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Ceraunius Fossae is the region of fractures and volcanic flows south of Alba Mons shown in this image captured by NASA's Mars Odyssey.
Ceraunius Fossae is the region of fractures and volcanic flows south of Alba Mons shown in this image captured by NASA's Mars Odyssey.

Ceraunius Fossae

This image from NASA's Mars Reconnaissance Orbiter spacecraft nicely captures several influential geologic processes that have shaped the landscape of Lycus Sulci.
This image from NASA's Mars Reconnaissance Orbiter spacecraft nicely captures several influential geologic processes that have shaped the landscape of Lycus Sulci.

Ridge and Talus in Lycus Sulci

Tithonium Chasma is a part of Valles Marineris, the largest canyon in the Solar System. If Valles Marineris was located on Earth it would span across almost the entire United States. This observation is from NASA's Mars Reconnaissance Orbiter spacecraft.
Tithonium Chasma is a part of Valles Marineris, the largest canyon in the Solar System. If Valles Marineris was located on Earth it would span across almost the entire United States. This observation is from NASA's Mars Reconnaissance Orbiter spacecraft.

Light-Toned Layers in Tithonium Chasma

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows a unique, resistant material on the floor of an unnamed crater.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows a unique, resistant material on the floor of an unnamed crater.

Terra Cimmeria Crater - False Color

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows the floor and rim of an unnamed crater in Terra Cimmeria.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows the floor and rim of an unnamed crater in Terra Cimmeria.

Crater - False Color

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

Crater Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows numerous gullies are visible on the cliff face of a depression within the floor of Lyell Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows numerous gullies are visible on the cliff face of a depression within the floor of Lyell Crater.

Lyell Crater

This image NASA's Mars Reconnaissance Orbiter shows an impact crater that was cut by lava in the Elysium Planitia region of Mars. It looks relatively flat, with a shallow floor, rough surface texture, and possible cooling cracks.
This image NASA's Mars Reconnaissance Orbiter shows an impact crater that was cut by lava in the Elysium Planitia region of Mars. It looks relatively flat, with a shallow floor, rough surface texture, and possible cooling cracks.

Which Way is Up?

This image captured by NASA's 2001 Mars Odyssey spacecraft spans from Tithonium Chasma (top of image) to Ius Chasma (bottom of image).
This image captured by NASA's 2001 Mars Odyssey spacecraft spans from Tithonium Chasma (top of image) to Ius Chasma (bottom of image).

Valles Marineris

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

Dunes

This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.
This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.

Mantled Terrain in the Southern Mid-Latitudes

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are near the large dune field called Olympia Undae.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are near the large dune field called Olympia Undae.

Polar Dunes

The cliff face in this image captured by NASA's 2001 Mars Odyssey spacecraft is called Rupes Tenius (rupes = scarp). The polar cap is the higher region to the left and the plains are located on the right side of the image.
The cliff face in this image captured by NASA's 2001 Mars Odyssey spacecraft is called Rupes Tenius (rupes = scarp). The polar cap is the higher region to the left and the plains are located on the right side of the image.

Rupes Tenuis

A delta deposit sits on the floor of this unnamed crater in Arabia Terra, as shown in this image from NASA's 2001 Mars Odyssey spacecraft. The channel that created the delta dissects the crater rim.
A delta deposit sits on the floor of this unnamed crater in Arabia Terra, as shown in this image from NASA's 2001 Mars Odyssey spacecraft. The channel that created the delta dissects the crater rim.

Crater Delta

The volcanic flows in this image captured by NASA's Mars Odyssey spacecraft are part of Daedalia Planum, an extensive flow field originating from Arsia Mons.
The volcanic flows in this image captured by NASA's Mars Odyssey spacecraft are part of Daedalia Planum, an extensive flow field originating from Arsia Mons.

Daedalia Planum

The volcanic flow in this image from NASA's 2001 Mars Odyssey spacecraft appears to have flowed in one layer. The surface texture is blocks of lava which cooled and still moved on molten lava below, producing the plate-like texture.
The volcanic flow in this image from NASA's 2001 Mars Odyssey spacecraft appears to have flowed in one layer. The surface texture is blocks of lava which cooled and still moved on molten lava below, producing the plate-like texture.

Lava

The main agent of erosion on Mars today is the wind. Wind has sculpted the surface in this region into a set of hills and valleys called yardangs on Earth. This image is from NASA's 2001 Mars Odyssey spacecraft.
The main agent of erosion on Mars today is the wind. Wind has sculpted the surface in this region into a set of hills and valleys called yardangs on Earth. This image is from NASA's 2001 Mars Odyssey spacecraft.

Erosion

This VIS image shows dunes in a topographic low within Aonia Terra.
This VIS image shows dunes in a topographic low within Aonia Terra.

Dunes

Daedalia Planum is comprised of lava flows from Arsia Mons. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
Daedalia Planum is comprised of lava flows from Arsia Mons. This image was captured by NASA's 2001 Mars Odyssey spacecraft.

Daedalia Planum

This scene shows the 'Murray Ridge' portion of the western rim of Endeavour Crater on Mars, as seen by NASA's Opportunity rover. It is presented in false color to make some differences between materials easier to see.
This scene shows the 'Murray Ridge' portion of the western rim of Endeavour Crater on Mars, as seen by NASA's Opportunity rover. It is presented in false color to make some differences between materials easier to see.

'Murray Ridge' on Rim of Endeavour Crater on Mars, False Color

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? These layered deposits look like a giant bear facing to the left.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? These layered deposits look like a giant bear facing to the left.

THEMIS Art #120

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the huge dune field located at the north polar cap. As spring continues to deepen, the dunes are becoming darker and darker as they lose their winter frost cover.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the huge dune field located at the north polar cap. As spring continues to deepen, the dunes are becoming darker and darker as they lose their winter frost cover.

North Polar Dunes

This image from NASA's Curiosity Rover shows a high-resolution view of an area that is known as Goulburn Scour, a set of rocks blasted by the engines of Curiosity's descent stage on Mars.
This image from NASA's Curiosity Rover shows a high-resolution view of an area that is known as Goulburn Scour, a set of rocks blasted by the engines of Curiosity's descent stage on Mars.

Best View of Goulburn Scour

This radargram profile from ESA's Mars Express and NASA's Mars Global Surveyor orbiter shows data from the subsurface of Mars in the ice-rich north polar plateau of Mars.
This radargram profile from ESA's Mars Express and NASA's Mars Global Surveyor orbiter shows data from the subsurface of Mars in the ice-rich north polar plateau of Mars.

Radargram of Mars North Polar Plateau from Mars Express

This image from NASA's Mars Odyssey shows different flow surfaces in Daedalia Planum.
This image from NASA's Mars Odyssey shows different flow surfaces in Daedalia Planum.

Daedalia Planum

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