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Digging by NASA's Phoenix Mars Lander on Aug. 23, 2008, reached a depth about three times greater than in any trench Phoenix has excavated. 3D glasses are necessary.
Digging by NASA's Phoenix Mars Lander on Aug. 23, 2008, reached a depth about three times greater than in any trench Phoenix has excavated. 3D glasses are necessary.

Deep 'Stone Soup' Trenching by Phoenix (Stereo)

This anaglyph, acquired by NASA's Phoenix Lander's show Phoenix's solar panel is seen in the bottom right corner of the image. 3D glasses are necessary to view this image.
This anaglyph, acquired by NASA's Phoenix Lander's show Phoenix's solar panel is seen in the bottom right corner of the image. 3D glasses are necessary to view this image.

Martian Surface as Seen by Phoenix

This view from NASA's Phoenix Mars Lander shows a portion of the trench informally named 'Snow White,' with two holes near the top of the image. 3D glasses are necessary to view this image.
This view from NASA's Phoenix Mars Lander shows a portion of the trench informally named 'Snow White,' with two holes near the top of the image. 3D glasses are necessary to view this image.

Two Holes from Using Rasp in 'Snow White' (Stereo)

This image shows an orbital view sweeping upward from Olympus Mons, the tallest volcano in the solar system, to the location of NASA's Phoenix Mars Lander in the northern polar reaches of Mars.
This image shows an orbital view sweeping upward from Olympus Mons, the tallest volcano in the solar system, to the location of NASA's Phoenix Mars Lander in the northern polar reaches of Mars.

Phoenix's Position on Mars

NASA's Mars Exploration Rover Opportunity captured a sweeping stereo image of 'Burns Cliff' after driving right to the base of this southeastern portion of the inner wall of 'Endurance Crater' in November 2004. 3D glasses are necessary to view this image.
NASA's Mars Exploration Rover Opportunity captured a sweeping stereo image of 'Burns Cliff' after driving right to the base of this southeastern portion of the inner wall of 'Endurance Crater' in November 2004. 3D glasses are necessary to view this image.

'Burns Cliff' in Color Stereo

This 360-degree three dimensional anaglyph view from NASA's Mars Exploration Rover Spirit highlights Gusev crater on sol 148. 3D glasses are necessary to view this image.
This 360-degree three dimensional anaglyph view from NASA's Mars Exploration Rover Spirit highlights Gusev crater on sol 148. 3D glasses are necessary to view this image.

Spirit's View on Sol 148 (3-D)

This 3-D anaglyph, from NASA's Mars Exploration Rover Spirit, shows an extreme close-up of round, blueberry-shaped grains on the crater floor near the rock outcrop at Meridiani Planum called Stone Mountain. 3D glasses are necessary.
This 3-D anaglyph, from NASA's Mars Exploration Rover Spirit, shows an extreme close-up of round, blueberry-shaped grains on the crater floor near the rock outcrop at Meridiani Planum called Stone Mountain. 3D glasses are necessary.

Even More Eye-popping 'Berries'

This 3-D anaglyph, from NASA's Mars Exploration Rover Spirit, shows a microscopic image taken of soil featuring round, blueberry-shaped rock formations on the crater floor at Meridiani Planum, Mars. 3D glasses are necessary to view this image.
This 3-D anaglyph, from NASA's Mars Exploration Rover Spirit, shows a microscopic image taken of soil featuring round, blueberry-shaped rock formations on the crater floor at Meridiani Planum, Mars. 3D glasses are necessary to view this image.

"Berries" on the Ground 2 (3-D)

This image from NASA's Mars Odyssey covers a region in western Arabia Terra, which contains two interesting craters. The eastern floor of the largest crater seen in most of this image is bumpy and ridged in places and relatively smooth in regions.
This image from NASA's Mars Odyssey covers a region in western Arabia Terra, which contains two interesting craters. The eastern floor of the largest crater seen in most of this image is bumpy and ridged in places and relatively smooth in regions.

Western Arabia Terra

The ejecta blanket of the crater in this image from NASA's Mars Odyssey spacecraft does not resemble the blocky, discontinuous ejecta associated with most fresh craters on Mars.
The ejecta blanket of the crater in this image from NASA's Mars Odyssey spacecraft does not resemble the blocky, discontinuous ejecta associated with most fresh craters on Mars.

Fluidized crater ejecta

This set of images from NASA's Mars Odyssey spacecraft shows the so-called 'face on Mars' landform located in the northern plains of Mars.
This set of images from NASA's Mars Odyssey spacecraft shows the so-called 'face on Mars' landform located in the northern plains of Mars.

The So-Called "Face on Mars" in Infrared

Hrad Valles, seen in this image from NASA's Mars Odyssey spacecraft, is located north-northwest of the large Elysium Mons volcanic complex and is yet another example of a channel that likely carried fluids.
Hrad Valles, seen in this image from NASA's Mars Odyssey spacecraft, is located north-northwest of the large Elysium Mons volcanic complex and is yet another example of a channel that likely carried fluids.

Hrad Valles

White Rock' is the unofficial name for this unusual landform which was first observed during NASA's Mariner 9 mission in the early 1970's and is now shown here in an image from NASA's Mars Odyssey spacecraft.
White Rock' is the unofficial name for this unusual landform which was first observed during NASA's Mariner 9 mission in the early 1970's and is now shown here in an image from NASA's Mars Odyssey spacecraft.

White Rock

This image is a single frame from a computer animation, which begins with a global view of the planet Mars created from images by NASA's Mars Odyssey. Color is used to emphasize the Martian topographic, andesite, and basalt compositional differences.
This image is a single frame from a computer animation, which begins with a global view of the planet Mars created from images by NASA's Mars Odyssey. Color is used to emphasize the Martian topographic, andesite, and basalt compositional differences.

Still From Odyssey Clip 2

This anaglyph view of 'Shark' was produced by NASA's Mars Pathfinder's Imager camera. 3D glasses are necessary to identify surface detail.
This anaglyph view of 'Shark' was produced by NASA's Mars Pathfinder's Imager camera. 3D glasses are necessary to identify surface detail.

Shark in Super Resolution from Super Panorama

This view of 'Bookshelf Two' was produced by combining the 'Super Panorama' frames from the IMP camera from NASA's Mars Pathfinder lander. 3D glasses are necessary to identify surface detail.
This view of 'Bookshelf Two' was produced by combining the 'Super Panorama' frames from the IMP camera from NASA's Mars Pathfinder lander. 3D glasses are necessary to identify surface detail.

Bookshelf Two in Super Resolution from Super Panorama

This panoramic view taken by NASA's Mars Pathfinder is a controlled mosaic of approximately 300 IMP images. 3D glasses are necessary to identify surface detail.
This panoramic view taken by NASA's Mars Pathfinder is a controlled mosaic of approximately 300 IMP images. 3D glasses are necessary to identify surface detail.

Panoramic Views of the Landing site from Sagan Memorial Station

'Barnacle Bill' is a small rock immediately west-northwest of NASA's Mars Pathfinder lander and was the first rock visited by the rover Sojourner. 3D glasses are necessary to identify surface detail.
'Barnacle Bill' is a small rock immediately west-northwest of NASA's Mars Pathfinder lander and was the first rock visited by the rover Sojourner. 3D glasses are necessary to identify surface detail.

Super Resolution Anaglyph of Barnacle Bill

At right, NASA's Sojourner has traveled off the lander's rear ramp and onto the surface of Mars. The rock 'Barnacle Bill' and the rear ramp is to the left of Sojourner. 3-D glasses are necessary to identify surface detail.
At right, NASA's Sojourner has traveled off the lander's rear ramp and onto the surface of Mars. The rock 'Barnacle Bill' and the rear ramp is to the left of Sojourner. 3-D glasses are necessary to identify surface detail.

Sojourner near Barnacle Bill - 3-D

Many prominent rocks near the Sagan Memorial Station are featured in this image, from NASA's Mars Pathfinder. Wedge is at lower left; Shark, Half-Dome, and Pumpkin are at center. 3D glasses are necessary to identify surface detail.
Many prominent rocks near the Sagan Memorial Station are featured in this image, from NASA's Mars Pathfinder. Wedge is at lower left; Shark, Half-Dome, and Pumpkin are at center. 3D glasses are necessary to identify surface detail.

Sojourner's Favorite Rocks - in 3-D

Ancient lava flow in Cerberus Planitia is observed here by NASA's Mars Reconnaissance Orbiter.
Ancient lava flow in Cerberus Planitia is observed here by NASA's Mars Reconnaissance Orbiter.

Chevrons on a Flow Surface in Marte Vallis

This observation from NASA's Mars Reconnaissance Orbiter shows a beautiful example of gullies in a massif in Nereidum Montes, located in Argyre Planitia, one of the largest impact basins on Mars.
This observation from NASA's Mars Reconnaissance Orbiter shows a beautiful example of gullies in a massif in Nereidum Montes, located in Argyre Planitia, one of the largest impact basins on Mars.

Gullied Massif in the Nereidum Montes

In this image from NASA's Mars Reconnaissance Orbiter, we can see a small notch in a crater rim with a well-formed channel. Lava appears to have flowed through this notch and filled in this crater.
In this image from NASA's Mars Reconnaissance Orbiter, we can see a small notch in a crater rim with a well-formed channel. Lava appears to have flowed through this notch and filled in this crater.

Breaching a Crater Rim in Tartarus Montes

This image captured by NASA's Mars Reconnaissance Orbiter was intended to search for surface changes after three Mars years in a dust-covered region west of the Alba Mons volcano.
This image captured by NASA's Mars Reconnaissance Orbiter was intended to search for surface changes after three Mars years in a dust-covered region west of the Alba Mons volcano.

Looking for Changes in Dust Drifts West of Alba Mons

This image from NASA's Mars Reconnaissance Orbiter covers many shallow irregular pits with raised rims, concentrated along ridges and other topographic features.
This image from NASA's Mars Reconnaissance Orbiter covers many shallow irregular pits with raised rims, concentrated along ridges and other topographic features.

Mystery Martian Morphology of the Month

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