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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 part of the floor of Trouvelot 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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Trouvelot Crater.

Trouvelot Crater - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the large dune field on the floor of Proctor Crater.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the large dune field on the floor of Proctor Crater.

Proctor Crater Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows multiple dune fields cover the floor of Hooke Crater, located on the northern margin of Argyre Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows multiple dune fields cover the floor of Hooke Crater, located on the northern margin of Argyre Planitia.

Hooke Crater Dunes

The linear graben in this image from NASA's 2001 Mars Odyssey spacecraft are part of Claritas Fossae.
The linear graben in this image from NASA's 2001 Mars Odyssey spacecraft are part of Claritas Fossae.

Claritas Fossae

One of the great strengths of the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is that its high resolution can help resolve interesting questions. Here, is the platy flow material younger than the yardang-forming material?
One of the great strengths of the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is that its high resolution can help resolve interesting questions. Here, is the platy flow material younger than the yardang-forming material?

Which Came First, the Yardang or the Platy Flow?

This image from NASA's Mars Odyssey spacecraft shows the highest elevation of layered deposit occurs at the top, but just south of the center of the image is a peak that does not appear to be layered and is eroding differently than the rest of Mt. Sharp.
This image from NASA's Mars Odyssey spacecraft shows the highest elevation of layered deposit occurs at the top, but just south of the center of the image is a peak that does not appear to be layered and is eroding differently than the rest of Mt. Sharp.

Images of Gale #14

The lava flows in this image are part of Daedalia Planum as seen by NASA's 2001 Mars Odyssey spacecraft.
The lava flows in this image are part of Daedalia Planum as seen by NASA's 2001 Mars Odyssey spacecraft.

Daedalia Planum

This image from NASA's 2001 Mars Odyssey spacecraft of Daedalia Planum shows the termination or end of a single flow. In this case it is the end of the brighter/rougher flow on the right side of the image.
This image from NASA's 2001 Mars Odyssey spacecraft of Daedalia Planum shows the termination or end of a single flow. In this case it is the end of the brighter/rougher flow on the right side of the image.

Daedalia Planum

This image from NASA's 2001 Mars Odyssey spacecraft shows the complex collapse features on the southern flank of Ascraeus Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows the complex collapse features on the southern flank of Ascraeus Mons.

Ascraeus Mon

This image from NASA's Mars Odyssey shows dunes on the floor of an unnamed crater west of Herschel Crater.
This image from NASA's Mars Odyssey shows dunes on the floor of an unnamed crater west of Herschel Crater.

Sand Dunes

The wind is responsible for the erosion seen in this image captured by NASA's 2001 Mars Odyssey spacecraft near Aeolis Planum.
The wind is responsible for the erosion seen in this image captured by NASA's 2001 Mars Odyssey spacecraft near Aeolis Planum.

Erosion

Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? Another bug!
Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? Another bug!

THEMIS Art #107

NASA's Mars Exploration Rover Spirit used its microscopic imager to capture this spectacular, jagged mini-landscape on a rock called 'GongGong.'
NASA's Mars Exploration Rover Spirit used its microscopic imager to capture this spectacular, jagged mini-landscape on a rock called 'GongGong.'

Hardened Lava Meets Wind on Mars

Tiu Valles is the location of the streamlined island in this image from NASA's 2001 Mars Odyssey spacecraft.
Tiu Valles is the location of the streamlined island in this image from NASA's 2001 Mars Odyssey spacecraft.

Tiu Valles

This region of Tharsis near Olympus Mons contains subtle features showing its lava flow origin. Note the 'softened' flow fronts and lava channels in this image captured by NASA's Mars Odyssey spacecraft.
This region of Tharsis near Olympus Mons contains subtle features showing its lava flow origin. Note the 'softened' flow fronts and lava channels in this image captured by NASA's Mars Odyssey spacecraft.

Tharsis Lava

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 captured by 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Nili Fossae.

Nili Fossae - 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 mesas and channels on the margin of Terra Sabaea.
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 mesas and channels on the margin of Terra Sabaea.

Terra Sabaea - False Color

This view of a test rover at NASA's Jet Propulsion Laboratory, Pasadena, California, results from advance testing of arm positions and camera pointings for taking a low-angle self-portrait of NASA's Curiosity Mars rover.
This view of a test rover at NASA's Jet Propulsion Laboratory, Pasadena, California, results from advance testing of arm positions and camera pointings for taking a low-angle self-portrait of NASA's Curiosity Mars rover.

Test Rover at JPL During Preparation for Mars Rover's Low-Angle Selfie

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 several linear depressions.
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 several linear depressions.

Sirenum Fossae - 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 depressions in the surface of southern Noachis 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 image from NASA's 2001 Mars Odyssey spacecraft shows depressions in the surface of southern Noachis Terra.

Sisyphi Cavi - 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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Sulci Gordii east of Olympus Mons.
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 part of Sulci Gordii east of Olympus Mons.

Sulci Gordii - False Color

The intersecting ridges in this image from NASA's 2001 Mars Odyssey spacecraft are part of Angustus Labyrinthus, informally called Inca City.
The intersecting ridges in this image from NASA's 2001 Mars Odyssey spacecraft are part of Angustus Labyrinthus, informally called Inca City.

Angustus Laybrinthus

The unnamed channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Terra Cimmeria.
The unnamed channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Terra Cimmeria.

Terra Cimmeria

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Ma'adim Vallis, which is a large channel that enters Gusev Crater from the south.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Ma'adim Vallis, which is a large channel that enters Gusev Crater from the south.

Ma'adim Vallis

This infrared image from NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Rabe Crater. The dunes are 'brighter' than the surrounding material, indicating that they are warmer.
This infrared image from NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Rabe Crater. The dunes are 'brighter' than the surrounding material, indicating that they are warmer.

Rabe Crater Dunes

Currently displaying images 2351-2375 of 3715
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