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Multiple landslide deposits are visible in this image of Ganges Chasma captured by NASA's 2001 Mars Odyssey spacecraft.
Multiple landslide deposits are visible in this image of Ganges Chasma captured by NASA's 2001 Mars Odyssey spacecraft.

Ganges Chasma

A region known as 'Cape York' on the western rim of Endeavour Crater, where the Opportunity rover worked for 20 months, is highlighted in these images from NASA's Mars Reconnaissance Orbiter.
A region known as 'Cape York' on the western rim of Endeavour Crater, where the Opportunity rover worked for 20 months, is highlighted in these images from NASA's Mars Reconnaissance Orbiter.

'Cape York' Explored

The pits in this image from NASA's 2001 Mars Odyssey spacecraft are collapse features on the northern flank of Ascraeus Mons.
The pits in this image from NASA's 2001 Mars Odyssey spacecraft are collapse features on the northern flank of Ascraeus Mons.

Ascraeus Mons

At the bottom of this image from NASA's Mars Odyssey is the cliff-face that is the sidewall of Ophir Chasma. Layering is easily visible in the upper cliff wall, with the thickness of the surface clearly visible.
At the bottom of this image from NASA's Mars Odyssey is the cliff-face that is the sidewall of Ophir Chasma. Layering is easily visible in the upper cliff wall, with the thickness of the surface clearly visible.

Layering

Echus Chasma separates the Tharsis region from Lunae Planum. This image from NASA's 2001 Mars Odyssey shows volcanic flow materials from Tharsis within the chasma.
Echus Chasma separates the Tharsis region from Lunae Planum. This image from NASA's 2001 Mars Odyssey shows volcanic flow materials from Tharsis within the chasma.

Echus Chasma

This image of Zephyria Planum, taken by NASA's 2001 Mars Odyssey spacecraft, shows wind eroded yardangs.
This image of Zephyria Planum, taken by NASA's 2001 Mars Odyssey spacecraft, shows wind eroded yardangs.

Yardangs on Zephyria Planum

The full-circle panorama in approximately true color taken by NASA's Phoenix Mars Lander shows the polygonal patterning of ground at the landing area, similar to patterns in permafrost areas on Earth.
The full-circle panorama in approximately true color taken by NASA's Phoenix Mars Lander shows the polygonal patterning of ground at the landing area, similar to patterns in permafrost areas on Earth.

Full-Circle Color Panorama of Phoenix Landing Site on Northern Mars

This image shows part of Rubicon Valles located on the northwestern flank of Alba Mons seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows part of Rubicon Valles located on the northwestern flank of Alba Mons seen by NASA's 2001 Mars Odyssey spacecraft.

Rubicon Valles

This image from NASA's 2001 Mars Odyssey shows dunes located on the floor of Proctor Crater.
This image from NASA's 2001 Mars Odyssey shows dunes located on the floor of Proctor Crater.

Proctor Crater Dunes

The floor of Eos Chasma is composed of thousands of small hills; this type of terrain is called
The floor of Eos Chasma is composed of thousands of small hills; this type of terrain is called

Eos Chaos

Located to the northeast of Olympus Mons, Cyane Sulci is a complexly fractured region of material inundated on its margins by volcanic flows. This image was captured by NASA's Mars Odyssey on Oct. 24, 2010.
Located to the northeast of Olympus Mons, Cyane Sulci is a complexly fractured region of material inundated on its margins by volcanic flows. This image was captured by NASA's Mars Odyssey on Oct. 24, 2010.

Cyane Sulci

This image taken by NASA's 2001 Mars Odyssey shows lava flows and tectonic features related to the Arsia Mons volcanic system. The tectonic graben (downdropped blocks bounded by faults) are called Oti Fossae.
This image taken by NASA's 2001 Mars Odyssey shows lava flows and tectonic features related to the Arsia Mons volcanic system. The tectonic graben (downdropped blocks bounded by faults) are called Oti Fossae.

Oti Fossae

Dunes forms top this sand sheet in the plains of Aonia Terra in this image captured by NASA's Mars Odyssey.
Dunes forms top this sand sheet in the plains of Aonia Terra in this image captured by NASA's Mars Odyssey.

Dunes in Aonia Terra

The southern rim of this unnamed crater in Tempe Terra is dissected by numerous gullies in this image captured by NASA's Mars Odyssey.
The southern rim of this unnamed crater in Tempe Terra is dissected by numerous gullies in this image captured by NASA's Mars Odyssey.

Gullies in Tempe Terra

This observation from NASA's Mars Reconnaissance Orbiter shows a small portion of Mawrth Vallis, one of the many outflow channels feeding north into the Chryse Basin. This ancient valley once hosted flowing water.
This observation from NASA's Mars Reconnaissance Orbiter shows a small portion of Mawrth Vallis, one of the many outflow channels feeding north into the Chryse Basin. This ancient valley once hosted flowing water.

Mawrth Vallis Geodiversity

This NASA Mars Odyssey image covers a tract of plateau territory called Ophir Planum. The most obvious features in this scene are the fractures (ranging from 1 to 5 km wide) running from the upper left to lower right.
This NASA Mars Odyssey image covers a tract of plateau territory called Ophir Planum. The most obvious features in this scene are the fractures (ranging from 1 to 5 km wide) running from the upper left to lower right.

Crustal Fractures of Ophir Planum

This is a more recent 'geometrically improved, color enhanced' version of the 360-degree 'Gallery Pan,' the first contiguous, uniform panorama taken by the Imager for Mars (IMP) over the course of Sols 8, 9, and 10.
This is a more recent 'geometrically improved, color enhanced' version of the 360-degree 'Gallery Pan,' the first contiguous, uniform panorama taken by the Imager for Mars (IMP) over the course of Sols 8, 9, and 10.

Improved MPF 360-degree Color Panorama

This image captured by NASA's 2001 Mars Odyssey spacecraft show the dark marks left behind after the passage of a dust devil cover this region of Utopia Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft show the dark marks left behind after the passage of a dust devil cover this region of Utopia Planitia.

Utopia Planitia

This image from NASA's Mars Reconnaissance Orbiter shows one of these icy lobate features wrapping around a small hill. Many lobate features are now known to be almost pure ice, like glaciers on the Earth.
This image from NASA's Mars Reconnaissance Orbiter shows one of these icy lobate features wrapping around a small hill. Many lobate features are now known to be almost pure ice, like glaciers on the Earth.

Martian Glaciers and Brain Terrain

This color-coded elevation map of the local terrain on the north side of NASA's Phoenix Mars Lander shows the contours of polygons and relationship of polygon boundaries to trenches and other features in the workspace of the lander's Robotic Arm.
This color-coded elevation map of the local terrain on the north side of NASA's Phoenix Mars Lander shows the contours of polygons and relationship of polygon boundaries to trenches and other features in the workspace of the lander's Robotic Arm.

Contour Map of Mars' Surface Beside Phoenix

This colorglyph, acquired by NASA's Phoenix Lander's Surface Stereo Imager shows part of Phoenix's workplace and is informally called 'Wonderland.' 3D glasses are necessary to view this image.
This colorglyph, acquired by NASA's Phoenix Lander's Surface Stereo Imager shows part of Phoenix's workplace and is informally called 'Wonderland.' 3D glasses are necessary to view this image.

Martian Surface as Seen by Phoenix

This image from the HiRISE instrument on NASA's Mars Reconnaissance Orbiter shows 'Victoria crater,' an impact crater at Meridiani Planum, near the equator of Mars.
This image from the HiRISE instrument on NASA's Mars Reconnaissance Orbiter shows 'Victoria crater,' an impact crater at Meridiani Planum, near the equator of Mars.

'Victoria Crater' at Meridiani Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the dunes on the floor of Darwin Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows some of the dunes on the floor of Darwin Crater.

Darwin Crater Dunes

Moving further east, this image from NASA's Mars Odyssey spacecraft shows the southern extent of Mt. Sharp as well as the crater floor and rim. In this image there are small dunes near Mt. Sharp as well as dunes near the crater rim.
Moving further east, this image from NASA's Mars Odyssey spacecraft shows the southern extent of Mt. Sharp as well as the crater floor and rim. In this image there are small dunes near Mt. Sharp as well as dunes near the crater rim.

Images of Gale #32

The dust devil tracks in this VIS image are located in Terra Cimmeria.
The dust devil tracks in this VIS image are located in Terra Cimmeria.

Dust Devil Tracks

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