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NASA's Mars rover Curiosity drove 6.2 feet (1.9 meters) during the 100th Martian day, or sol, of the mission (Nov. 16, 2012). The view spans from north at the left to south-southeast at the right. It is presented in a cylindrical projection.
NASA's Mars rover Curiosity drove 6.2 feet (1.9 meters) during the 100th Martian day, or sol, of the mission (Nov. 16, 2012). The view spans from north at the left to south-southeast at the right. It is presented in a cylindrical projection.

Curiosity's Eastward View After Sol 100 Drive

The wide channel in this image captured by NASA's Mars Odyssey is Tinto Vallis.
The wide channel in this image captured by NASA's Mars Odyssey is Tinto Vallis.

Tinto Vallis

This image captured by NASA's 2001 Mars Odyssey shows a small portion of the large fracture called Cerberus Fossae.
This image captured by NASA's 2001 Mars Odyssey shows a small portion of the large fracture called Cerberus Fossae.

Cerberus Fossae

This image from NASA's Curiosity rover shows the great diversity of grains found on the surface of a Martian rock.
This image from NASA's Curiosity rover shows the great diversity of grains found on the surface of a Martian rock.

Texture of 'Gillespie Lake' Rock

Dunes cover the floor of this unnamed crater in the northern lowlands in this image captured by NASA's Mars Odyssey.
Dunes cover the floor of this unnamed crater in the northern lowlands in this image captured by NASA's Mars Odyssey.

Northern Dunes

This image taken by NASA's 2001 Mars Odyssey shows secondary channeling on a terrace of the huge Kasei Valles outflow system.
This image taken by NASA's 2001 Mars Odyssey shows secondary channeling on a terrace of the huge Kasei Valles outflow system.

Kasei Valles

This image from NASA's Mars Odyssey shows the southeast flank of Olympus Mons. This huge volcano is surrounded by an escarpment, a large cliff at the volcano margin; a landslide lies alongside the escarpment.
This image from NASA's Mars Odyssey shows the southeast flank of Olympus Mons. This huge volcano is surrounded by an escarpment, a large cliff at the volcano margin; a landslide lies alongside the escarpment.

Olympus Mons

The depressions in this image from NASA's Mars Odyssey likely formed due to both volcanic and tectonic forces. Tectonic forces likely account for some of the depressions, while collapse into lava tubes and lava flow erosion account for the remainder.
The depressions in this image from NASA's Mars Odyssey likely formed due to both volcanic and tectonic forces. Tectonic forces likely account for some of the depressions, while collapse into lava tubes and lava flow erosion account for the remainder.

Collapse Features

The sand dunes in this image are part of Olympia Undae, a huge sand sea located near the north polar cap as seen by NASA's 2001 Mars Odyssey spacecraft.
The sand dunes in this image are part of Olympia Undae, a huge sand sea located near the north polar cap as seen by NASA's 2001 Mars Odyssey spacecraft.

Olympia Undae

This image shows a portion of Samara Valles as seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows a portion of Samara Valles as seen by NASA's 2001 Mars Odyssey spacecraft.

Samara Valles

The linear ridges in this image captured by NASA's 2001 Mars Odyssey spacecraft are located near the south polar cap.
The linear ridges in this image captured by NASA's 2001 Mars Odyssey spacecraft are located near the south polar cap.

Linear Ridges

With the changing of seasons comes changes in weather. This image from NASA's 2001 Mars Odyssey spacecraft shows clouds in the north polar region. The surface is just barely visible in part of the image.
With the changing of seasons comes changes in weather. This image from NASA's 2001 Mars Odyssey spacecraft shows clouds in the north polar region. The surface is just barely visible in part of the image.

Polar Clouds

One type of feature of scientific interest on the mountain inside Gale crater is exposure of cemented fractures, evidence that groundwater once reached to at least that height of the mountain. This image is from NASA's Mars Reconnaissance Orbiter.
One type of feature of scientific interest on the mountain inside Gale crater is exposure of cemented fractures, evidence that groundwater once reached to at least that height of the mountain. This image is from NASA's Mars Reconnaissance Orbiter.

Cemented Fractures in Mountain Inside Gale Crater on Mars

Channels are dissecting the flank of Apollinaris Mons in this image from NASA's 2001 Mars Odyssey spacecraft.
Channels are dissecting the flank of Apollinaris Mons in this image from NASA's 2001 Mars Odyssey spacecraft.

Apollineris Mons

This image of an area south of Olympus Mons shows a region where the wind has been an active agent in modifying the surface. Small linear dunes cover the surface in this image taken by NASA's 2001 Mars Odyssey spacecraft.
This image of an area south of Olympus Mons shows a region where the wind has been an active agent in modifying the surface. Small linear dunes cover the surface in this image taken by NASA's 2001 Mars Odyssey spacecraft.

Wind Power

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 sand sheet with surface dune forms in an unnamed crater.
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 sand sheet with surface dune forms in an unnamed crater.

Noachis Terra Dunes - False Color

This April 16, 2015, panorama from the Mast Camera on NASA's Curiosity Mars rover shows a detailed view toward two areas, 'Mount Shields' and 'Logan Pass,' on lower Mount Sharp, chosen for close-up inspection in subsequent weeks.
This April 16, 2015, panorama from the Mast Camera on NASA's Curiosity Mars rover shows a detailed view toward two areas, 'Mount Shields' and 'Logan Pass,' on lower Mount Sharp, chosen for close-up inspection in subsequent weeks.

Looking Toward Curiosity Study Areas, Spring 2015

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 an unnamed crater in Tyrrhena Terra.
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 an unnamed crater in Tyrrhena Terra.

Tyrrhena Terra - False Color

The dark lobed material in this image from NASA's 2001 Mars Odyssey spacecraft is a lava flow located northwest of the Elysium Volcanic Complex.
The dark lobed material in this image from NASA's 2001 Mars Odyssey spacecraft is a lava flow located northwest of the Elysium Volcanic Complex.

Lava Channel

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

Ascraeus Mons

Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? The dark dune deposit resembles a howling animal.
Do you see what I see in this image captured by NASA's 2001 Mars Odyssey spacecraft? The dark dune deposit resembles a howling animal.

THEMIS Art #99

This image from NASA's Curiosity rover shows the cover on an inlet that will receive powdered rock and soil samples for analysis. The image also shows sand and angular and rounded pebbles that were deposited on the rover deck when it landed.
This image from NASA's Curiosity rover shows the cover on an inlet that will receive powdered rock and soil samples for analysis. The image also shows sand and angular and rounded pebbles that were deposited on the rover deck when it landed.

Getting Ready for Sampling on Mars

A small section of Dao Vallis in shown in this image from NASA's 2001 Mars Odyssey spacecraft. Dao Vallis is a major channel that drains into Hellas Planitia.
A small section of Dao Vallis in shown in this image from NASA's 2001 Mars Odyssey spacecraft. Dao Vallis is a major channel that drains into Hellas Planitia.

Dao Valles

Extensive lava flows originating from Arsia Mons created Daedalia Planum. This image is from NASA's 2001 Mars Odyssey spacecraft.
Extensive lava flows originating from Arsia Mons created Daedalia Planum. This image is from NASA's 2001 Mars Odyssey spacecraft.

Daedalia Planum

The THEMIS VIS camera contains 5 filters. The data from different filters can create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Schaeberle Crater, including small dunes.
The THEMIS VIS camera contains 5 filters. The data from different filters can create a false color image. This false color image from NASA's 2001 Mars Odyssey spacecraft shows part of the floor of Schaeberle Crater, including small dunes.

Schaeberle Crater - False Color

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