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These two images come from the HiRISE camera on NASA's Mars Reconnaissance Orbiter. Images of locations in Gale Crater taken from orbit around Mars reveal evidence of erosion in recent geological times and development of small scarps, or vertical surfaces
These two images come from the HiRISE camera on NASA's Mars Reconnaissance Orbiter. Images of locations in Gale Crater taken from orbit around Mars reveal evidence of erosion in recent geological times and development of small scarps, or vertical surfaces

Erosion Patterns May Guide Mars Rover to Rocks Recently Exposed

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

Daedalia Planum

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

Proctor Crater Dunes

This colorful scene is situated in the Noctis Labyrinthus, perched high on the Tharsis rise in the upper reaches of the Valles Marineris canyon system as seen by NASA's Mars Reconnaissance Orbiter.
This colorful scene is situated in the Noctis Labyrinthus, perched high on the Tharsis rise in the upper reaches of the Valles Marineris canyon system as seen by NASA's Mars Reconnaissance Orbiter.

Two Generations of Windblown Sediments

Dark slope streaks are common throughout the ridges that comprise Lycus Sulci in this image captured by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks are common throughout the ridges that comprise Lycus Sulci in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Lycus Sulci

This image from NASA's 2001 Mars Odyssey spacecraft is of Lycus Sulci, located on the western side of Olympus Mons and dominated by multi-direction ridges which contains material less resistant than the ridges to the effects of wind.
This image from NASA's 2001 Mars Odyssey spacecraft is of Lycus Sulci, located on the western side of Olympus Mons and dominated by multi-direction ridges which contains material less resistant than the ridges to the effects of wind.

Lycus Sulci

Huge gullies, like these captured by NASA's 2001 Mars Odyssey, line both rims of Ius Chasma.
Huge gullies, like these captured by NASA's 2001 Mars Odyssey, line both rims of Ius Chasma.

Gullies in Ius Chasma

Windstreaks are a common feature on the surface of Daedalia Planum volcanic flows. This image was captured by NASA's Mars Odyssey.
Windstreaks are a common feature on the surface of Daedalia Planum volcanic flows. This image was captured by NASA's Mars Odyssey.

Windstreaks

This stereo mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 93.3-meter (306-foot) drive east-northeastward on Oct. 6, 2010. 3D glasses are necessary to view this image.
This stereo mosaic of images from NASA's Mars Exploration Rover Opportunity shows surroundings of the rover's location following an 93.3-meter (306-foot) drive east-northeastward on Oct. 6, 2010. 3D glasses are necessary to view this image.

Opportunity's Eastward View After Sol 2382 Drive (Stereo)

These dark dunes captured by NASA's 2001 Mars Odyssey are located on the floor of Danielson Crater in Meridiani Planum.
These dark dunes captured by NASA's 2001 Mars Odyssey are located on the floor of Danielson Crater in Meridiani Planum.

Danielson Crater Dunes

NASA's Mars Exploration Rover Opportunity has found a rock that apparently is another meteorite, less than three weeks after driving away from a larger meteorite that the rover examined for six weeks.
NASA's Mars Exploration Rover Opportunity has found a rock that apparently is another meteorite, less than three weeks after driving away from a larger meteorite that the rover examined for six weeks.

Opportunity Finds Another Meteorite

The Compact Reconnaissance Imaging Spectrometer for Mars, an instrument on NASA's Mars Reconnaissance Orbiter, obtained information confirming material excavated by a fresh impact and Identified as water ice.
The Compact Reconnaissance Imaging Spectrometer for Mars, an instrument on NASA's Mars Reconnaissance Orbiter, obtained information confirming material excavated by a fresh impact and Identified as water ice.

Material Excavated by a Fresh Impact and Identified as Water Ice

This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles), as observed by NASA's Mars Reconnaissance Orbiter.
This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles), as observed by NASA's Mars Reconnaissance Orbiter.

Pitted Landforms in Southern Hellas Planitia

Several terrain types converge in this scene observed by NASA's Mars Reconnaissance Orbiter from Arsinoes Chaos, in the far eastern portions of Valles Marineris.
Several terrain types converge in this scene observed by NASA's Mars Reconnaissance Orbiter from Arsinoes Chaos, in the far eastern portions of Valles Marineris.

Yardangs in Arsinoes Chaos, Mars

In this observation from NASA's Mars Reconnaissance Orbiter made for a study of ancient craters, we see the craters filled with smooth material that has subsequently degraded into scallops. These formations might be possibly due to ground ice sublimation.
In this observation from NASA's Mars Reconnaissance Orbiter made for a study of ancient craters, we see the craters filled with smooth material that has subsequently degraded into scallops. These formations might be possibly due to ground ice sublimation.

Filled Crater and Scallops

This image from NASA's Mars Reconnaissance Orbiter shows several seemingly active gullies and their associated fans near the Argyre region.
This image from NASA's Mars Reconnaissance Orbiter shows several seemingly active gullies and their associated fans near the Argyre region.

Gullies Old and New Near the Argyre Region

This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.
This region of linear, intersecting ridges near the south pole is called Angustus Labyrinthus, as shown in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Angustus Labyrinthus

This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Aspledon Undae, a region of dunes near the north pole. The right side of the image shows hundreds of small, isolated dunes.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of Aspledon Undae, a region of dunes near the north pole. The right side of the image shows hundreds of small, isolated dunes.

Aspledon Undae

This image NASA's Mars Reconnaissance Orbitershows a prominently stratified transect through the rock of a mountain of material in the middle of Hebes Chasma.
This image NASA's Mars Reconnaissance Orbitershows a prominently stratified transect through the rock of a mountain of material in the middle of Hebes Chasma.

A Revealing Landslide in Hebes Chasma

This complex graben is part of Labeatis Fossae. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
This complex graben is part of Labeatis Fossae. This image was captured by NASA's 2001 Mars Odyssey spacecraft.

Labeatis Fossae

This image captured by NASA's 2001 Mars Odyssey spacecraf shows a portion of Patapsco Vallis, located on the eastern margin of the Elysium volcanic complex.
This image captured by NASA's 2001 Mars Odyssey spacecraf shows a portion of Patapsco Vallis, located on the eastern margin of the Elysium volcanic complex.

Patapsco Vallis

Numerous channels dissect the rim of this large crater located on Acheron Fossae as seen by NASA's 2001 Mars Odyssey spacecraft.
Numerous channels dissect the rim of this large crater located on Acheron Fossae as seen by NASA's 2001 Mars Odyssey spacecraft.

Crater Rim Channels

This image from NASA's 2001 Mars Odyssey shows the central portion of the complex caldera at the summit of Olympus Mons.
This image from NASA's 2001 Mars Odyssey shows the central portion of the complex caldera at the summit of Olympus Mons.

Olympus Mons Summit

This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large deposit on the floor of Nicholson Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the large deposit on the floor of Nicholson Crater.

Nicholson Crater

This image from NASA's 2001 Mars Odyssey spacecraf shows part of the southern flank of Ascraeus Mons. Large collapse features are common in this area.
This image from NASA's 2001 Mars Odyssey spacecraf shows part of the southern flank of Ascraeus Mons. Large collapse features are common in this area.

Ascraeus Mons Collapse Pits

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