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NASA's 2001 Mars Odyssey captured this image of individual dunes located on the floor of Briault Crater.
NASA's 2001 Mars Odyssey captured this image of individual dunes located on the floor of Briault Crater.

Briault Crater Dunes

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

Several Landslides on Coprates Chasma

The mitten-shaped feature in Candor Chasma is a landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft.
The mitten-shaped feature in Candor Chasma is a landslide deposit in this image from NASA's 2001 Mars Odyssey spacecraft.

Candor Chasma

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Sulci Gordii, a complexly fractured region east of Olympus Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Sulci Gordii, a complexly fractured region east of Olympus Mons.

Sulci Gordii

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Siton Undae, one of the dune fields near the north polar cap.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Siton Undae, one of the dune fields near the north polar cap.

Siton Undae

The dunes seen in this view from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Brashear Crater.
The dunes seen in this view from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Brashear Crater.

Brashear Crater Dunes

The intersecting ridges in this image from NASA's 2001 Mars Odyssey spacecraft are part of Angustus Labyrinthus, informally called Inca City.
The intersecting ridges in this image from NASA's 2001 Mars Odyssey spacecraft are part of Angustus Labyrinthus, informally called Inca City.

Angustus Laybrinthus

The graben in this image from NASA's 2001 Mars Odyssey spacecraft is Cyane Fossae. The lava flows are part of the extensive Tharsis volcanic flows.
The graben in this image from NASA's 2001 Mars Odyssey spacecraft is Cyane Fossae. The lava flows are part of the extensive Tharsis volcanic flows.

Cyane Fossae

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Elysium Planitia and were likely created by lava flow.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft are located in Elysium Planitia and were likely created by lava flow.

Channels

This pair of graphs shows about one-fourth of a Martian year's record of temperatures (in degrees Celsius) measured by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.
This pair of graphs shows about one-fourth of a Martian year's record of temperatures (in degrees Celsius) measured by the Rover Environmental Monitoring Station (REMS) on NASA's Curiosity rover.

Steady Temperatures at Mars' Gale Crater

This image NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Brashear Crater.
This image NASA's 2001 Mars Odyssey spacecraft shows part of the dune field on the floor of Brashear Crater.

Brashear Dunes

This image from NASA's 2001 Mars Odyssey spacecraft of a ridge in the Tharsis region (called Uranius Dorsum) reminds one of a skeletal spine.
This image from NASA's 2001 Mars Odyssey spacecraft of a ridge in the Tharsis region (called Uranius Dorsum) reminds one of a skeletal spine.

Uranius Dorsum

The channel-like features in image captured by NASA's 2001 Mars Odyssey spacecraft are fracture sets related to the formation of Iani Chaos, which occurs directly north of the image.
The channel-like features in image captured by NASA's 2001 Mars Odyssey spacecraft are fracture sets related to the formation of Iani Chaos, which occurs directly north of the image.

Iani Chaos

This image from NASA's Mars Odyssey shows a portion of a large landslide deposit in Ius Chasma.
This image from NASA's Mars Odyssey shows a portion of a large landslide deposit in Ius Chasma.

Ius Chasma Landslide

As northern summer approaches on Mars, dunes near the pole defrost and become darker appearing as shown in this image from NASA's Mars Odyssey captured on July 8, 2010.
As northern summer approaches on Mars, dunes near the pole defrost and become darker appearing as shown in this image from NASA's Mars Odyssey captured on July 8, 2010.

Polar Dunes

Twelve orbits a day provide NASA's Mars Global Surveyor MOC wide angle cameras a global 'snapshot' of weather patterns across the planet. Here, bluish-white water ice clouds hang above the Tharsis volcanoes.
Twelve orbits a day provide NASA's Mars Global Surveyor MOC wide angle cameras a global 'snapshot' of weather patterns across the planet. Here, bluish-white water ice clouds hang above the Tharsis volcanoes.

Mars Daily Global Image from April 1999

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the dunes on the floor of Bogia Crater, a crater in Hellas Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the dunes on the floor of Bogia Crater, a crater in Hellas Planitia.

Bogia Crater Dunes

The complex channel in this image is a small section of Reull Vallis as seen by NASA's 2001 Mars Odyssey spacecraft.
The complex channel in this image is a small section of Reull Vallis as seen by NASA's 2001 Mars Odyssey spacecraft.

Reull Vallis

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? The group of craters at the bottom of the image look like a muppet.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? The group of craters at the bottom of the image look like a muppet.

THEMIS Art #122

The fracture system shown in this image from NASA's Mars Odyssey is on the northern margin of the Kasei Valles lowland. Fractures like this can become chaos with continued downdropping of blocks and widening fractures.
The fracture system shown in this image from NASA's Mars Odyssey is on the northern margin of the Kasei Valles lowland. Fractures like this can become chaos with continued downdropping of blocks and widening fractures.

Kasei Valles Fractures

The Russell Crater dune field is covered seasonally by carbon dioxide frost; this image from NASA's Mars Reconnaissance Orbiter shows the dune field after the frost has sublimated. There are just a few patches left of the bright seasonal frost.
The Russell Crater dune field is covered seasonally by carbon dioxide frost; this image from NASA's Mars Reconnaissance Orbiter shows the dune field after the frost has sublimated. There are just a few patches left of the bright seasonal frost.

Russell Crater Dunes, Defrosted

The dunes in this image captured by NASA's 2001 Mars Odyssey are located in an unnamed crater in Terra Cimmeria.
The dunes in this image captured by NASA's 2001 Mars Odyssey are located in an unnamed crater in Terra Cimmeria.

Dunes in Terra Cimmeria

This image, captured by NASA's Mars Odyssey on May 23, 2010 of Daedalia Planum, shows various lava flows from Arsia Mons.
This image, captured by NASA's Mars Odyssey on May 23, 2010 of Daedalia Planum, shows various lava flows from Arsia Mons.

Daedalia Planum

Richardson Crater is home to this sea of sand dunes. It was fall in the Southern hemisphere when NASA's MRO acquired this image of the dunes frosted with the first bit of carbon dioxide ice condensed from the atmosphere.
Richardson Crater is home to this sea of sand dunes. It was fall in the Southern hemisphere when NASA's MRO acquired this image of the dunes frosted with the first bit of carbon dioxide ice condensed from the atmosphere.

Fall Frosting

This diagram shows how materials analyzed by the ChemCam instrument on NASA's Curiosity Mars rover during the first 100 Martian days of the mission differed with regard to hydrogen content (horizontal axis) and alkali (vertical axis).
This diagram shows how materials analyzed by the ChemCam instrument on NASA's Curiosity Mars rover during the first 100 Martian days of the mission differed with regard to hydrogen content (horizontal axis) and alkali (vertical axis).

Curiosity's ChemCam Analyzes Rocks, Soils and Dust

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