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Layering of Arabia Terra is evident in this image from NASA's 2001 Mars Odyssey spacecraft.
Layering of Arabia Terra is evident in this image from NASA's 2001 Mars Odyssey spacecraft.

Layers

This image from NASA's Mars Odyssey shows part of the summit of Ceraunius Tholus.
This image from NASA's Mars Odyssey shows part of the summit of Ceraunius Tholus.

Ceraunius Tholus

This frame from an animation from NASA's Mars rover Curiosity shows the rover drilling into rock target 'Cumberland.' The drilling was performed during the 279th Martian day, or sol, of the Curiosity's work on Mars (May 19, 2013).
This frame from an animation from NASA's Mars rover Curiosity shows the rover drilling into rock target 'Cumberland.' The drilling was performed during the 279th Martian day, or sol, of the Curiosity's work on Mars (May 19, 2013).

Curiosity Mars Rover Drilling Into Its Second Rock

This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes in located on the floor of Lyot Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes in located on the floor of Lyot Crater.

Lyot Crater Dunes

This image, taken by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is of a gully on a south-facing slope in middle southern latitudes of Mars.
This image, taken by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is of a gully on a south-facing slope in middle southern latitudes of Mars.

Changes in a Gully in a Mars Crater (Two-Image Comparison)

This windstreak is located on the volcanic plains of Daedalia Planum as seen by NASA's Mars Odyssey. The dark outer margin is the region of dust being removed from the surface. The inner bright part is where dust is being deposited.
This windstreak is located on the volcanic plains of Daedalia Planum as seen by NASA's Mars Odyssey. The dark outer margin is the region of dust being removed from the surface. The inner bright part is where dust is being deposited.

Windstreak on Daedalia Planum

These dunes in Richardson Crater are still frost covered in this image captured by NASA's Mars Odyssey. As spring deepens the frost will sublimate and the dark dunes will appear.
These dunes in Richardson Crater are still frost covered in this image captured by NASA's Mars Odyssey. As spring deepens the frost will sublimate and the dark dunes will appear.

Richardson Crater Dunes

NASA's Curiosity Mars rover targeted the laser of the ChemCam instrument with remarkable accuracy for assessing the composition of the wall of a drilled hole and tailings that resulted from the drilling.
NASA's Curiosity Mars rover targeted the laser of the ChemCam instrument with remarkable accuracy for assessing the composition of the wall of a drilled hole and tailings that resulted from the drilling.

Accurate Pointing by Curiosity

This map of Mars from NASA's Mars Odyssey orbiter shows relative locations of three types of findings related to salt or frozen water, plus a new type of finding that may be related to both salt and water.
This map of Mars from NASA's Mars Odyssey orbiter shows relative locations of three types of findings related to salt or frozen water, plus a new type of finding that may be related to both salt and water.

Ice, Salt and Warm-Season Flows on Mars

This image captured by NASA's 2001 Mars Odyssey shows a landslide deposit located in an unnamed crater in Syrtis Planum.
This image captured by NASA's 2001 Mars Odyssey shows a landslide deposit located in an unnamed crater in Syrtis Planum.

Syrtis Planum Landslide

This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows from Alba Mons. The depression and collapse features within it are part of the large system of tectonic features created by the apparent collapse of the volcano.
This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows from Alba Mons. The depression and collapse features within it are part of the large system of tectonic features created by the apparent collapse of the volcano.

Alba Mons Flows

A volcanic vent has created a small construct (a volcano) in this region of Tharsis east of Arsia Mons. This image is from NASA's 2001 Mars Odyssey spacecraft.
A volcanic vent has created a small construct (a volcano) in this region of Tharsis east of Arsia Mons. This image is from NASA's 2001 Mars Odyssey spacecraft.

Tharsis Volcanics

The wind etched region in this image captured by NASA's Mars Odyssey on July 23, 2010 is called Zephyria Planum.
The wind etched region in this image captured by NASA's Mars Odyssey on July 23, 2010 is called Zephyria Planum.

Zephyria Planum

The THEMIS camera contains 5 filters. The 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 part of Nili Fossae.
The THEMIS camera contains 5 filters. The 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 part of Nili Fossae.

Nili Fossae - False Color

Dark slope streaks mark the rim of this unnamed crater near Schiaparelli Crater as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks mark the rim of this unnamed crater near Schiaparelli Crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

This unnamed as seen by NASA's 2001 Mars Odyssey spacecraft channel drains part of Margaritifer Terra.
This unnamed as seen by NASA's 2001 Mars Odyssey spacecraft channel drains part of Margaritifer Terra.

Channel

This image from NASA's Mars Reconnaissance Orbiter shows a number of unusual, quasi-circular structures that apparently formed within bright flows in Meridiani Planum.
This image from NASA's Mars Reconnaissance Orbiter shows a number of unusual, quasi-circular structures that apparently formed within bright flows in Meridiani Planum.

Concentric Structures in Meridiani Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a number of unnamed channels located on the northeastern margin of Terra Sabaea.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a number of unnamed channels located on the northeastern margin of Terra Sabaea.

Channels

Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? The head of an eagle, with it's sharp beak, looks towards the bottom of the image.
Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? The head of an eagle, with it's sharp beak, looks towards the bottom of the image.

THEMIS Art #106

The channel in this image from NASA's 2001 Mars Odyssey spacecraft is located in northern Terra Sabaea and runs semi-parallel to Auqakuh Vallis.
The channel in this image from NASA's 2001 Mars Odyssey spacecraft is located in northern Terra Sabaea and runs semi-parallel to Auqakuh Vallis.

Channel

NASA's 2001 Mars Odyssey captured this image of a channel entering Eberswalde Crater and depositing a fan-shaped delta on the crater floor.
NASA's 2001 Mars Odyssey captured this image of a channel entering Eberswalde Crater and depositing a fan-shaped delta on the crater floor.

Eberswalde Crater Delta

The THEMIS camera contains 5 filters. The 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 part of Terby Crater.
The THEMIS camera contains 5 filters. The 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 part of Terby Crater.

Terby Crater - False Color

This view from the Mars Hand Lens Imager (MAHLI) on the arm of NASA's Curiosity Mars rover shows texture within a light-toned vein at a site called 'Garden City' on lower Mount Sharp.
This view from the Mars Hand Lens Imager (MAHLI) on the arm of NASA's Curiosity Mars rover shows texture within a light-toned vein at a site called 'Garden City' on lower Mount Sharp.

Crystal Growth Texture in Light Vein at 'Garden City'

The intersecting ridges in this image captured by NASA's 2001 Mars Odyssey spacecraft are called Angustus Labyrinthus. They were formed due to tectonic activity.
The intersecting ridges in this image captured by NASA's 2001 Mars Odyssey spacecraft are called Angustus Labyrinthus. They were formed due to tectonic activity.

Angustus Laybrinthus

The volcanic flows in this image from NASA's Mars Odyssey spacecraft are part of Daedalia Planum. The flows originated at Arsia Mons.
The volcanic flows in this image from NASA's Mars Odyssey spacecraft are part of Daedalia Planum. The flows originated at Arsia Mons.

Daedalia Planum

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