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This picture of a heart-shaped feature in Arabia Terra on Mars was taken on May 23, 2010, by NASA's Mars Reconnaissance Orbiter. A small impact crater near the tip of the heart is responsible for the formation of the bright, heart-shaped feature.
This picture of a heart-shaped feature in Arabia Terra on Mars was taken on May 23, 2010, by NASA's Mars Reconnaissance Orbiter. A small impact crater near the tip of the heart is responsible for the formation of the bright, heart-shaped feature.

Heart-Shaped Feature in Arabia Terra

The steep northern wall of Tithonium Chasma crosses this image from NASA's 2001 Mars Odyssey spacecraft. Landslide deposits from slope failure can be seen at the lower left corner of the image.
The steep northern wall of Tithonium Chasma crosses this image from NASA's 2001 Mars Odyssey spacecraft. Landslide deposits from slope failure can be seen at the lower left corner of the image.

Tithonium Chasma

The yellow line on this map shows where NASA's Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, upper left end of track, to a point about 2.2 miles away from reaching the rim of Endeavour crater.
The yellow line on this map shows where NASA's Mars Rover Opportunity has driven from the place where it landed in January 2004, inside Eagle crater, upper left end of track, to a point about 2.2 miles away from reaching the rim of Endeavour crater.

Eagle to Endeavour: Opportunity's Path, Sol 2609

A Martian rock in the 'Yellowknife Bay' area of Mars' Gale Crater is illuminated by white-light light emitting diodes.
A Martian rock in the 'Yellowknife Bay' area of Mars' Gale Crater is illuminated by white-light light emitting diodes.

MAHLI's First Night Imaging of Martian Rock, White Lighting

This image from the MAHLI camera on NASA's Mars rover Curiosity shows details of rock texture and color in an area where the rover's Dust Removal Tool (DRT) brushed away dust that was on the rock.
This image from the MAHLI camera on NASA's Mars rover Curiosity shows details of rock texture and color in an area where the rover's Dust Removal Tool (DRT) brushed away dust that was on the rock.

Close-up of Brushed Area on Martian Rock Target 'Ekwir_1'

Three images of the same location, taken by NASA's Mars Reconnaissance Orbiter at different times on Mars, show seasonal activity causing sand avalanches and ripple changes on a Martian dune. Time sequence of the images progresses from top to bottom.
Three images of the same location, taken by NASA's Mars Reconnaissance Orbiter at different times on Mars, show seasonal activity causing sand avalanches and ripple changes on a Martian dune. Time sequence of the images progresses from top to bottom.

Seasonal Changes in Northern Mars Dune Field

This view of Lyot Crater is a combined mapping by NASA's Project Viking with elevation information from Mars Global Surveyor showing at least one of the nine craters in the northern lowlands of Mars with exposures of hydrated minerals detected from orbit.
This view of Lyot Crater is a combined mapping by NASA's Project Viking with elevation information from Mars Global Surveyor showing at least one of the nine craters in the northern lowlands of Mars with exposures of hydrated minerals detected from orbit.

Hydrated Minerals Exposed at Lyot, Northern Mars

This false color image from NASA's rover Opportunity takes a look at Matijevic Hill, an area within the 'Cape York' segment of Endeavour's rim where clay minerals have been detected from orbit.
This false color image from NASA's rover Opportunity takes a look at Matijevic Hill, an area within the 'Cape York' segment of Endeavour's rim where clay minerals have been detected from orbit.

'Matijevic Hill' Panorama for Rover's Ninth Anniversary (False Color)

A sand dune field is located on the floor of this unnamed crater in Terra Cimmeria by NASA's 2001 Mars Odyssey spacecraft.
A sand dune field is located on the floor of this unnamed crater in Terra Cimmeria by NASA's 2001 Mars Odyssey spacecraft.

Sand Dunes in Terra Cimmeria

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of northeastern Syrtis Major. In this image are several windstreaks and a lava flow that has entered the crater on the top of the image.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of northeastern Syrtis Major. In this image are several windstreaks and a lava flow that has entered the crater on the top of the image.

Syrtis Major

The straight lines in Curiosity's zigzag track marks are Morse code for JPL. The 'footprint' is an important reference mark that the rover can use to drive more precisely via a system called visual odometry.
The straight lines in Curiosity's zigzag track marks are Morse code for JPL. The 'footprint' is an important reference mark that the rover can use to drive more precisely via a system called visual odometry.

Reading the Rover's Tracks

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 some of the plains of Sabaea 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 from NASA's 2001 Mars Odyssey spacecraft shows some of the plains of Sabaea Terra.

Terra Sabaea - False Color

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 part of Juventae 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 from NASA's 2001 Mars Odyssey spacecraft shows part of Juventae Chasma.

Juventae Chasma - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Olympia Undae, a large sand sea located near the north polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Olympia Undae, a large sand sea located near the north polar cap.

Olympia Undae

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 the surface of the south polar cap during springtime.
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 the surface of the south polar cap during springtime.

Southern Spring - False Color

This set of images from Mars shows the handiwork of different tools on three NASA missions to the surface of Mars.
This set of images from Mars shows the handiwork of different tools on three NASA missions to the surface of Mars.

Different Tools for Different Purposes on Mars

The power of the wind is undeniable in this image of the surface of Mars as seen by NASA's 2001 Mars Odyssey spacecraft.
The power of the wind is undeniable in this image of the surface of Mars as seen by NASA's 2001 Mars Odyssey spacecraft.

Wind Erosion

Dark slope streaks are visible on the rim of this unnamed crater located on the floor of Cassini Crater in this image from NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks are visible on the rim of this unnamed crater located on the floor of Cassini Crater in this image from NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

The pits at the top of this image are created by the action of the wind in this image captured by NASA's Mars Odyssey.
The pits at the top of this image are created by the action of the wind in this image captured by NASA's Mars Odyssey.

Wind Erosion

Clouds are common near the north polar caps throughout the spring and summer. The clouds typically cause a haze over the extensive dune fields. This image from NASA's Mars Odyssey shows the edge of the cloud front.
Clouds are common near the north polar caps throughout the spring and summer. The clouds typically cause a haze over the extensive dune fields. This image from NASA's Mars Odyssey shows the edge of the cloud front.

Clouds

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the South Polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the South Polar cap.

Polar Textures

This image from the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover shows detailed texture of a rock target called 'Elk' on Mars' Mount Sharp.
This image from the Chemistry and Camera (ChemCam) instrument on NASA's Curiosity Mars rover shows detailed texture of a rock target called 'Elk' on Mars' Mount Sharp.

Details on Silica-Rich 'Elk' Target near 'Marias Pass'

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rzvius Valles, located on the northern flank of Alba Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Rzvius Valles, located on the northern flank of Alba Mons.

Ravius Valles

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 the region at the start of Morava Valles in Margaritifer Terra.
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 the region at the start of Morava Valles in Margaritifer Terra.

Morava Valles - False Color

Sand dunes on the floor of Rabe Crater are brighter in this infrared image from NASA's 2001 Mars Odyssey spacecraft than the surrounding materials. This is because the sand is warmer than the surrounding rock.
Sand dunes on the floor of Rabe Crater are brighter in this infrared image from NASA's 2001 Mars Odyssey spacecraft than the surrounding materials. This is because the sand is warmer than the surrounding rock.

Rabe Dunes in IR

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