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NASA's Curiosity Mars rover used the Dust Removal Tool on its robotic arm to brush aside reddish, more-oxidized dust, revealing a gray patch of less-oxidized rock material at a target called 'Bonanza King,' visible from the rover's Mastcam.
NASA's Curiosity Mars rover used the Dust Removal Tool on its robotic arm to brush aside reddish, more-oxidized dust, revealing a gray patch of less-oxidized rock material at a target called 'Bonanza King,' visible from the rover's Mastcam.

Curiosity's Brushwork on Martian 'Bonanza King' Target

This image shows the location of the 150-micrometer sieve screen on NASA's Mars rover Curiosity, a device used to remove larger particles from samples before delivery to science instruments.
This image shows the location of the 150-micrometer sieve screen on NASA's Mars rover Curiosity, a device used to remove larger particles from samples before delivery to science instruments.

Sifting Martian Samples

This region of arcuate (or curved) fractures is located north of Apollinaris Mons as seen by NASA's 2001 Mars Odyssey spacecraft.
This region of arcuate (or curved) fractures is located north of Apollinaris Mons as seen by NASA's 2001 Mars Odyssey spacecraft.

Arcuate Fractures

This image taken by the MAHLI camera shows a sample of basaltic rock from a lava flow in New Mexico serves as a calibration target carried on the front of NASA's Mars rover Curiosity for the rover's Canadian-made APXS instrument.
This image taken by the MAHLI camera shows a sample of basaltic rock from a lava flow in New Mexico serves as a calibration target carried on the front of NASA's Mars rover Curiosity for the rover's Canadian-made APXS instrument.

A Piece of New Mexico on Mars

This image from NASA's Mars Exploration Rover at the edge of
This image from NASA's Mars Exploration Rover at the edge of

Textures of 'Santa Maria' Crater, Sol 2476

Lycus Sulci is an extremely complex region surrounding the western and northern flanks of Olympus Mons. With a multitude of fault formed cliff faces, dark slope streaks are a common occurrence. This image was captured by NASA's Mars Odyssey.
Lycus Sulci is an extremely complex region surrounding the western and northern flanks of Olympus Mons. With a multitude of fault formed cliff faces, dark slope streaks are a common occurrence. This image was captured by NASA's Mars Odyssey.

Lycus Sulci

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the southern wall of Juventae Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the southern wall of Juventae Chasma.

Juventae Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft is located in Aeolis Mensae, east of Gale Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft is located in Aeolis Mensae, east of Gale Crater.

Yardangs

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 a hill in Tyrrhena Terra.
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 a hill in Tyrrhena Terra.

Tyrrhena Terra - False Color

This image from NASA's Mars Reconnaissance Orbiter spacecraft shows a water-carved channel. The channel pattern, called dendritic because of its tree, like branching running down over the rim of an ancient impact basin across the basin floor.
This image from NASA's Mars Reconnaissance Orbiter spacecraft shows a water-carved channel. The channel pattern, called dendritic because of its tree, like branching running down over the rim of an ancient impact basin across the basin floor.

Ancient Rivers

Located southwest of Olympus Mons, this image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a complex region that has undergone several geologic processes.
Located southwest of Olympus Mons, this image captured by NASA's 2001 Mars Odyssey spacecraft shows part of a complex region that has undergone several geologic processes.

Ridges and Flows

The THEMIS VIS 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 the mesa that Escorial Crater is located on.
The THEMIS VIS 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 the mesa that Escorial Crater is located on.

Escorial Crater- False Color

The THEMIS VIS 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 small dunes on the floor of Bamberg Crater.
The THEMIS VIS 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 small dunes on the floor of Bamberg Crater.

Bamberg Crater Dunes - False Color

Kasei Valles is a valley system was likely carved by some combination of flowing water and lava. In some areas, erosion formed cliffs along the flow path resulting in water or lava falls as seen by NASA's Mars Reconnaissance Orbiter spacecraft.
Kasei Valles is a valley system was likely carved by some combination of flowing water and lava. In some areas, erosion formed cliffs along the flow path resulting in water or lava falls as seen by NASA's Mars Reconnaissance Orbiter spacecraft.

Kasei Valles

In the best-selling novel 'The Martian' and the movie based on it, stranded astronaut Mark Watney's adventures take him to the rim of Mawrth Crater. This image from NASA's Mars Reconnaissance Orbiter shows the nature of this terrain.
In the best-selling novel 'The Martian' and the movie based on it, stranded astronaut Mark Watney's adventures take him to the rim of Mawrth Crater. This image from NASA's Mars Reconnaissance Orbiter shows the nature of this terrain.

Western Edge of Mars' Marth Crater, a Movie Location

The THEMIS VIS 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 where Mawrth Vallis empties into Chryse Planitia.
The THEMIS VIS 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 where Mawrth Vallis empties into Chryse Planitia.

Mawrth Vallis - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the complex channel called Mengala Valles.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the complex channel called Mengala Valles.

Mangala Valles

The THEMIS VIS 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 Coprates Chasma.
The THEMIS VIS 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 Coprates Chasma.

Coprates Chasma - False Color

This VIS image captured by NASA's 2001 Mars Odyssey spacecraft was collected at the same time as yesterday's IR image. The dunes are darker in visible wavelengths than the surrounding material.
This VIS image captured by NASA's 2001 Mars Odyssey spacecraft was collected at the same time as yesterday's IR image. The dunes are darker in visible wavelengths than the surrounding material.

Noachis Terra Dunes - VIS

The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows windstreaks in Daedalia Planum.
The THEMIS VIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows windstreaks in Daedalia Planum.

Windstreaks - False Color

This image from NASA's 2001 Mars Odyssey spacecraft shows dark slope streaks on the inner rim of an unnamed crater in Amazonis Planitia.
This image from NASA's 2001 Mars Odyssey spacecraft shows dark slope streaks on the inner rim of an unnamed crater in Amazonis Planitia.

Dark Slope Streaks

The lava flows and depressions in this image from NASA's 2001 Mars Odyssey spacecraft are located south of Alba Mons.
The lava flows and depressions in this image from NASA's 2001 Mars Odyssey spacecraft are located south of Alba Mons.

Tharsis Volcanics

Numerous unnamed channels seen in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the eastern margin of Tempe Terra.
Numerous unnamed channels seen in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the eastern margin of Tempe Terra.

Tempe Terra

The small channel and lava flows in this image NASA's 2001 Mars Odyssey spacecraft are located northeast of Olympus Mons.
The small channel and lava flows in this image NASA's 2001 Mars Odyssey spacecraft are located northeast of Olympus Mons.

Channel

This image captured by NASA's 2001 Mars Odyssey spacecraft shows windstreaks on the volcanic surface between Alba Mons and Acheron Fossae.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows windstreaks on the volcanic surface between Alba Mons and Acheron Fossae.

Wind Streaks

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