features.
This NASA 2001 Mars Odyssey image of the southwestern flank of Alba Mons shows lava flows and collapse features.

Alba Mons

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