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NASA's Mars Exploration Rover Spirit used its microscopic imager to capture this spectacular, jagged mini-landscape on a rock called 'GongGong.'
NASA's Mars Exploration Rover Spirit used its microscopic imager to capture this spectacular, jagged mini-landscape on a rock called 'GongGong.'

Hardened Lava Meets Wind on Mars

Tiu Valles is the location of the streamlined island in this image from NASA's 2001 Mars Odyssey spacecraft.
Tiu Valles is the location of the streamlined island in this image from NASA's 2001 Mars Odyssey spacecraft.

Tiu Valles

This region of Tharsis near Olympus Mons contains subtle features showing its lava flow origin. Note the 'softened' flow fronts and lava channels in this image captured by NASA's Mars Odyssey spacecraft.
This region of Tharsis near Olympus Mons contains subtle features showing its lava flow origin. Note the 'softened' flow fronts and lava channels in this image captured by NASA's Mars Odyssey spacecraft.

Tharsis Lava

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

Hebes Chasma

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

Terra Cimmeria

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Ma'adim Vallis, which is a large channel that enters Gusev Crater from the south.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Ma'adim Vallis, which is a large channel that enters Gusev Crater from the south.

Ma'adim Vallis

This infrared image from NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Rabe Crater. The dunes are 'brighter' than the surrounding material, indicating that they are warmer.
This infrared image from NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Rabe Crater. The dunes are 'brighter' than the surrounding material, indicating that they are warmer.

Rabe Crater Dunes

The small channel in this image from NASA's 2001 Mars Odyssey spacecraft is located on the floor of Newton Crater.
The small channel in this image from NASA's 2001 Mars Odyssey spacecraft is located on the floor of Newton Crater.

Channel

This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Dittaino Valles.
This image from NASA's 2001 Mars Odyssey spacecraft shows a portion of Dittaino Valles.

Dittaino Valles

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the sand sheet and dunes on the floor of Rabe Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the sand sheet and dunes on the floor of Rabe Crater.

Rabe Crater Dunes

Gullies dissect the rim of this unnamed crater on the northern margin of Argyre Planitia in this image from NASA's 2001 Mars Odyssey spacecraft.
Gullies dissect the rim of this unnamed crater on the northern margin of Argyre Planitia in this image from NASA's 2001 Mars Odyssey spacecraft.

Gullies on Argyre Planitia

NASA's 2001 Mars Odyssey captured dark slope streaks, like the ones on the rim of a unnamed crater in Terra Sabaea, are thought to have been formed by material moving down slope due to gravity.
NASA's 2001 Mars Odyssey captured dark slope streaks, like the ones on the rim of a unnamed crater in Terra Sabaea, are thought to have been formed by material moving down slope due to gravity.

Dark Slope Streaks

The channel-like features in this image captured by NASA's Mars Odyssey are fault bounded down-dropped blocks of material. These tectonic features are called Labaetis Fossae and are located on the eastern margin of the Tharsis Volcanic complex.
The channel-like features in this image captured by NASA's Mars Odyssey are fault bounded down-dropped blocks of material. These tectonic features are called Labaetis Fossae and are located on the eastern margin of the Tharsis Volcanic complex.

Labeatis Fossae

This map shows the route driven by NASA's Curiosity Mars in its approach to and April 1, 2014, arrival at a waypoint called 'the Kimberley,' which rover team scientists chose in 2013 as the location for the mission's next major investigations.
This map shows the route driven by NASA's Curiosity Mars in its approach to and April 1, 2014, arrival at a waypoint called 'the Kimberley,' which rover team scientists chose in 2013 as the location for the mission's next major investigations.

Map of Curiosity Mars Rover's Drives to 'the Kimberley' Waypoint

Stages in the seasonal disappearance of surface ice from the ground around the Phoenix Mars Lander are visible in these images taken by NASA's Mars Reconnaissance Rover on 2-8-2010 and 2-25-2010, during springtime on northern Mars.
Stages in the seasonal disappearance of surface ice from the ground around the Phoenix Mars Lander are visible in these images taken by NASA's Mars Reconnaissance Rover on 2-8-2010 and 2-25-2010, during springtime on northern Mars.

Ice Around Phoenix Lander Continues to Lessen in Spring

The edge of the south polar cap is the bright band in the center of this image captured by NASA's 2001 Mars Odyssey spacecraft.
The edge of the south polar cap is the bright band in the center of this image captured by NASA's 2001 Mars Odyssey spacecraft.

Polar Dunes

This map traces where NASA's Mars rover Curiosity drove between landing at a site subsequently named 'Bradbury Landing,' and the position reached during the mission's 123rd Martian day, or sol, (Aug. 10, 2012).
This map traces where NASA's Mars rover Curiosity drove between landing at a site subsequently named 'Bradbury Landing,' and the position reached during the mission's 123rd Martian day, or sol, (Aug. 10, 2012).

Curiosity Traverse Map, Sol 123

This complex set of dunes is located in an unnamed crater in Arabia Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
This complex set of dunes is located in an unnamed crater in Arabia Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Arabia Terra Dunes

This image from NASA's 2001 Mars Odyssey spacecraft shows a clear boundary between material being eroded by the wind (bottom of image) and a surface scoured clean (top of frame) northwest of Apollinaris Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows a clear boundary between material being eroded by the wind (bottom of image) and a surface scoured clean (top of frame) northwest of Apollinaris Mons.

Boundaries

Today's image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, which is comprised of lava flows from Arsia Mons. Note the small channel in the image. This channel was likely created by lava rather than water flow.
Today's image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, which is comprised of lava flows from Arsia Mons. Note the small channel in the image. This channel was likely created by lava rather than water flow.

Daedalia Planum

This image from NASA's Mars Reconnaissance Orbiter shows a graben (a trough formed when the ground drops between two parallel faults) and a lava flow in the Tharsis volcanic province of Mars. North is up.
This image from NASA's Mars Reconnaissance Orbiter shows a graben (a trough formed when the ground drops between two parallel faults) and a lava flow in the Tharsis volcanic province of Mars. North is up.

Graben Cutting Lava Flow in Tharsis

This image captured by NASA's 2001 Mars Odyssey shows a portion of the northeastern flank of Ascraeus Mons.
This image captured by NASA's 2001 Mars Odyssey shows a portion of the northeastern flank of Ascraeus Mons.

Ascraeus Mons

The amount of sand in this region of Juventae Chasma has coalesced into a sand sheet, rather than individual dune forms. Wind continues to sculpt the sand around high standing hills in this image from NASA's Mars Odyssey.
The amount of sand in this region of Juventae Chasma has coalesced into a sand sheet, rather than individual dune forms. Wind continues to sculpt the sand around high standing hills in this image from NASA's Mars Odyssey.

Juventae Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft is located southwest of Olympus Mons, shows the end of a lava flow that has flowed between the hills at the upper left portion of the image.
This image captured by NASA's 2001 Mars Odyssey spacecraft is located southwest of Olympus Mons, shows the end of a lava flow that has flowed between the hills at the upper left portion of the image.

Lava End

This view of the lower front and underbelly areas of NASA's Mars rover Curiosity was taken by the rover's MAHLI camera during Sept. 9, 2012. Also visible are the hazard avoidance cameras on the front of the rover.
This view of the lower front and underbelly areas of NASA's Mars rover Curiosity was taken by the rover's MAHLI camera during Sept. 9, 2012. Also visible are the hazard avoidance cameras on the front of the rover.

Belly Check for Curiosity

Currently displaying images 1801-1825 of 3022
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