2460 images found for "Mars" Wallpaper
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This image from NASA's Mars Odyssey shows part of the summit caldera of Pavonis Mons, the middle of three Tharsis volcanos that form a line southeast of Olympus Mons and northwest of Vallis Marineris.
This image from NASA's Mars Odyssey shows part of the summit caldera of Pavonis Mons, the middle of three Tharsis volcanos that form a line southeast of Olympus Mons and northwest of Vallis Marineris.

Pavonis Mons Summit Caldera

Coprates Chasma comprises the central portion of the Valles Marineris canyon system complex. This image from NASA's Mars Odyssey spacecraft of the southern wall of Coprates Chasma contains a landslide deposit with dunes over portions of slide.
Coprates Chasma comprises the central portion of the Valles Marineris canyon system complex. This image from NASA's Mars Odyssey spacecraft of the southern wall of Coprates Chasma contains a landslide deposit with dunes over portions of slide.

Coprates Chasma Landslide

Reull Vallis, located in Mars' cratered southern hemisphere, flows for over 1,000 km (about 620 miles) toward the Hellas basin. This NASA Mars Odyssey image shows a portion of the channel with its enigmatic lineated floor deposits.
Reull Vallis, located in Mars' cratered southern hemisphere, flows for over 1,000 km (about 620 miles) toward the Hellas basin. This NASA Mars Odyssey image shows a portion of the channel with its enigmatic lineated floor deposits.

Reull Vallis

This NASA Mars Odyssey image captures a portion of several lava flows in Daedalia Planum southwest of the Arsia Mons shield volcano. Textures characteristic of the variable surface roughness associated with different lava flows in this region are easily s
This NASA Mars Odyssey image captures a portion of several lava flows in Daedalia Planum southwest of the Arsia Mons shield volcano. Textures characteristic of the variable surface roughness associated with different lava flows in this region are easily s

Lava Flows of Daedalia Planum

This image from NASA's Mars Odyssey is located near the equator and the prime meridian of Mars in a region called Terra Meridiani. This is a unique area of Mars that displays layers of material that appear to be in the process of being stripped away.
This image from NASA's Mars Odyssey is located near the equator and the prime meridian of Mars in a region called Terra Meridiani. This is a unique area of Mars that displays layers of material that appear to be in the process of being stripped away.

Terra Meridiani

Like drippings from a candle, these lava flows on the flank of Olympus Mons volcano, seen in this image from NASA's Mars Odyssey spacecraft, demonstrate how it became the largest volcano in the solar system.
Like drippings from a candle, these lava flows on the flank of Olympus Mons volcano, seen in this image from NASA's Mars Odyssey spacecraft, demonstrate how it became the largest volcano in the solar system.

Olympus Mons Flows

This image from NASA's Mars Odyssey shows deposits in a crater located in Arabia Terra. Arabia is generally dust covered and dark streaks or dust avalanches are present in the crater walls.
This image from NASA's Mars Odyssey shows deposits in a crater located in Arabia Terra. Arabia is generally dust covered and dark streaks or dust avalanches are present in the crater walls.

Arabia Terra

This NASA Mars Odyssey image shows parts of the dissected and eroded remnants of an impact crater rim and volcanic material located north of Apollinaris Patera near the southern highlands - northern lowlands dichotomy on Mars.
This NASA Mars Odyssey image shows parts of the dissected and eroded remnants of an impact crater rim and volcanic material located north of Apollinaris Patera near the southern highlands - northern lowlands dichotomy on Mars.

Appollinaris Patera

Located in Arabia Terra, the crater shown in this image from NASA's Mars Odyssey spacecraft is known as Henry Crater. Like many other craters on Mars, the interior of Henry Crater is filled with a layered deposit.
Located in Arabia Terra, the crater shown in this image from NASA's Mars Odyssey spacecraft is known as Henry Crater. Like many other craters on Mars, the interior of Henry Crater is filled with a layered deposit.

Henry Crater

The Cydonia region on Mars, seen in this image from NASA's Mars Odyssey spacecraft, straddles the boundary between the bright, dusty, cratered highlands to the southeast and the dark, relatively dust-free, lowland plains to the west.
The Cydonia region on Mars, seen in this image from NASA's Mars Odyssey spacecraft, straddles the boundary between the bright, dusty, cratered highlands to the southeast and the dark, relatively dust-free, lowland plains to the west.

Cydonia Landscape

This NASA Mars Odyssey image was taken during winter in the southern hemisphere, meaning that the usually cloudy Hellas Basin is relatively free from clouds.
This NASA Mars Odyssey image was taken during winter in the southern hemisphere, meaning that the usually cloudy Hellas Basin is relatively free from clouds.

Winter in Hellas Basin

This scene from NASA's Mars Odyssey spacecraft shows several interesting geologic features associated with impact craters on Mars.
This scene from NASA's Mars Odyssey spacecraft shows several interesting geologic features associated with impact craters on Mars.

Impact Crater

This image from NASA's Mars Odyssey shows the cratered highlands of Terra Cimmeria. The image contains several long troughs of Sirenum Fossae running primarily from left to right. These features are parallel to semi-parallel fractures called graben.
This image from NASA's Mars Odyssey shows the cratered highlands of Terra Cimmeria. The image contains several long troughs of Sirenum Fossae running primarily from left to right. These features are parallel to semi-parallel fractures called graben.

Terra Cimmeria Highlands

This image from NASA's Mars Odyssey is of a region of Mars called Tempe Terra, which is located between the topographically high Tharsis Region and Acidalia Planitia, a large low albedo region of in the Martian northern hemisphere.
This image from NASA's Mars Odyssey is of a region of Mars called Tempe Terra, which is located between the topographically high Tharsis Region and Acidalia Planitia, a large low albedo region of in the Martian northern hemisphere.

Tempe Terra

With a diameter of roughly 2,000 km (1,243 miles) and a depth of over 7 km (more than 4 miles), the Hellas Basin, shown in this image from NASA's Mars Odyssey spacecraft, is the largest impact feature on Mars.
With a diameter of roughly 2,000 km (1,243 miles) and a depth of over 7 km (more than 4 miles), the Hellas Basin, shown in this image from NASA's Mars Odyssey spacecraft, is the largest impact feature on Mars.

Floor of Hellas Basin

This image from NASA's Mars Odyssey spacecraft covers part of Tithonium Chasma, which is part of the Valles Marineris system of canyons that stretch for thousands of kilometers.
This image from NASA's Mars Odyssey spacecraft covers part of Tithonium Chasma, which is part of the Valles Marineris system of canyons that stretch for thousands of kilometers.

Tithonium Chasma

An isolated mesa east of the Phlegra Montes in northeastern Elysium Planitia has a cracked surface that, combined with its overall shape, gives the appearance of a giant loaf of bread in this image from NASA's Mars Odyssey spacecraft.
An isolated mesa east of the Phlegra Montes in northeastern Elysium Planitia has a cracked surface that, combined with its overall shape, gives the appearance of a giant loaf of bread in this image from NASA's Mars Odyssey spacecraft.

"Bread Loaf" Mesa East of Phlegra Montes

This image from NASA's Mars Odyssey spacecraft shows a location within Semeykin Crater, which is in the Martian northern hemisphere.
This image from NASA's Mars Odyssey spacecraft shows a location within Semeykin Crater, which is in the Martian northern hemisphere.

Semeykin Crater

In this region of the Olympus Mons aureole, located to the southwest of the volcano, the surface has been eroded by the wind into linear landforms called yardangs, which can be seen in this image from NASA's Mars Odyssey spacecraft.
In this region of the Olympus Mons aureole, located to the southwest of the volcano, the surface has been eroded by the wind into linear landforms called yardangs, which can be seen in this image from NASA's Mars Odyssey spacecraft.

Yardangs near Olympus Mons

Located north of Olympus Mons and west of Alba Patera, Acheron Fossae, seen in this NASA Mars Odyssey image, provides a record of early tectonic activity in the Tharsis region.
Located north of Olympus Mons and west of Alba Patera, Acheron Fossae, seen in this NASA Mars Odyssey image, provides a record of early tectonic activity in the Tharsis region.

Western Portion of Acheron Fossae

This scene from NASA's Mars Odyssey spacecraft of the dust covered plains of eastern Arabia Terra portrays a range of geological time. Three craters at the center of the image capture some of this range.
This scene from NASA's Mars Odyssey spacecraft of the dust covered plains of eastern Arabia Terra portrays a range of geological time. Three craters at the center of the image capture some of this range.

Geological Time on Display in Arabia Terra

Palos Crater, seen in this NASA Mars Odyssey image, has been suggested as a future landing site for Mars missions because it may contain lake deposits. This crater has a channel called Tinto Vallis, which enters from the south.
Palos Crater, seen in this NASA Mars Odyssey image, has been suggested as a future landing site for Mars missions because it may contain lake deposits. This crater has a channel called Tinto Vallis, which enters from the south.

Palos Crater

This NASA Mars Odyssey image shows the dissected interior of a crater in the Cydonia region of Mars. The flat-topped buttes and mesas in the northern portion of the image were once a continuous layer of material that filled the crater.
This NASA Mars Odyssey image shows the dissected interior of a crater in the Cydonia region of Mars. The flat-topped buttes and mesas in the northern portion of the image were once a continuous layer of material that filled the crater.

Crater in Cydonia

This image from NASA's Mars Odyssey spacecraft shows Rampart crater in Utopia Planitia, west of NASA's Viking 2 landing site.
This image from NASA's Mars Odyssey spacecraft shows Rampart crater in Utopia Planitia, west of NASA's Viking 2 landing site.

Rampart Crater

This pair of craters seen by NASA's Mars Odyssey just north of the Hellas Basin demonstrate the rugged topography that can result when an impact occurs on the rim of an existing crater.
This pair of craters seen by NASA's Mars Odyssey just north of the Hellas Basin demonstrate the rugged topography that can result when an impact occurs on the rim of an existing crater.

Crater Upon Crater

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