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NASA's Mars Odyssey spacecraft captured this image of dunes located in Aonia Terra.
NASA's Mars Odyssey spacecraft captured this image of dunes located in Aonia Terra.

Dunes in Aonia Terra

North polar troughs are the typical location to see evidence of strong polar surface winds. This image captured by NASA's 2001 Mars Odyssey shows 'streamers' of clouds created by catabatic winds.
North polar troughs are the typical location to see evidence of strong polar surface winds. This image captured by NASA's 2001 Mars Odyssey shows 'streamers' of clouds created by catabatic winds.

Polar Winds

This image taken by NASA's Mars Reconnaissance Orbiter shows a series of parallel layers eroding into peculiar knobs and hills.
This image taken by NASA's Mars Reconnaissance Orbiter shows a series of parallel layers eroding into peculiar knobs and hills.

Reading the Geologic Record

On Feb. 19, 2005, NASA's Mars Exploration Rover Opportunity set a one-day distance record for martian driving; Opportunity rolled 177.5 meters (582 feet) across the plain of Meridiani. 3-D glasses are necessary to view this image.
On Feb. 19, 2005, NASA's Mars Exploration Rover Opportunity set a one-day distance record for martian driving; Opportunity rolled 177.5 meters (582 feet) across the plain of Meridiani. 3-D glasses are necessary to view this image.

Record Drive Day, Opportunity Sol 383 (3-D)

Dynamic Albedo of Neutrons (DAN), measures the flow of neutrons with different energy levels returning from the ground, and their delay times, as an indication of the amount and depth of hydrogen in the ground beneath the NASA's rover, Curiosity.
Dynamic Albedo of Neutrons (DAN), measures the flow of neutrons with different energy levels returning from the ground, and their delay times, as an indication of the amount and depth of hydrogen in the ground beneath the NASA's rover, Curiosity.

Russian Hydrogen-Checking Instrument on Curiosity Fires 2 Millionth Pulse

These dunes are moving along the hard volcanic surface Nili Patera in Syrtis Major. This image was captured by NASA's Mars Odyssey.
These dunes are moving along the hard volcanic surface Nili Patera in Syrtis Major. This image was captured by NASA's Mars Odyssey.

Nili Patera Dunes

This image captured by NASA's Mars Odyssey shows parts of two giant gully that are located on the southern side of Ius Chasma. Ius Chasma has the largest number of mega gullies of any of the chasmata that make up Valles Marineris.
This image captured by NASA's Mars Odyssey shows parts of two giant gully that are located on the southern side of Ius Chasma. Ius Chasma has the largest number of mega gullies of any of the chasmata that make up Valles Marineris.

Ius Chasma Mega Gullies

This subtle, unnamed channel is located in northern Terra Cimmeria as seen by NASA's Mars Odyssey.
This subtle, unnamed channel is located in northern Terra Cimmeria as seen by NASA's Mars Odyssey.

Channel in Terra Cimmeria

A sandsheet with dune forms covers most of the floor of this unnamed crater within Coprates Chasma in this image captured by NASA's Mars Odyssey on June 23, 2010.
A sandsheet with dune forms covers most of the floor of this unnamed crater within Coprates Chasma in this image captured by NASA's Mars Odyssey on June 23, 2010.

Dunes Within Coprates Chasma

This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a large landslide deposit in an unnamed crater southwest of Holden Crater.
This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows a large landslide deposit in an unnamed crater southwest of Holden Crater.

Landslide Southwest of Holden Crater

This image from NASA's 2001 Mars Odyssey shows a delta deposit on the floor of Holden Crater. This delta was formed by small channels dissecting the rim of the crater, rather than the influx of material from Uzboi Vallis.
This image from NASA's 2001 Mars Odyssey shows a delta deposit on the floor of Holden Crater. This delta was formed by small channels dissecting the rim of the crater, rather than the influx of material from Uzboi Vallis.

Holden Crater Delta

This image, taken by NASA's Mars Odyssey, shows a short section of Nirgal Vallis. Several tributaries are visible in this image.
This image, taken by NASA's Mars Odyssey, shows a short section of Nirgal Vallis. Several tributaries are visible in this image.

Nirgal Vallis

The High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter captured this image of spider-shaped features on Mars, carved by vaporizing dry ice.
The High Resolution Imaging Science Experiment camera on NASA's Mars Reconnaissance Orbiter captured this image of spider-shaped features on Mars, carved by vaporizing dry ice.

Radial Channels Carved by Dry Ice

Using observations from NASA's Mars Reconnaissance Orbiter, this map shows five locations where fresh impact cratering has excavated water ice from just beneath the surface of Mars.
Using observations from NASA's Mars Reconnaissance Orbiter, this map shows five locations where fresh impact cratering has excavated water ice from just beneath the surface of Mars.

Expected Depths to Ice, Mid-Latitude Northern Mars

This mosaic image was taken with the microscopic imager on NASA's Mars Exploration Rover Spirit to get a look underneath the rover.
This mosaic image was taken with the microscopic imager on NASA's Mars Exploration Rover Spirit to get a look underneath the rover.

Spirit's View of Own Underbelly, Sol 1990

NASA's Mars Exploration Rover Spirit used its navigation camera to take the images assembled into this stereo, 120-degree view southward after a short drive on February 3, 2009. 3D glasses are necessary to view this image.
NASA's Mars Exploration Rover Spirit used its navigation camera to take the images assembled into this stereo, 120-degree view southward after a short drive on February 3, 2009. 3D glasses are necessary to view this image.

Spirit Beside 'Home Plate,' Sol 1809 (Stereo)

The robotic arm on NASA's Phoenix Mars Lander slid a rock out of the way on Sept. 22, 2008 to gain access to soil that had been underneath the rock. 3D glasses are necessary to view this image.
The robotic arm on NASA's Phoenix Mars Lander slid a rock out of the way on Sept. 22, 2008 to gain access to soil that had been underneath the rock. 3D glasses are necessary to view this image.

Rock Moved by Mars Lander Arm, Stereo View

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)

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