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The depression in the center of this image captured by NASA's 2001 Mars Odyssey spacecraft is a graben (fault bounded block of material). This graben is called Mangala Fossa.
The depression in the center of this image captured by NASA's 2001 Mars Odyssey spacecraft is a graben (fault bounded block of material). This graben is called Mangala Fossa.

Mangala Fossa

This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Angustus Labyrinthus

This image NASA's Mars Reconnaissance Orbitershows a prominently stratified transect through the rock of a mountain of material in the middle of Hebes Chasma.
This image NASA's Mars Reconnaissance Orbitershows a prominently stratified transect through the rock of a mountain of material in the middle of Hebes Chasma.

A Revealing Landslide in Hebes Chasma

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

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

This image captured by NASA's 2001 Mars Odyssey spacecraft is of an unnamed channel located on the northern margin of Terra Cimmeria.
This image captured by NASA's 2001 Mars Odyssey spacecraft is of an unnamed channel located on the northern margin of Terra Cimmeria.

Channel

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

'Twin Peaks' are modest-size hills to the southwest of NASA's Mars Pathfinder landing site. They were discovered on the first panoramas taken by the IMP camera on the 4th of July, 1997. 3D glasses are necessary to identify surface detail.
'Twin Peaks' are modest-size hills to the southwest of NASA's Mars Pathfinder landing site. They were discovered on the first panoramas taken by the IMP camera on the 4th of July, 1997. 3D glasses are necessary to identify surface detail.

The Twin Peaks in 3-D, as Viewed by the Mars Pathfinder IMP Camera

Dark streaks mark the steep slopes of this ridge located east of Mangala Valles as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark streaks mark the steep slopes of this ridge located east of Mangala Valles as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

Dark surface material is starting to appear as the frost is sublimated in this image of Pityusa Patera as seen by NASA's Mars Odyssey.
Dark surface material is starting to appear as the frost is sublimated in this image of Pityusa Patera as seen by NASA's Mars Odyssey.

Pityusa Patera

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? Mickey Mouse is really getting around on Mars, here's his head again!
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? Mickey Mouse is really getting around on Mars, here's his head again!

THEMIS Art #123

These windstreaks are located on Syrtis Major Planum, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
These windstreaks are located on Syrtis Major Planum, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Windstreaks

Acheron Fossae is a dissected region of rugged terrain located north of Olympus Mons. Numerous channels are visible in this image captured by NASA's 2001 Mars Odyssey.
Acheron Fossae is a dissected region of rugged terrain located north of Olympus Mons. Numerous channels are visible in this image captured by NASA's 2001 Mars Odyssey.

Acheron Fossae

This image from NASA's 2001 Mars Odyssey spacecraft shows streamlined islands within part of Kasei Valles.
This image from NASA's 2001 Mars Odyssey spacecraft shows streamlined islands within part of Kasei Valles.

Kasei Valles

This map shows the route that NASA's Curiosity Mars rover drove inside Gale Crater from its landing in August 2013 through Jan. 26, 2004. The rover is approaching a gap between two low scarps, 'Dingo Gap.'
This map shows the route that NASA's Curiosity Mars rover drove inside Gale Crater from its landing in August 2013 through Jan. 26, 2004. The rover is approaching a gap between two low scarps, 'Dingo Gap.'

Traverse Map for Mars Rover Curiosity as of Jan. 26, 2014

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? There is a mickey mouse hat sitting on the top right side of this daytime infrared image.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? There is a mickey mouse hat sitting on the top right side of this daytime infrared image.

THEMIS Art #112

Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is both tectonically fractured rocks (top) and volcanic flows (middle and bottom). This image is from NASA's 2001 Mars Odyssey spacecraft.
Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is both tectonically fractured rocks (top) and volcanic flows (middle and bottom). This image is from NASA's 2001 Mars Odyssey spacecraft.

Echus Chasma

This image, captured by NASA's Mars Odyssey on Sept. 9, 2010, shows some of the dunes of the floor of Moreux Crater.
This image, captured by NASA's Mars Odyssey on Sept. 9, 2010, shows some of the dunes of the floor of Moreux Crater.

Moreux Crater Dunes

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

Tithonium Chasma

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