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The north/south trending parallel hills and valleys in this image captured by NASA's 2001 Mars Odyssey spacecraft were created by wind erosion and are called yardangs. These yardangs are located in Zephyria Planum.
The north/south trending parallel hills and valleys in this image captured by NASA's 2001 Mars Odyssey spacecraft were created by wind erosion and are called yardangs. These yardangs are located in Zephyria Planum.

Yardangs

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 false color image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed crater in Terra Cimmeria.
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 false color image from NASA's 2001 Mars Odyssey spacecraft shows an unnamed crater in Terra Cimmeria.

Crater - False Color

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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Coprates Chasma.
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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Coprates Chasma.

Coprates Chasma - False Color

This map shows where NASA's Mars rover Curiosity landed in August 2012 at 'Bradbury Landing.' All of these features are inside Gale Crater. Curiosity's next major destination, the entry point to the base of Mount Sharp.
This map shows where NASA's Mars rover Curiosity landed in August 2012 at 'Bradbury Landing.' All of these features are inside Gale Crater. Curiosity's next major destination, the entry point to the base of Mount Sharp.

From 'Glenelg' to Mount Sharp

The sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Hargraves Crater.
The sand dunes in this image from NASA's 2001 Mars Odyssey spacecraft are located on the floor of Hargraves Crater.

Hargraves Crater Dunes

A view from NASA's Mars Reconnaissance Orbiter on April 8, 2015, catches sight of NASA's Curiosity Mars rover passing through a valley called 'Artist's Drive' on the lower slope of Mount Sharp.
A view from NASA's Mars Reconnaissance Orbiter on April 8, 2015, catches sight of NASA's Curiosity Mars rover passing through a valley called 'Artist's Drive' on the lower slope of Mount Sharp.

Mars Orbiter Sees Curiosity Rover in 'Artist's Drive'

NASA's Mars Reconnaissance Orbiter's HiRISE, with its high resolution and eight years in orbit about Mars, has shown that many dunes and ripples on the planet are active.
NASA's Mars Reconnaissance Orbiter's HiRISE, with its high resolution and eight years in orbit about Mars, has shown that many dunes and ripples on the planet are active.

Hardened Dunes in Arcadia Planitia

This image from NASA's 2001 Mars Odyssey spacecraft is of Apollineris Mons, which shows erosion of the materials on it's southern flank.
This image from NASA's 2001 Mars Odyssey spacecraft is of Apollineris Mons, which shows erosion of the materials on it's southern flank.

Apollinaris Mons

This image captured by NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel located on the northwest margin of Arabia Terra.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows an unnamed channel located on the northwest margin of Arabia Terra.

Channel

Dark slope streaks mark many of the hills in this image captured by NASA's 2001 Mars Odyssey spacecraft. This region of hills is called Tartarus Colles. The term colles means small hills or knobs.
Dark slope streaks mark many of the hills in this image captured by NASA's 2001 Mars Odyssey spacecraft. This region of hills is called Tartarus Colles. The term colles means small hills or knobs.

Tartarus Colles

The surface textures located southeast of Aeolis Planum likely had wind action as one of the contributing processes, as shown by NASA's 2001 Mars Odyssey spacecraft.
The surface textures located southeast of Aeolis Planum likely had wind action as one of the contributing processes, as shown by NASA's 2001 Mars Odyssey spacecraft.

Surface Textures

The ridges and mesas in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Hydraotes Chaos.
The ridges and mesas in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Hydraotes Chaos.

Hydraotes Chaos

At the eastern end of Valles Marineris the chasma floors are typically filled with the hills and mounds of chaos terrain as seen by NASA's Mars Odyssey.
At the eastern end of Valles Marineris the chasma floors are typically filled with the hills and mounds of chaos terrain as seen by NASA's Mars Odyssey.

Eos Chasma

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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Renaudot Crater.
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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Renaudot Crater.

Renaudot Crater - False Color

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Melas Chasma.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Melas Chasma.

Melas Chasma

The channel feature in this image from NASA's 2001 Mars Odyssey spacecraft is a huge gully that empties into Echus Chasma.
The channel feature in this image from NASA's 2001 Mars Odyssey spacecraft is a huge gully that empties into Echus Chasma.

Mega Gully

This image from NASA's Mars Odyssey is of the south polar surface. These pits appear to coalesce and reveal the surface below.
This image from NASA's Mars Odyssey is of the south polar surface. These pits appear to coalesce and reveal the surface below.

South Polar Surface

Located on the margin of Zephyria Planum, this image from NASA's 2001 Mars Odyssey shows the effect the wind has had on the surface of Mars. Loose materials have been removed and semi-consolidated materials have been eroded into narrow hill forms.
Located on the margin of Zephyria Planum, this image from NASA's 2001 Mars Odyssey shows the effect the wind has had on the surface of Mars. Loose materials have been removed and semi-consolidated materials have been eroded into narrow hill forms.

Wind Effects

This image from NASA's Mars Reconnaissance Orbiter shows dark dunes in the western Medusae Fossae. This image shows no large dunes, but many of the dark sand patches cover slopes up to discrete layers.
This image from NASA's Mars Reconnaissance Orbiter shows dark dunes in the western Medusae Fossae. This image shows no large dunes, but many of the dark sand patches cover slopes up to discrete layers.

Dunes in Western Medusae Fossae Formation

This false color image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the complex region at the west end of Candor Chasma.
This false color image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the complex region at the west end of Candor Chasma.

Candor Chasma - False Color

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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Hargraves Crater.
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 false color image from NASA's 2001 Mars Odyssey spacecraft shows part of Hargraves Crater.

Hargraves Crater - False Color

Data graphed here are examples from the Sample Analysis at Mars (SAM) laboratory's detection of Martian organics in a sample of powder that the drill on NASA's Curiosity Mars rover collected from a rock target called 'Cumberland.'
Data graphed here are examples from the Sample Analysis at Mars (SAM) laboratory's detection of Martian organics in a sample of powder that the drill on NASA's Curiosity Mars rover collected from a rock target called 'Cumberland.'

Some Data from Detection of Organics in a Rock on Mars

By measuring absorption of light at specific wavelengths, Tunable Laser Spectrometer (TLS) onboard NASA's Curiosity measures concentrations of methane, carbon dioxide and water vapor in Mars' atmosphere.
By measuring absorption of light at specific wavelengths, Tunable Laser Spectrometer (TLS) onboard NASA's Curiosity measures concentrations of methane, carbon dioxide and water vapor in Mars' atmosphere.

Tunable Laser Spectrometer on NASA's Curiosity Mars Rover

This diagram depicts rivers entering a lake. Where the water's flow decelerates, sediments drop out, and a delta forms, depositing a prism of sediment that tapers out toward the lake's interior.
This diagram depicts rivers entering a lake. Where the water's flow decelerates, sediments drop out, and a delta forms, depositing a prism of sediment that tapers out toward the lake's interior.

How a Delta Forms Where River Meets Lake

This image from NASA's 2001 Mars Odyssey spacecraft shows several channels dissecting the rim of Semeykin Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows several channels dissecting the rim of Semeykin Crater.

Semeykin Crater

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