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Daedalia Planum is comprised of enormous amounts of lava flows, the majority of which appear to be related to Arsia Mons. In this image from NASA's 2001 Mars Odyssey spacecraft, multiple overlapping flows are evident.
Daedalia Planum is comprised of enormous amounts of lava flows, the majority of which appear to be related to Arsia Mons. In this image from NASA's 2001 Mars Odyssey spacecraft, multiple overlapping flows are evident.

Daedalia Planum

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

Channels

This full-circle panorama of the landscape surrounding NASA's Curiosity Mars rover on July 31, 2014, offers a view into sandy lower terrain called 'Hidden Valley'
This full-circle panorama of the landscape surrounding NASA's Curiosity Mars rover on July 31, 2014, offers a view into sandy lower terrain called 'Hidden Valley'

Curiosity's 360-Degree View Before Entering 'Hidden Valley'

NASA's Mars Exploration Rover Spirit recorded this fisheye view after completing a drive during on Mars on Feb. 8, 2010. The drive left Spirit in the position where the rover will stay parked during the upcoming Mars southern-hemisphere winter.
NASA's Mars Exploration Rover Spirit recorded this fisheye view after completing a drive during on Mars on Feb. 8, 2010. The drive left Spirit in the position where the rover will stay parked during the upcoming Mars southern-hemisphere winter.

Spirit's Rear View After Parking for Fourth Winter

This image from NASA's Mars Odyssey spacecraft shows the western rim of Gale Crater. Several channels dissect the rim of the crater.
This image from NASA's Mars Odyssey spacecraft shows the western rim of Gale Crater. Several channels dissect the rim of the crater.

Images of Gale #22

These images, made from data obtained by Curiosity's CheMin, show the patterns obtained from a drift of windblown dust and sand called 'Rocknest' and from a powdered rock sample drilled from the 'John Klein' bedrock.
These images, made from data obtained by Curiosity's CheMin, show the patterns obtained from a drift of windblown dust and sand called 'Rocknest' and from a powdered rock sample drilled from the 'John Klein' bedrock.

Minerals at 'Rocknest' and 'John Klein'

This cut-out from a color panorama image taken by NASA's Curiosity rover shows the effects of the descent stage's rocket engines blasting the ground. It comes from the right side of the thumbnail panorama obtained the Mast Camera.
This cut-out from a color panorama image taken by NASA's Curiosity rover shows the effects of the descent stage's rocket engines blasting the ground. It comes from the right side of the thumbnail panorama obtained the Mast Camera.

A Set of Blast Marks in Color, Right Side

This image from NASA's Mars Reconnaissance Orbiter shows an area of layered deposits in Candor Chasma. Sheets and dunes of dark-toned sand cover the light-toned, layered bedrock.
This image from NASA's Mars Reconnaissance Orbiter shows an area of layered deposits in Candor Chasma. Sheets and dunes of dark-toned sand cover the light-toned, layered bedrock.

Layered Bedrock in Candor Chasma

In this image from NASA's Mars Odyssey the majority of the surface appears uniform with a few small hills, the region of fractured blocks sticks out as 'something different,' perhaps remnants of crater ejecta, or an area of a different type of rock.
In this image from NASA's Mars Odyssey the majority of the surface appears uniform with a few small hills, the region of fractured blocks sticks out as 'something different,' perhaps remnants of crater ejecta, or an area of a different type of rock.

Something Different

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Bahram Vallis.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Bahram Vallis.

Bahram Vallis

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 the northern tip of Baetis Mensa.
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 the northern tip of Baetis Mensa.

Baetis Mensa - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the margin between the higher elevations of Xanthe Terra and the lower elevations of Hydraotes Chaos.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the margin between the higher elevations of Xanthe Terra and the lower elevations of Hydraotes Chaos.

Xanthe 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Ophir Chasma.
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 Ophir Chasma.

Ophir Chasma - 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Candor Chasma.
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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Candor Chasma.

Candor Chasma - False Color

This image from NASA's 2001 Mars Odyssey spacecraft shows Asimov Crater is unique in that the crater floor has been completely filled with material to approximately the crater rim and then a series depressions have occurred near the crater rim.
This image from NASA's 2001 Mars Odyssey spacecraft shows Asimov Crater is unique in that the crater floor has been completely filled with material to approximately the crater rim and then a series depressions have occurred near the crater rim.

Asimov Crater

The dark, narrow band of sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft is called Hyperboreae Undae.
The dark, narrow band of sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft is called Hyperboreae Undae.

Hyperboreae Undae

Dunes cover all but the highest hill of this image captured by NASA's 2001 Mars Odyssey spacecraft. These dunes are part of Olympia Undae, a huge dune field located near the north pole.
Dunes cover all but the highest hill of this image captured by NASA's 2001 Mars Odyssey spacecraft. These dunes are part of Olympia Undae, a huge dune field located near the north pole.

Olympia Undae

Many small channels dissect the rim of Martz Crater, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Many small channels dissect the rim of Martz Crater, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Martz Crater

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.

Dust Devil Tracks

This close-up view shows Curiosity's heat shield, which helped the rover survive the harrowing journey through the Martian atmosphere, on the surface of Mars. NASA's Mars Reconnaissance Orbiter about 24 hours after landing.
This close-up view shows Curiosity's heat shield, which helped the rover survive the harrowing journey through the Martian atmosphere, on the surface of Mars. NASA's Mars Reconnaissance Orbiter about 24 hours after landing.

Final Resting Spot for Curiosity's Heat Shield

Only part of the rim of an unnamed crater remains visible above the lava flows in this region of Tharsis. This image is from NASA's 2001 Mars Odyssey spacecraft.
Only part of the rim of an unnamed crater remains visible above the lava flows in this region of Tharsis. This image is from NASA's 2001 Mars Odyssey spacecraft.

Just the Rim

NASA's Curiosity Mars rover recorded this stereo view of various rock types at waypoint called 'the Kimberley' shortly after arriving at the location on April 2, 2014. You need 3-D glasses to view this image.
NASA's Curiosity Mars rover recorded this stereo view of various rock types at waypoint called 'the Kimberley' shortly after arriving at the location on April 2, 2014. You need 3-D glasses to view this image.

Curiosity's View From Arrival Point at 'The Kimberley' Waypoint (Stereo)

Today's VIS image shows more of the channel network that comprises Arda Valles.
Today's VIS image shows more of the channel network that comprises Arda Valles.

Arda Valles

Large-scale crossbedding in the sandstone of this ridge on a lower slope of Mars' Mount Sharp is typical of windblown sand dunes that have petrified. NASA's Curiosity Mars rover used its Mastcam to capture this vista on Aug. 27, 2015.
Large-scale crossbedding in the sandstone of this ridge on a lower slope of Mars' Mount Sharp is typical of windblown sand dunes that have petrified. NASA's Curiosity Mars rover used its Mastcam to capture this vista on Aug. 27, 2015.

Vista from Curiosity Shows Crossbedded Martian Sandstone

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that make up Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a small portion of the lava flows that make up Daedalia Planum.

Daedalia Planum

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