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The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows a unique, resistant material on the floor of an unnamed crater.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows a unique, resistant material on the floor of an unnamed crater.

Terra Cimmeria Crater - False Color

The THEMIS VIS camera contains 5 filters. 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 the floor and rim of an unnamed crater in Terra Cimmeria.
The THEMIS VIS camera contains 5 filters. 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 the floor and rim of an unnamed crater in Terra Cimmeria.

Crater - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes on the floor of an unnamed crater in Noachis Terra.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes on the floor of an unnamed crater in Noachis Terra.

Crater Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows numerous gullies are visible on the cliff face of a depression within the floor of Lyell Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows numerous gullies are visible on the cliff face of a depression within the floor of Lyell Crater.

Lyell Crater

This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Arabia Terra.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Arabia Terra.

Dunes

The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.
The north end of this long image from NASA's Mars Reconnaissance Orbiter shows a lava surface in southern Elysium Planitia. Small cones are common on the extensive young flood lavas in this region.

Strange Cones and Flows

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Alba Fossae, located on the northwestern margin of Alba Mons. Small channels are also visible.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Alba Fossae, located on the northwestern margin of Alba Mons. Small channels are also visible.

Alba Fossae

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Nanedi Valles.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Nanedi Valles.

Nanedi Valles

Since landing on Mars in August 2012, NASA's Curiosity Mars rover has fired the laser on its Chemistry and Camera (ChemCam) instrument more than 100,000 times at rock and soil targets up to about 23 feet (7 meters) away.
Since landing on Mars in August 2012, NASA's Curiosity Mars rover has fired the laser on its Chemistry and Camera (ChemCam) instrument more than 100,000 times at rock and soil targets up to about 23 feet (7 meters) away.

Target for 100,000th Laser Shot by Curiosity on Mars

This image of terrain inside Mars' Gale Crater and the calibration target for Mastcam on NASA's Mars rover Curiosity illustrate how false color can be used to make differences more evident in the materials in the scene.
This image of terrain inside Mars' Gale Crater and the calibration target for Mastcam on NASA's Mars rover Curiosity illustrate how false color can be used to make differences more evident in the materials in the scene.

Using False Color from Curiosity's Mast Camera

The eastern margin of a rippled dune in Herschel Crater on Mars moved an average distance of three meters (about three yards) between March 3, 2007 and December 1, 2010, in one of two images taken by NASA's Mars Reconnaissance Orbiter.
The eastern margin of a rippled dune in Herschel Crater on Mars moved an average distance of three meters (about three yards) between March 3, 2007 and December 1, 2010, in one of two images taken by NASA's Mars Reconnaissance Orbiter.

Shifting Sand in Herschel Crater

The area in and near the landing site selected for landing of NASA's Mars Science Laboratory offers a diversity of possible targets for examination by the mission's rover, Curiosity.
The area in and near the landing site selected for landing of NASA's Mars Science Laboratory offers a diversity of possible targets for examination by the mission's rover, Curiosity.

Attractions for Study in and near Curiosity's Selected Landing Site

The dunes in this image from NASA's Mars Odyssey are located on the floor of an unnamed crater in Terra Cimmeria.
The dunes in this image from NASA's Mars Odyssey are located on the floor of an unnamed crater in Terra Cimmeria.

Terra Cimmeria Dunes

Alluvial fans are piles of debris dumped by rivers when they emerge from the mountains and enter a mostly dry valley as seen by NASA's Mars Reconnaissance Orbiter.
Alluvial fans are piles of debris dumped by rivers when they emerge from the mountains and enter a mostly dry valley as seen by NASA's Mars Reconnaissance Orbiter.

Sinuous Ridge on the Orson Welles Bajada

This infrared image captured by NASA's 2001 Mars Odyssey spacecraft shows bright toned material, which is warmer than dark toned surfaces. Material has moved downslope from the top of this hill in Promethei Terra.
This infrared image captured by NASA's 2001 Mars Odyssey spacecraft shows bright toned material, which is warmer than dark toned surfaces. Material has moved downslope from the top of this hill in Promethei Terra.

Debris Flow

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 some of the plains of Arabia Terra.
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 some of the plains of Arabia Terra.

Arabia Terra - False Color

This was the first image to be acquired by NASA's Mars Reconnaissance Orbiter after the sun rose on Inca City, marking the end to polar night. A few fans are visible emerging from the araneiforms.
This was the first image to be acquired by NASA's Mars Reconnaissance Orbiter after the sun rose on Inca City, marking the end to polar night. A few fans are visible emerging from the araneiforms.

Spring in Inca City I

In the northern section of this from image NASA's Mars Reconnaissance Orbiter, we see flat terrain that is probably an ancient lava field. These dust avalanches are common in dust-covered regions on Mars.
In the northern section of this from image NASA's Mars Reconnaissance Orbiter, we see flat terrain that is probably an ancient lava field. These dust avalanches are common in dust-covered regions on Mars.

A Collection of Landforms in Eastern Elysium Planitia

The hills in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Avernus Colles.
The hills in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Avernus Colles.

Avernus Colles

The term 'colles' means hills. The hills in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern plains near Phlegra Dorsa.
The term 'colles' means hills. The hills in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern plains near Phlegra Dorsa.

Colles

This image from NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae, but unlike yesterday's image, there is more topography in this region.
This image from NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae, but unlike yesterday's image, there is more topography in this region.

North Polar Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes on the margin of Olympia Undae, a large dune field near the north pole.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows dunes on the margin of Olympia Undae, a large dune field near the north pole.

North Polar Dunes

Shadows cast by the high walls and high hills within Candor Chasma are visible in this image from NASA's 2001 Mars Odyssey spacecraft. The local time is near 5:00 in the afternoon.
Shadows cast by the high walls and high hills within Candor Chasma are visible in this image from NASA's 2001 Mars Odyssey spacecraft. The local time is near 5:00 in the afternoon.

Shadows

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the region slightly south of yesterday's image, including the floor of the crater at the bottom of the frame.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the region slightly south of yesterday's image, including the floor of the crater at the bottom of the frame.

Images of Gale #13

This graph presents information from the NASA Curiosity Mars rover's onboard analysis of rock powder drilled from the 'Buckskin' and 'Greenhorn' target locations on lower Mount Sharp.
This graph presents information from the NASA Curiosity Mars rover's onboard analysis of rock powder drilled from the 'Buckskin' and 'Greenhorn' target locations on lower Mount Sharp.

Silica in Opal at 'Buckskin' and 'Greenhorn' on Mount Sharp

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