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This image captured by NASA's Mars Reconnaissance Orbiter is of an area called Aram Dorsum (also known by its old name, Oxia Palus) that has been suggested for the 2018/2020 ExoMars Rover because it contains an ancient, exhumed alluvial system.
This image captured by NASA's Mars Reconnaissance Orbiter is of an area called Aram Dorsum (also known by its old name, Oxia Palus) that has been suggested for the 2018/2020 ExoMars Rover because it contains an ancient, exhumed alluvial system.

A Possible Landing Site in Aram Dorsum for the ExoMars Rover

Dark slope streaks are common throughout Lycus Sulci as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks are common throughout Lycus Sulci as seen by NASA's 2001 Mars Odyssey spacecraft.

Lycus Sulci

With southern summer drawing to a close, the surface of the polar ice cap will begin to frost over on Mars as seen by NASA's 2001 Mars Odyssey spacecraft.
With southern summer drawing to a close, the surface of the polar ice cap will begin to frost over on Mars as seen by NASA's 2001 Mars Odyssey spacecraft.

South Polar Surface

This image from NASA's 2001 Mars Odyssey spacecraft shows the northern margin of Beatis Mensa, a large mound of material in the center of Ophir Chasma.
This image from NASA's 2001 Mars Odyssey spacecraft shows the northern margin of Beatis Mensa, a large mound of material in the center of Ophir Chasma.

Beatis Mensa

The lava flows in this image from NASA's 2001 Mars Odyssey spacecraft are located east of Olympus Mons.
The lava flows in this image from NASA's 2001 Mars Odyssey spacecraft are located east of Olympus Mons.

Lava Flows

This image shows warm-season flows on a north-facing slope in middle southern latitudes of Mars. It was taken by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter on June 24, 2011. The season was summer in Mars' southern hemisphere.
This image shows warm-season flows on a north-facing slope in middle southern latitudes of Mars. It was taken by the HiRISE camera onboard NASA's Mars Reconnaissance Orbiter on June 24, 2011. The season was summer in Mars' southern hemisphere.

Site of Warm Season Flows in Mars Crater

Dunes and the distal end of a landslide deposit are evident in this image from NASA's 2001 Mars Odyssey of eastern Ius Chasma.
Dunes and the distal end of a landslide deposit are evident in this image from NASA's 2001 Mars Odyssey of eastern Ius Chasma.

Ius Chasma

The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the eastern flank of Olympus Mons.
The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the eastern flank of Olympus Mons.

Olympus Mons

The dunes shown in this image from NASA's 2001 Mars Odyssey are located on the floor of Hussey Crater in Terra Sirenum.
The dunes shown in this image from NASA's 2001 Mars Odyssey are located on the floor of Hussey Crater in Terra Sirenum.

Hussey Crater Dunes

On May 19th, 2005, NASA's Mars Exploration Rover Spirit captured this stunning view as the Sun sank below the rim of Gusev crater on Mars. This Panoramic Camera (Pancam) mosaic was taken around 6:07 in the evening of  the rover's 489th martian day.
On May 19th, 2005, NASA's Mars Exploration Rover Spirit captured this stunning view as the Sun sank below the rim of Gusev crater on Mars. This Panoramic Camera (Pancam) mosaic was taken around 6:07 in the evening of  the rover's 489th martian day.

A Moment Frozen in Time

This image from NASA's 2001 Mars Odyssey spacecraft had been targeted on the dunes on the floor of Charlier Crater. Unfortunately, clouds are obscuring the view of the surface.
This image from NASA's 2001 Mars Odyssey spacecraft had been targeted on the dunes on the floor of Charlier Crater. Unfortunately, clouds are obscuring the view of the surface.

Clouds over Charlier Crater

This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows small individual dunes on the floor of Moreux Crater.
This image, taken by NASA's 2001 Mars Odyssey spacecraft, shows small individual dunes on the floor of Moreux Crater.

Moreux Crater

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the complex caldera at the summit of Ascraeus Mons.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the complex caldera at the summit of Ascraeus Mons.

Ascraeus Mons

Many different surface textures are found on the polar caps. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the surface of the south polar cap.
Many different surface textures are found on the polar caps. This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the surface of the south polar cap.

South Pole

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the edge of the clouds in a weather front in the northern latitudes.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the edge of the clouds in a weather front in the northern latitudes.

Storm Front

Dark slope streaks mark the inner rim of this unnamed crater in Terra Sabaea, as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks mark the inner rim of this unnamed crater in Terra Sabaea, as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

We now begin a traverse across Mt. Sharp moving from east to west. The layering of the material that comprises Mt. Sharp is visible in the bottom third of this image from NASA's Mars Odyssey spacecraft; showing the weathering that has affected Mt. Sharp.
We now begin a traverse across Mt. Sharp moving from east to west. The layering of the material that comprises Mt. Sharp is visible in the bottom third of this image from NASA's Mars Odyssey spacecraft; showing the weathering that has affected Mt. Sharp.

Images of Gale #9

This image, made by the quadrupole mass spectrometer in the SAM suite of instruments in NASA's Curiosity Mars rover. shows the ratio of the argon isotope argon-36 to the heavier argon isotope argon-38, in various measurements.
This image, made by the quadrupole mass spectrometer in the SAM suite of instruments in NASA's Curiosity Mars rover. shows the ratio of the argon isotope argon-36 to the heavier argon isotope argon-38, in various measurements.

Argon Isotopes Provide Robust Signature of Atmospheric Loss

The frosted gullies in this observation from NASA's Mars Reconnaissance Orbiter are located along an irregularly shaped pit which lies within an impact crater in Sisyphi Planum ocated northwards of the Southern polar layered deposits.
The frosted gullies in this observation from NASA's Mars Reconnaissance Orbiter are located along an irregularly shaped pit which lies within an impact crater in Sisyphi Planum ocated northwards of the Southern polar layered deposits.

Frosted Gullies in a Central Pit

The linear graben in this image from NASA's 2001 Mars Odyssey spacecraft are all part of Claritas Fossae.
The linear graben in this image from NASA's 2001 Mars Odyssey spacecraft are all part of Claritas Fossae.

Claritas Fossae

The sinuous channel at the bottom of this image captured by NASA's 2001 Mars Odyssey spacecraft is called Anio Valles.
The sinuous channel at the bottom of this image captured by NASA's 2001 Mars Odyssey spacecraft is called Anio Valles.

Anio Valles

This image shows a small portion of the extensive lava flows created by the large Tharsis volcanoes as seen by NASA's 2001 Mars Odyssey spacecraft. These flows are located north east of Ascraeus Mons.
This image shows a small portion of the extensive lava flows created by the large Tharsis volcanoes as seen by NASA's 2001 Mars Odyssey spacecraft. These flows are located north east of Ascraeus Mons.

Tharsis Lava Flows

This graph shows about one-fourth of a Martian year's pattern atmospheric pressure at the surface of Mars, as measured by the Rover Environmental Monitoring Station on NASA's Curiosity rover.
This graph shows about one-fourth of a Martian year's pattern atmospheric pressure at the surface of Mars, as measured by the Rover Environmental Monitoring Station on NASA's Curiosity rover.

Seasonal Pressure Curve Peaks at Gale Crater

This image from NASA's 2001 Mars Odyssey spacecraft shows part of a dune field near the north polar cap. This is not Olympia Undae, the largest dune field near the north polar cap, but is rather a portion of a smaller dune field further to the east.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of a dune field near the north polar cap. This is not Olympia Undae, the largest dune field near the north polar cap, but is rather a portion of a smaller dune field further to the east.

Polar Dunes

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 captured by 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 captured by NASA's 2001 Mars Odyssey spacecraft shows part of Coprates Chasma.

Coprates Chasma - False Color

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