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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 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

Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.
Lava flows south of Arsia Mons in Daedalia Planum transition from younger flows with elongated, sinuous morphologies to the northeast, to older, broader lobes and sheet flows to the southwest. This image is from NASA's Mars Reconnaissance Orbiter.

Overlapping Lobate Lava Flows in Daedalia Planum

NASA's Mars Exploration Rover capturde this 360-degree view near the ridgeline of Endeavour Crater's western rim. The center is southeastward. Rocks on the slope to the right of center are in an outcrop area targeted for the rover to study.
NASA's Mars Exploration Rover capturde this 360-degree view near the ridgeline of Endeavour Crater's western rim. The center is southeastward. Rocks on the slope to the right of center are in an outcrop area targeted for the rover to study.

Approaching a Target Deposit on Mars Crater Rim

The flows in this image captured by NASA's 2001 Mars Odyssey spacecraft originated at Alba Mons.
The flows in this image captured by NASA's 2001 Mars Odyssey spacecraft originated at Alba Mons.

Alba Mons Flows

This image captured by NASA's 2001 Mars Odyssey spacecraft of Gale Crater shows the region of the crater that is 'home' to the Curiosity Rover.
This image captured by NASA's 2001 Mars Odyssey spacecraft of Gale Crater shows the region of the crater that is 'home' to the Curiosity Rover.

Gale Crater

Nirgal Vallis is one of the largest and longest valley networks on Mars as seen by NASA's Mars Reconnaissance Orbiter.
Nirgal Vallis is one of the largest and longest valley networks on Mars as seen by NASA's Mars Reconnaissance Orbiter.

Nirgal Vallis Tributaries

This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows in Daedalia Planum.
This image from NASA's 2001 Mars Odyssey spacecraft shows lava flows in Daedalia Planum.

Daedalia Planum

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive field of lava flows that make up Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive field of lava flows that make up Daedalia Planum.

Daedalia Planum

This image from NASA's Mars Odyssey spacecraft shows the eastern part of Hydrae Chasma.
This image from NASA's Mars Odyssey spacecraft shows the eastern part of Hydrae Chasma.

Hydrae Chasma

The parallel ridges in this image captured by NASA's Mars Odyssey spacecraft are part of Arsia Sulci - a region west of Arsia Mons. How these features were formed is unknown.
The parallel ridges in this image captured by NASA's Mars Odyssey spacecraft are part of Arsia Sulci - a region west of Arsia Mons. How these features were formed is unknown.

Arsia Sulci

This graph compares a typical daily pattern of changing atmospheric pressure (blue) with the pattern during a regional dust storm hundreds of miles away (red). The data are by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.
This graph compares a typical daily pattern of changing atmospheric pressure (blue) with the pattern during a regional dust storm hundreds of miles away (red). The data are by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.

Atmospheric Pressure Patterns Before and During Dust Storm

Impact craters can have a variety of floor features. This image from NASA's Mars Odyssey is a central peak/pit combination crater in Terra Cimmeria.
Impact craters can have a variety of floor features. This image from NASA's Mars Odyssey is a central peak/pit combination crater in Terra Cimmeria.

Crater Centers

This image from NASA's Mars Odyssey caputured on July 23, 2010 off the northern flank of Arsia Mons shows collapse/vent features.
This image from NASA's Mars Odyssey caputured on July 23, 2010 off the northern flank of Arsia Mons shows collapse/vent features.

Arsia Mons

Cumulative driving by NASA's Mars Exploration Rover Opportunity surpassed marathon distance on March 24, 2015, as the rover neared a destination called 'Marathon Valley,' which is middle ground of this stereo view from early March.
Cumulative driving by NASA's Mars Exploration Rover Opportunity surpassed marathon distance on March 24, 2015, as the rover neared a destination called 'Marathon Valley,' which is middle ground of this stereo view from early March.

Opportunity's Approach to 'Marathon Valley' (Stereo)

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 Candor Labes.
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 Candor Labes.

Candor Labes - 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 the floor of Antoniadi 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 Antoniadi Crater.

Antoniadi Crater - False Color

This false color image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the summit caldera of Arsia Mons. The mottled bluish tones are from clouds.
This false color image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the summit caldera of Arsia Mons. The mottled bluish tones are from clouds.

Arsia Mons False Color

This image from NASA's Mars Odyssey spacecraft is just slightly south of yesterday's, and shows how close the dunes are to the crater rim.
This image from NASA's Mars Odyssey spacecraft is just slightly south of yesterday's, and shows how close the dunes are to the crater rim.

Images of Gale #29

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Aram Chaos. There are several layers of material in this region.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Aram Chaos. There are several layers of material in this region.

Aram Chaos

This mosaic shows the calibration target for the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity rover, as seen by the ChemCam's remote micro-imager. The 10 images incorporated in this mosaic were taken on Aug. 15.
This mosaic shows the calibration target for the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity rover, as seen by the ChemCam's remote micro-imager. The 10 images incorporated in this mosaic were taken on Aug. 15.

Checking out ChemCam's View

This image shows the calibration target for the Chemistry and Camera instrument on NASA's Curiosity rover before it was installed on the rover and readied for launch.
This image shows the calibration target for the Chemistry and Camera instrument on NASA's Curiosity rover before it was installed on the rover and readied for launch.

Pre-Launch Calibration Target for ChemCam

These windstreaks are located in northern Terra Tyrrhena. The wind was blowing from NE to SW to create the streaks in the lee of the craters. This image is from NASA's Mars Odyssey.
These windstreaks are located in northern Terra Tyrrhena. The wind was blowing from NE to SW to create the streaks in the lee of the craters. This image is from NASA's Mars Odyssey.

Windstreaks

The ejecta materials of this crater are more resistant to erosion than the surrounding materials. The wind has eroded pits and other features around the crater causing it to become a topographic high. This image is from NASA's Mars Odyssey.
The ejecta materials of this crater are more resistant to erosion than the surrounding materials. The wind has eroded pits and other features around the crater causing it to become a topographic high. This image is from NASA's Mars Odyssey.

Wind and Rock

Individual sand dunes are visible in this image of Nili Patera taken by NASA's Mars Odyssey.
Individual sand dunes are visible in this image of Nili Patera taken by NASA's Mars Odyssey.

Nili Patera Dunes

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