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This image from NASA's Mars Odyssey spacecraft shows dark material at the bottom of the image, likely deposited by the large channel. It shows how close that material is to Mt. Sharp and how different the two deposits appear in a visible wavelength image.
This image from NASA's Mars Odyssey spacecraft shows dark material at the bottom of the image, likely deposited by the large channel. It shows how close that material is to Mt. Sharp and how different the two deposits appear in a visible wavelength image.

Images of Gale #24

This oblique, southward-looking view of Gale crater shows the mound of layered rocks that NASA's Mars Science Laboratory will investigate. The mission's selected landing site is just north of the mound inside the crater.
This oblique, southward-looking view of Gale crater shows the mound of layered rocks that NASA's Mars Science Laboratory will investigate. The mission's selected landing site is just north of the mound inside the crater.

Context of Curiosity Landing Site in Gale Crater

This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft northwest of the crater. NASA has selected Gale as the landing site for the Mars Science Laboratory mission.
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft northwest of the crater. NASA has selected Gale as the landing site for the Mars Science Laboratory mission.

Oblique view of Gale Crater from the Northwest

This image of the floor of Proctor Crater, taken by NASA's 2001 Mars Odyssey spacecraft, shows part of the sand sheet and dune forms that are located there.
This image of the floor of Proctor Crater, taken by NASA's 2001 Mars Odyssey spacecraft, shows part of the sand sheet and dune forms that are located there.

Proctor Crater Dunes

NASA's Mars rover Curiosity has delivered sample portions of rock powder collected from the interior of a rock on Mars into laboratory instruments inside the rover.
NASA's Mars rover Curiosity has delivered sample portions of rock powder collected from the interior of a rock on Mars into laboratory instruments inside the rover.

Check-up Image After Delivering Martian Rock Powder

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the western margin of Ophir Chasma. Layering can be seen in the upper walls of the canyon.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the western margin of Ophir Chasma. Layering can be seen in the upper walls of the canyon.

Ophir Chasma

The bright features in this image captured by NASA's Mars Odyssey are the tops of clouds north of Alba Mons.
The bright features in this image captured by NASA's Mars Odyssey are the tops of clouds north of Alba Mons.

Storm Clouds

There is a large deposit of material on the floor of Nicholson Crater, as seen in this image from NASA's 2001 Mars Odyssey spacecraft. This pile of material appears to be undergoing erosion by the wind.
There is a large deposit of material on the floor of Nicholson Crater, as seen in this image from NASA's 2001 Mars Odyssey spacecraft. This pile of material appears to be undergoing erosion by the wind.

Nicholson Crater

The cliff face in this image from NASA's 2001 Mars Odyssey spacecraft was created by tectonic activity and is located in a region of Tempe Terra that is complexly fractured.
The cliff face in this image from NASA's 2001 Mars Odyssey spacecraft was created by tectonic activity and is located in a region of Tempe Terra that is complexly fractured.

Tempe Fossae

This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Tithonium Chasma, part of the western side of Valles Marineris.
This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Tithonium Chasma, part of the western side of Valles Marineris.

Tithonium Chasma

This image captured by NASA's Mars Odyssey shows a portion of Coprates Chasma.
This image captured by NASA's Mars Odyssey shows a portion of Coprates Chasma.

Coprates Chasma

The hills and ridges at the top of this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Nilus Mensae, which is part of the complex Kasei Valles channels.
The hills and ridges at the top of this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Nilus Mensae, which is part of the complex Kasei Valles channels.

Nilus Mensae

This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae. Compare this to previous images and notice how uniform the dunes are in this region.
This image captured by NASA's 2001 Mars Odyssey spacecraft is part of Olympia Undae. Compare this to previous images and notice how uniform the dunes are in this region.

Olympia Undae

This image from NASA's Mar Reconnaissance Orbiter combines a photograph of seasonal dark flows on a Martian slope at Palikir Crater with a grid of colors based on data collected by a mineral-mapping spectrometer observing the same area.
This image from NASA's Mar Reconnaissance Orbiter combines a photograph of seasonal dark flows on a Martian slope at Palikir Crater with a grid of colors based on data collected by a mineral-mapping spectrometer observing the same area.

Color-Coded Clues to Composition Superimposed on Martian Seasonal-Flow Image

NASA's 2001 Mars Odyssey spacecraft captured this image of dunes on the floor of an unnamed crater in Tyrrhena Terra.
NASA's 2001 Mars Odyssey spacecraft captured this image of dunes on the floor of an unnamed crater in Tyrrhena Terra.

Dunes in Tyrrhena Terra

The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft originated at Pavonis Mons.
The lava flows in this image captured by NASA's 2001 Mars Odyssey spacecraft originated at Pavonis Mons.

Pavonis Mons

This image, taken Jan. 26, 2012, shows NASA's no-longer-active Phoenix Mars Lander spacecraft after its second Martian arctic winter.
This image, taken Jan. 26, 2012, shows NASA's no-longer-active Phoenix Mars Lander spacecraft after its second Martian arctic winter.

Phoenix Lander After Second Martian Winter

This image from NASA's Mars Odyssey shows part of the floor of Ganges Chasma. Deposits of fine surface materials and bright layered deposits are visible in this image.
This image from NASA's Mars Odyssey shows part of the floor of Ganges Chasma. Deposits of fine surface materials and bright layered deposits are visible in this image.

Ganges Chasma

Spring time brings storms to the north polar region of Mars. This image captured by NASA's 2001 Mars Odyssey spacecraft shows a storm front, as bright clouds shadow and obscure the surface.
Spring time brings storms to the north polar region of Mars. This image captured by NASA's 2001 Mars Odyssey spacecraft shows a storm front, as bright clouds shadow and obscure the surface.

Storm Front

A branch of Nanedi Valles entered a crater and deposited a delta that fills the majority of the crater floor. This image was captured by NASA's Mars Odyssey.
A branch of Nanedi Valles entered a crater and deposited a delta that fills the majority of the crater floor. This image was captured by NASA's Mars Odyssey.

Nanedi Valles

Taken by NASA's 2001 Mars Odyssey spacecraft, this image shows a fan shaped deposit located on the floor of Holden Crater.
Taken by NASA's 2001 Mars Odyssey spacecraft, this image shows a fan shaped deposit located on the floor of Holden Crater.

Holden Crater Fan

This image from a movie clip shows Phobos, the larger of the two moons of Mars, passing in front of the other Martian moon, Deimos, on Aug. 1, from the perspective of NASA's Mars rover Curiosity.
This image from a movie clip shows Phobos, the larger of the two moons of Mars, passing in front of the other Martian moon, Deimos, on Aug. 1, from the perspective of NASA's Mars rover Curiosity.

Smoothed Movie of Phobos Passing Deimos in Martian Sky

Dark streaks mark the slope of this crater rim south of Tikhonravov Crater in this image captured by NASA's Mars Odyssey.
Dark streaks mark the slope of this crater rim south of Tikhonravov Crater in this image captured by NASA's Mars Odyssey.

Dark Slope Streaks

Parts of Meridiani Planum have a surface that appears to be composed of different layers of material. In this image taken by NASA's Mars Odyssey the contrast of bright and dark materials indicates the different layers.
Parts of Meridiani Planum have a surface that appears to be composed of different layers of material. In this image taken by NASA's Mars Odyssey the contrast of bright and dark materials indicates the different layers.

Meridiani Planum

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

Olympus Mons

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