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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

This is a version of one of the first images taken by a front Hazard-Avoidance camera on NASA's Curiosity rover. It was taken through a
This is a version of one of the first images taken by a front Hazard-Avoidance camera on NASA's Curiosity rover. It was taken through a

Curiosity's Front View, Linearized

The two depression crossing this image are called Pavonis Fossae and are located just north of the volcano in this image captured by NASA's 2001 Mars Odyssey spacecraft.
The two depression crossing this image are called Pavonis Fossae and are located just north of the volcano in this image captured by NASA's 2001 Mars Odyssey spacecraft.

Pavonis Fossae

Thick stacks of clay minerals indicate chemical alteration of thick stacks of rock by interaction with liquid water on ancient Mars as seen in this image from NASA's Mars Reconnaissance Orbiter.
Thick stacks of clay minerals indicate chemical alteration of thick stacks of rock by interaction with liquid water on ancient Mars as seen in this image from NASA's Mars Reconnaissance Orbiter.

Chemical Alteration by Water, Mawrth Vallis

Dark slope streaks are visible in this image of Amazonis Planitia captured by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks are visible in this image of Amazonis Planitia captured by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

The dunes in this image captured by NASA's Mars Odyssey are located on the floor of Kaiser Crater.
The dunes in this image captured by NASA's Mars Odyssey are located on the floor of Kaiser Crater.

Kaiser Crater Dunes

This image from NASA's Mars Odyssey shows dark slope streaks, a common feature on the rim of this unnamed crater within Tikhonravov Crater.
This image from NASA's Mars Odyssey shows dark slope streaks, a common feature on the rim of this unnamed crater within Tikhonravov Crater.

Dark Slope Streaks within Tikhonravov Crater

NASA's Mars Exploration Rover Opportunity used the wire brush of its rock abrasion tool to scour dust from a circular target area on a rock called 'Marquette Island.'
NASA's Mars Exploration Rover Opportunity used the wire brush of its rock abrasion tool to scour dust from a circular target area on a rock called 'Marquette Island.'

Examining 'Marquette Island'

The windstreak in this image from NASA's 2001 Mars Odyssey spacecraft is located on Tharsis volcanic lava flows east of Olympus Mons.
The windstreak in this image from NASA's 2001 Mars Odyssey spacecraft is located on Tharsis volcanic lava flows east of Olympus Mons.

Windstreak

The unusual and apparently layered surface in this image from NASA's 2001 Mars Odyssey spacecraft is located in Aureum Chaos.
The unusual and apparently layered surface in this image from NASA's 2001 Mars Odyssey spacecraft is located in Aureum Chaos.

Aureum Chaos

Small channels dissect the inner rim of this unnamed crater in Arabia Terra as seen by NASA's 2001 Mars Odyssey spacecraft.
Small channels dissect the inner rim of this unnamed crater in Arabia Terra as seen by NASA's 2001 Mars Odyssey spacecraft.

Channels

This image captured by NASA's 2001 Mars Odyssey spacecraft shows the complexity of wind erosion on Mars. The erosion of the hills and the gouge-like pits indicate two, if not three wind directions that all altered the surface.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows the complexity of wind erosion on Mars. The erosion of the hills and the gouge-like pits indicate two, if not three wind directions that all altered the surface.

Wind Erosion

Craters are most often the site of gully formation on Mars. Mega-gullies are also found on the southwestern parts of Vallis Marineris, and in this image from NASA's 2001 Mars Odyssey spacecraft, on hills east of Argyre Planitia.
Craters are most often the site of gully formation on Mars. Mega-gullies are also found on the southwestern parts of Vallis Marineris, and in this image from NASA's 2001 Mars Odyssey spacecraft, on hills east of Argyre Planitia.

Gullies

This image taken by NASA's Mars Reconnaissance Orbiter covers part of a candidate landing site that appears to be a shallow depression with a deposit perhaps consisting of chlorides, like table salt.
This image taken by NASA's Mars Reconnaissance Orbiter covers part of a candidate landing site that appears to be a shallow depression with a deposit perhaps consisting of chlorides, like table salt.

Candidate Landing Site in Possible Salt Playa

The Kasei Valles region is very complex. This image captured by NASA's Mars Odyssey illustrates that complexity with features created by fluvial action (channels) and tectonic processes (fractures).
The Kasei Valles region is very complex. This image captured by NASA's Mars Odyssey illustrates that complexity with features created by fluvial action (channels) and tectonic processes (fractures).

Kasei Valles

This map shows the route driven and route planned for NASA's Curiosity Mars rover from before reaching 'Dingo Gap' in upper right, to the mission's next science waypoint, 'Kimberley' (formerly referred to as 'KMS-9'), lower left.
This map shows the route driven and route planned for NASA's Curiosity Mars rover from before reaching 'Dingo Gap' in upper right, to the mission's next science waypoint, 'Kimberley' (formerly referred to as 'KMS-9'), lower left.

Map of Recent and Planned Driving by Curiosity as of Feb. 18, 2014

Constant sand-blasting by the winds on Mars have eroded and sculpted the surface in the equatorial region around Medusae Fossae in this image captured by NASA's Mars Odyssey.
Constant sand-blasting by the winds on Mars have eroded and sculpted the surface in the equatorial region around Medusae Fossae in this image captured by NASA's Mars Odyssey.

Wind Erosion

Dark slope streaks are found throughout Lycus Sulci in this image taken by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks are found throughout Lycus Sulci in this image taken by NASA's 2001 Mars Odyssey spacecraft.

Lycus Sulci

The channels in this image from NASA's 2001 Mars Odyssey spacecraft are dissecting the northwestern flank of Alba Mons.
The channels in this image from NASA's 2001 Mars Odyssey spacecraft are dissecting the northwestern flank of Alba Mons.

Channels

The sand sheet and dunes in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are located on the floor of Juventae Chasma.
The sand sheet and dunes in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are located on the floor of Juventae Chasma.

Juventae Chasma

Layers of rock in the upper portion of a tall mound near the center of Gale Crater on Mars exhibit a regular thickness of several meters in this image taken by NASA's Mars Reconnaissance Orbiter.
Layers of rock in the upper portion of a tall mound near the center of Gale Crater on Mars exhibit a regular thickness of several meters in this image taken by NASA's Mars Reconnaissance Orbiter.

Layers in Upper Formation of Gale Crater Mound

Sand dunes such as those seen in this image from NASA's Mars Reconnaissance Orbiter have been observed to creep slowly across the surface of Mars through the action of the wind.
Sand dunes such as those seen in this image from NASA's Mars Reconnaissance Orbiter have been observed to creep slowly across the surface of Mars through the action of the wind.

Dunes on the Rim of the Hellas Impact Basin

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? The connected craters at the top and bottom of this image look like bugs, perhaps a bumble bee at the top and a wasp at the bottom.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? The connected craters at the top and bottom of this image look like bugs, perhaps a bumble bee at the top and a wasp at the bottom.

THEMIS Art #101

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