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This image from NASA's 2001 Mars Odyssey spacecraft shows a clear boundary between material being eroded by the wind (bottom of image) and a surface scoured clean (top of frame) northwest of Apollinaris Mons.
This image from NASA's 2001 Mars Odyssey spacecraft shows a clear boundary between material being eroded by the wind (bottom of image) and a surface scoured clean (top of frame) northwest of Apollinaris Mons.

Boundaries

Today's image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, which is comprised of lava flows from Arsia Mons. Note the small channel in the image. This channel was likely created by lava rather than water flow.
Today's image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Daedalia Planum, which is comprised of lava flows from Arsia Mons. Note the small channel in the image. This channel was likely created by lava rather than water flow.

Daedalia Planum

This image from NASA's Mars Reconnaissance Orbiter shows a graben (a trough formed when the ground drops between two parallel faults) and a lava flow in the Tharsis volcanic province of Mars. North is up.
This image from NASA's Mars Reconnaissance Orbiter shows a graben (a trough formed when the ground drops between two parallel faults) and a lava flow in the Tharsis volcanic province of Mars. North is up.

Graben Cutting Lava Flow in Tharsis

This image captured by NASA's 2001 Mars Odyssey shows a portion of the northeastern flank of Ascraeus Mons.
This image captured by NASA's 2001 Mars Odyssey shows a portion of the northeastern flank of Ascraeus Mons.

Ascraeus Mons

The amount of sand in this region of Juventae Chasma has coalesced into a sand sheet, rather than individual dune forms. Wind continues to sculpt the sand around high standing hills in this image from NASA's Mars Odyssey.
The amount of sand in this region of Juventae Chasma has coalesced into a sand sheet, rather than individual dune forms. Wind continues to sculpt the sand around high standing hills in this image from NASA's Mars Odyssey.

Juventae Chasma

This map shows the route driven by NASA's Curiosity Mars rover from the location where it landed in August 2012 to its location in early March 2016, approaching a geological waypoint called Naukluft Plateau.
This map shows the route driven by NASA's Curiosity Mars rover from the location where it landed in August 2012 to its location in early March 2016, approaching a geological waypoint called Naukluft Plateau.

New Waypoint, Science Team Newcomers for Curiosity

This image captured by NASA's 2001 Mars Odyssey spacecraft is located southwest of Olympus Mons, shows the end of a lava flow that has flowed between the hills at the upper left portion of the image.
This image captured by NASA's 2001 Mars Odyssey spacecraft is located southwest of Olympus Mons, shows the end of a lava flow that has flowed between the hills at the upper left portion of the image.

Lava End

This view of the lower front and underbelly areas of NASA's Mars rover Curiosity was taken by the rover's MAHLI camera during Sept. 9, 2012. Also visible are the hazard avoidance cameras on the front of the rover.
This view of the lower front and underbelly areas of NASA's Mars rover Curiosity was taken by the rover's MAHLI camera during Sept. 9, 2012. Also visible are the hazard avoidance cameras on the front of the rover.

Belly Check for Curiosity

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows Pyrrhae Chaos.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows Pyrrhae Chaos.

Pyrrhae Chaos - False Color

This image captured by NASA's Mars Reconnaissance Orbiter spacecraft shows what looks like drag folds, where rock layers bend (fold) before they break in a fault. The North Polar layered deposits are composed of ice.
This image captured by NASA's Mars Reconnaissance Orbiter spacecraft shows what looks like drag folds, where rock layers bend (fold) before they break in a fault. The North Polar layered deposits are composed of ice.

Drag Folds in the North Polar Layered Deposits

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of Ophir Chasma.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of Ophir Chasma.

Ophir Chasma - False Color

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Coprates Chasma.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Coprates Chasma.

Coprates Chasma - False Color

The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image captured by NASA's 2001 Mars Odyssey spacecraft shows Nili Patera.
The THEMIS camera contains 5 filters. The data from different filters can be combined in multiple ways to create a false color image. This image captured by NASA's 2001 Mars Odyssey spacecraft shows Nili Patera.

Nili Patera - False Color

The sinuous ridges in this image from NASA's Mars Reconnaissance Orbiter spacecraft display strong characteristics of ancient meandering riverbeds that are preserved as inverted topography.
The sinuous ridges in this image from NASA's Mars Reconnaissance Orbiter spacecraft display strong characteristics of ancient meandering riverbeds that are preserved as inverted topography.

Inverted Streams in the Aeolis Region

This image from NASA's Mars Reconnaissance Orbiter spacecraft is of a landing site that the flattest, safest place on Mars: part of Meridiani Planum, close to where the Opportunity rover landed.
This image from NASA's Mars Reconnaissance Orbiter spacecraft is of a landing site that the flattest, safest place on Mars: part of Meridiani Planum, close to where the Opportunity rover landed.

A Landing Site for ExoMars 2016

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 image from NASA's 2001 Mars Odyssey spacecraft shows part of Iani Chaos.
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 image from NASA's 2001 Mars Odyssey spacecraft shows part of Iani Chaos.

Iani Chaos - False Color

This image from NASA's Mars Reconnaissance Orbiter spacecraft nicely captures several influential geologic processes that have shaped the landscape of Lycus Sulci.
This image from NASA's Mars Reconnaissance Orbiter spacecraft nicely captures several influential geologic processes that have shaped the landscape of Lycus Sulci.

Ridge and Talus in Lycus Sulci

Tithonium Chasma is a part of Valles Marineris, the largest canyon in the Solar System. If Valles Marineris was located on Earth it would span across almost the entire United States. This observation is from NASA's Mars Reconnaissance Orbiter spacecraft.
Tithonium Chasma is a part of Valles Marineris, the largest canyon in the Solar System. If Valles Marineris was located on Earth it would span across almost the entire United States. This observation is from NASA's Mars Reconnaissance Orbiter spacecraft.

Light-Toned Layers in Tithonium Chasma

The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows a rim of material between two unnamed craters in Tyrrhena Terra.
The THEMIS VIS camera contains 5 filters. Data from different filters can be combined in many ways to create a false color image. This image from NASA's 2001 Mars Odyssey spacecraft shows a rim of material between two unnamed craters in Tyrrhena Terra.

Tyrrhena Terra - False Color

This image, acquired by NASA's Mars Reconnaissance Orbiter, shows there are a few more fans on the ridge as spring activity progresses in Inca City.
This image, acquired by NASA's Mars Reconnaissance Orbiter, shows there are a few more fans on the ridge as spring activity progresses in Inca City.

Spring in Inca City III

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Labou Vallis.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Labou Vallis.

Labou Vallis

This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering in the plains that comprise Utopia Planitia.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows layering in the plains that comprise Utopia Planitia.

Plains Layers

Moving further east, we see more dunes. This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the crater rim and the crater floor seen in the image is not as smooth as in other parts of the crater.
Moving further east, we see more dunes. This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the crater rim and the crater floor seen in the image is not as smooth as in other parts of the crater.

Images of Gale #7

This image from NASA's Mars Odyssey spacecraft shows the northern part of Mt. Sharp and the crater floor between Mt. Sharp and the northern rim of Gale Crater. The layering of Mt. Sharp is visible at the bottom of the image.
This image from NASA's Mars Odyssey spacecraft shows the northern part of Mt. Sharp and the crater floor between Mt. Sharp and the northern rim of Gale Crater. The layering of Mt. Sharp is visible at the bottom of the image.

Images of Gale #4

Dark slope steaks mark the ridges of this region in Lycus Sulci in this image from NASA's 2001 Mars Odyssey spacecraft.
Dark slope steaks mark the ridges of this region in Lycus Sulci in this image from NASA's 2001 Mars Odyssey spacecraft.

Lycus Sulci

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