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Several landslides occurred on this steep cliff face in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Several landslides occurred on this steep cliff face in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Landslide

This unnamed crater in northern Terra Cimmeria has a small channel that created a delta feature. Such features are important indicators of liquid water in Mars' past as shown in this image from NASA's Mars Odyssey.
This unnamed crater in northern Terra Cimmeria has a small channel that created a delta feature. Such features are important indicators of liquid water in Mars' past as shown in this image from NASA's Mars Odyssey.

Delta in Terra Cimmeria

This map shows the path that NASA's Mars Exploration Rover Spirit followed from the 743rd Martian day (Feb. 4, 2009), or sol, to Sol 2471 (Dec. 15, 2010). Spirit has been at a sand-trap location called 'Troy' since April 2009.
This map shows the path that NASA's Mars Exploration Rover Spirit followed from the 743rd Martian day (Feb. 4, 2009), or sol, to Sol 2471 (Dec. 15, 2010). Spirit has been at a sand-trap location called 'Troy' since April 2009.

Spirit Traverse Map, Sol 2471

The north/south trending parallel hills and valleys in this image captured by NASA's 2001 Mars Odyssey spacecraft were created by wind erosion and are called yardangs. These yardangs are located in Zephyria Planum.
The north/south trending parallel hills and valleys in this image captured by NASA's 2001 Mars Odyssey spacecraft were created by wind erosion and are called yardangs. These yardangs are located in Zephyria Planum.

Yardangs

This map shows where NASA's Mars rover Curiosity landed in August 2012 at 'Bradbury Landing.' All of these features are inside Gale Crater. Curiosity's next major destination, the entry point to the base of Mount Sharp.
This map shows where NASA's Mars rover Curiosity landed in August 2012 at 'Bradbury Landing.' All of these features are inside Gale Crater. Curiosity's next major destination, the entry point to the base of Mount Sharp.

From 'Glenelg' to Mount Sharp

The sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Hargraves Crater.
The sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Hargraves Crater.

Hargraves Crater Dunes

The dark lobed material in this image from NASA's 2001 Mars Odyssey spacecraft is a lava flow located northwest of the Elysium Volcanic Complex.
The dark lobed material in this image from NASA's 2001 Mars Odyssey spacecraft is a lava flow located northwest of the Elysium Volcanic Complex.

Lava Channel

This image captured by NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel located on the northwest margin of Arabia Terra.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel located on the northwest margin of Arabia Terra.

Channel

The surface textures located southeast of Aeolis Planum likely had wind action as one of the contributing processes, as shown by NASA's 2001 Mars Odyssey spacecraft.
The surface textures located southeast of Aeolis Planum likely had wind action as one of the contributing processes, as shown by NASA's 2001 Mars Odyssey spacecraft.

Surface Textures

The ridges and mesas in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Hydraotes Chaos.
The ridges and mesas in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Hydraotes Chaos.

Hydraotes Chaos

At the eastern end of Valles Marineris the chasma floors are typically filled with the hills and mounds of chaos terrain as seen by NASA's Mars Odyssey.
At the eastern end of Valles Marineris the chasma floors are typically filled with the hills and mounds of chaos terrain as seen by NASA's Mars Odyssey.

Eos Chasma

The channel feature in this image from NASA's 2001 Mars Odyssey spacecraft is a huge gully that empties into Echus Chasma.
The channel feature in this image from NASA's 2001 Mars Odyssey spacecraft is a huge gully that empties into Echus Chasma.

Mega Gully

This image from NASA's Mars Odyssey is of the south polar surface. These pits appear to coalesce and reveal the surface below.
This image from NASA's Mars Odyssey is of the south polar surface. These pits appear to coalesce and reveal the surface below.

South Polar Surface

Located on the margin of Zephyria Planum, this image from NASA's 2001 Mars Odyssey shows the effect the wind has had on the surface of Mars. Loose materials have been removed and semi-consolidated materials have been eroded into narrow hill forms.
Located on the margin of Zephyria Planum, this image from NASA's 2001 Mars Odyssey shows the effect the wind has had on the surface of Mars. Loose materials have been removed and semi-consolidated materials have been eroded into narrow hill forms.

Wind Effects

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Aspledon Undae, a region of dunes near the north pole. The right side of the image shows hundreds of small, isolated dunes.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Aspledon Undae, a region of dunes near the north pole. The right side of the image shows hundreds of small, isolated dunes.

Aspledon Undae

This image from NASA's 2001 Mars Odyssey spacecraft shows several channels dissecting the rim of Semeykin Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows several channels dissecting the rim of Semeykin Crater.

Semeykin Crater

This image captured by NASA's 2001 Mars Odyssey spacecraf shows a portion of Patapsco Vallis, located on the eastern margin of the Elysium volcanic complex.
This image captured by NASA's 2001 Mars Odyssey spacecraf shows a portion of Patapsco Vallis, located on the eastern margin of the Elysium volcanic complex.

Patapsco Vallis

The windstreaks in this image from NASA's 2001 Mars Odyssey spacecraft are located on the volcanic plains of Daedalia Planum.
The windstreaks in this image from NASA's 2001 Mars Odyssey spacecraft are located on the volcanic plains of Daedalia Planum.

Windstreaks

The sand dunes in this image from NASA's Mars Odyssey are located on the floor of Russell Crater.
The sand dunes in this image from NASA's Mars Odyssey are located on the floor of Russell Crater.

Russell Crater Dunes

Maumee Valles is the main channel visible in this image captured by NASA's Mars Odyssey.
Maumee Valles is the main channel visible in this image captured by NASA's Mars Odyssey.

Maumee Valles

On this map of Mars, spectrometers on spacecraft orbiting Mars have detected clay minerals (green) and hydrated minerals -- clays, sulfates and others (blue).
On this map of Mars, spectrometers on spacecraft orbiting Mars have detected clay minerals (green) and hydrated minerals -- clays, sulfates and others (blue).

Regions of Mars with Clays and Hydrated Minerals Identified from Orbit

This daytime infrared image of Kaiser Crater, taken by NASA's 2001 Mars Odyssey spacecraft, shows the majority of the dune field located on the floor of the crater.
This daytime infrared image of Kaiser Crater, taken by NASA's 2001 Mars Odyssey spacecraft, shows the majority of the dune field located on the floor of the crater.

Kaiser Crater Dunes (VIS)

This image taken by NASA's Mars Odyssey spacecraft shows a portion of Maunder Crater with a number of interesting features including a series of barchan dunes that are traveling from right to left and gullies.
This image taken by NASA's Mars Odyssey spacecraft shows a portion of Maunder Crater with a number of interesting features including a series of barchan dunes that are traveling from right to left and gullies.

Maunder Crater

Syrtis Major and Arabia Terra, Mars

'Yogi' is a meter-size rock about 5 meters northwest of NASA's Mars Pathfinder lander and was the second rock visited by the Sojourner Rover's alpha proton X-ray spectrometer (APXS) instrument. 3D glasses are necessary to identify surface detail.
'Yogi' is a meter-size rock about 5 meters northwest of NASA's Mars Pathfinder lander and was the second rock visited by the Sojourner Rover's alpha proton X-ray spectrometer (APXS) instrument. 3D glasses are necessary to identify surface detail.

Yogi in Super Resolution from Super Panorama

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