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This image from NASA's 2001 Mars Odyssey spacecraft shows streamlined islands within part of Kasei Valles.
This image from NASA's 2001 Mars Odyssey spacecraft shows streamlined islands within part of Kasei Valles.

Kasei Valles

This map shows the route that NASA's Curiosity Mars rover drove inside Gale Crater from its landing in August 2013 through Jan. 26, 2004. The rover is approaching a gap between two low scarps, 'Dingo Gap.'
This map shows the route that NASA's Curiosity Mars rover drove inside Gale Crater from its landing in August 2013 through Jan. 26, 2004. The rover is approaching a gap between two low scarps, 'Dingo Gap.'

Traverse Map for Mars Rover Curiosity as of Jan. 26, 2014

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? There is a mickey mouse hat sitting on the top right side of this daytime infrared image.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? There is a mickey mouse hat sitting on the top right side of this daytime infrared image.

THEMIS Art #112

Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is both tectonically fractured rocks (top) and volcanic flows (middle and bottom). This image is from NASA's 2001 Mars Odyssey spacecraft.
Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is both tectonically fractured rocks (top) and volcanic flows (middle and bottom). This image is from NASA's 2001 Mars Odyssey spacecraft.

Echus Chasma

This image, captured by NASA's Mars Odyssey on Sept. 9, 2010, shows some of the dunes of the floor of Moreux Crater.
This image, captured by NASA's Mars Odyssey on Sept. 9, 2010, shows some of the dunes of the floor of Moreux Crater.

Moreux Crater Dunes

Two landslide deposits are visible in this image of Tithonium Chasma taken by NASA's 2001 Mars Odyssey spacecraft.
Two landslide deposits are visible in this image of Tithonium Chasma taken by NASA's 2001 Mars Odyssey spacecraft.

Tithonium Chasma

This image uses a view from the navigation camera on NASA's Mars Exploration Rover Opportunity to show context for a horizon shot by the rover's narrower-angle panoramic camera of the rim of Endeavour crater.
This image uses a view from the navigation camera on NASA's Mars Exploration Rover Opportunity to show context for a horizon shot by the rover's narrower-angle panoramic camera of the rim of Endeavour crater.

Endeavour on the Horizon (Context View)

This daytime IR image from shows NASA's 2001 Mars Odyssey spacecraft part of the dune field on the floor of Rabe Crater. The dunes show up as brighter than the surrounding materials because they are warmer.
This daytime IR image from shows NASA's 2001 Mars Odyssey spacecraft part of the dune field on the floor of Rabe Crater. The dunes show up as brighter than the surrounding materials because they are warmer.

Rabe Crater Dunes

The appearance of the dunes in the North Polar Erg (or sand sea) changes as the seasons move from winter to summer. This summer image from NASA's Mars Odyssey shows the dunes totally free of frost.
The appearance of the dunes in the North Polar Erg (or sand sea) changes as the seasons move from winter to summer. This summer image from NASA's Mars Odyssey shows the dunes totally free of frost.

North Polar Dunes

The channels in this image are part of Ravi Vallis as seen by NASA's 2001 Mars Odyssey spacecraft.
The channels in this image are part of Ravi Vallis as seen by NASA's 2001 Mars Odyssey spacecraft.

Ravi Vallis

This graphic from NASA's Curiosity mission shows close-ups of light-toned veins in rocks in the 'Yellowknife Bay' area of Mars together with analyses of their composition.
This graphic from NASA's Curiosity mission shows close-ups of light-toned veins in rocks in the 'Yellowknife Bay' area of Mars together with analyses of their composition.

Calcium-Rich Veins in Martian Rocks

Dunes cover the floor of Bopolu Crater in Meridiani Planum in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Dunes cover the floor of Bopolu Crater in Meridiani Planum in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Bopolu Dunes

The layered ridge and mesas in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern margin of Hellas Basin.
The layered ridge and mesas in this image from NASA's 2001 Mars Odyssey spacecraft are located on the northern margin of Hellas Basin.

Layering

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Elysium Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Elysium Mons.

Elysium Mons

These windstreaks are located on Syrtis Major Planum, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
These windstreaks are located on Syrtis Major Planum, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Windstreaks

The depressions and offset ridge in this image captured by NASA's Mars Odyssey spacecraft are evidence of faulting in this region of Sinai Dorsa.
The depressions and offset ridge in this image captured by NASA's Mars Odyssey spacecraft are evidence of faulting in this region of Sinai Dorsa.

Faults

This graphic depicts the relative shapes and distances from Mars for five active orbiter missions plus the planet's two natural satellites. It illustrates the potential for intersections of the spacecraft orbits.
This graphic depicts the relative shapes and distances from Mars for five active orbiter missions plus the planet's two natural satellites. It illustrates the potential for intersections of the spacecraft orbits.

Diverse Orbits Around Mars (Graphic)

In February 2015, NASA's Mars Exploration Rover Opportunity is approaching a cumulative driving distance on Mars equal to the length of a marathon race. This map shows the rover's position relative to where it could surpass that distance.
In February 2015, NASA's Mars Exploration Rover Opportunity is approaching a cumulative driving distance on Mars equal to the length of a marathon race. This map shows the rover's position relative to where it could surpass that distance.

Opportunity Rover Nears Mars Marathon Feat

This northeast-facing view from the lower edge of the pale 'Pahrump Hills' outcrop at the base of Mount Sharp includes wind-sculpted ripples of sand and dust in the middle ground. It was taken by Curiosity's Navcam on Nov. 13, 2014.
This northeast-facing view from the lower edge of the pale 'Pahrump Hills' outcrop at the base of Mount Sharp includes wind-sculpted ripples of sand and dust in the middle ground. It was taken by Curiosity's Navcam on Nov. 13, 2014.

Ripples Beside 'Pahrump Hills' Outcrop at Base of Mount Sharp

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

More Polar Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive lava flows that comprise Daedalia Planum.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the extensive lava flows that comprise Daedalia Planum.

Daedalia Planum

This image from NASA's Mars Odyssey shows are region of lava covered plains east of Olympus Mons. Winds are common in the area and have created windstreaks downwind of craters in the region and on the lava flows.
This image from NASA's Mars Odyssey shows are region of lava covered plains east of Olympus Mons. Winds are common in the area and have created windstreaks downwind of craters in the region and on the lava flows.

Tharsis Lava

Dunes appear on the floor of Nili Patera, one of the two volcanic calderas of Syrtis Major in this image taken by NASA's 2001 Mars Odyssey.
Dunes appear on the floor of Nili Patera, one of the two volcanic calderas of Syrtis Major in this image taken by NASA's 2001 Mars Odyssey.

Nili Patera Dunes

Dark slope streaks, like the ones in this unnamed crater in Terra Sabaea, are believed to be formed when surface dust is displaced and the darker rock below is exposed. Rocks falling due to gravity likely formed these streaks.
Dark slope streaks, like the ones in this unnamed crater in Terra Sabaea, are believed to be formed when surface dust is displaced and the darker rock below is exposed. Rocks falling due to gravity likely formed these streaks.

Dark Slope Streak

As NASA's Mars rover Curiosity is progressing toward Mount Sharp, researchers are using the rover's RIM and ChemCam instruments to examine soils and rocks in Gale Crater.
As NASA's Mars rover Curiosity is progressing toward Mount Sharp, researchers are using the rover's RIM and ChemCam instruments to examine soils and rocks in Gale Crater.

Crystal-Laden Martian Rock Examined by Curiosity's Laser Instrument

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