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NASA's 2001 Mars Odyssey spacecraft took this image of Candor Chasma showing a complex region of eroded layered deposits.
NASA's 2001 Mars Odyssey spacecraft took this image of Candor Chasma showing a complex region of eroded layered deposits.

Candor Chasma

NASA's 2001 Mars Odyssey spacecraft captured numerous dark slope streaks in this small unnamed crater in Zephyria Planum.
NASA's 2001 Mars Odyssey spacecraft captured numerous dark slope streaks in this small unnamed crater in Zephyria Planum.

Dark Slope Streaks

One of the great strengths of the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is that its high resolution can help resolve interesting questions. Here, is the platy flow material younger than the yardang-forming material?
One of the great strengths of the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter is that its high resolution can help resolve interesting questions. Here, is the platy flow material younger than the yardang-forming material?

Which Came First, the Yardang or the Platy Flow?

This image from NASA's Mars Odyssey spacecraft shows the highest elevation of layered deposit occurs at the top, but just south of the center of the image is a peak that does not appear to be layered and is eroding differently than the rest of Mt. Sharp.
This image from NASA's Mars Odyssey spacecraft shows the highest elevation of layered deposit occurs at the top, but just south of the center of the image is a peak that does not appear to be layered and is eroding differently than the rest of Mt. Sharp.

Images of Gale #14

The lava flows in this image are part of Daedalia Planum as seen by NASA's 2001 Mars Odyssey spacecraft.
The lava flows in this image are part of Daedalia Planum as seen by NASA's 2001 Mars Odyssey spacecraft.

Daedalia Planum

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.

Daedalia Planum

This image from NASA's 2001 Mars Odyssey spacecraft shows the complex collapse features on the southern flank of Ascraeus Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows the complex collapse features on the southern flank of Ascraeus Mons.

Ascraeus Mon

This image from NASA's Mars Odyssey shows dunes on the floor of an unnamed crater west of Herschel Crater.
This image from NASA's Mars Odyssey shows dunes on the floor of an unnamed crater west of Herschel Crater.

Sand Dunes

The wind is responsible for the erosion seen in this image captured by NASA's 2001 Mars Odyssey spacecraft near Aeolis Planum.
The wind is responsible for the erosion seen in this image captured by NASA's 2001 Mars Odyssey spacecraft near Aeolis Planum.

Erosion

Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? Another bug!
Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? Another bug!

THEMIS Art #107

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

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