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Impact craters can be created anywhere on the surface of Mars at any time. This image taken by NASA's 2001 Mars Odyssey shows a crater located on the floor of Coprates Chasma.
Impact craters can be created anywhere on the surface of Mars at any time. This image taken by NASA's 2001 Mars Odyssey shows a crater located on the floor of Coprates Chasma.

Coprates Crater

This image from NASA's 2001 Mars Odyssey is of an unnamed channel located in Xanthe Terra.
This image from NASA's 2001 Mars Odyssey is of an unnamed channel located in Xanthe Terra.

Channel in Xanthe Terra

This image from NASA's 2001 Mars Odyssey spacecraft shows dunes near the north polar cap of Mars. It is springtime at the north pole and the dunes are starting to lose their frost cover.
This image from NASA's 2001 Mars Odyssey spacecraft shows dunes near the north polar cap of Mars. It is springtime at the north pole and the dunes are starting to lose their frost cover.

Polar Dunes

The lava flows in this image taken by NASA's 2001 Mars Odyssey spacecraft are part of the extensive flow field of Arsia Mons.
The lava flows in this image taken by NASA's 2001 Mars Odyssey spacecraft are part of the extensive flow field of Arsia Mons.

Arsia Mons Flows

This image from NASA's 2001 Mars Odyssey is located south of Olympus Mons and east of Gordii Dorsum, in a heavily wind eroded region. The winds are predominately east/west in this area.
This image from NASA's 2001 Mars Odyssey is located south of Olympus Mons and east of Gordii Dorsum, in a heavily wind eroded region. The winds are predominately east/west in this area.

Wind Effects

Wind has eroded the deposit on the floor of Gale Crater in this image captured by NASA's 2001 Mars Odyssey.
Wind has eroded the deposit on the floor of Gale Crater in this image captured by NASA's 2001 Mars Odyssey.

Gale Crater

The rock 'Ithaca' is shown here with a rougher lower texture and smoother texture on top, and appears to be a piece of the local sedimentary bedrock protruding from the surrounding soil in Gale Crater as seen by NASA's Curiosity Mars rover.
The rock 'Ithaca' is shown here with a rougher lower texture and smoother texture on top, and appears to be a piece of the local sedimentary bedrock protruding from the surrounding soil in Gale Crater as seen by NASA's Curiosity Mars rover.

Target Rock 'Ithaca' in Gale Crater, Mars

Moving eastward from the previous image, we continue to see the northern floor and rim of Gale Crater and the northern part of Mt. Sharp. This image from NASA's Mars Odyssey spacecraft shows a weathered region of the lower elevations of Mt. Sharp.
Moving eastward from the previous image, we continue to see the northern floor and rim of Gale Crater and the northern part of Mt. Sharp. This image from NASA's Mars Odyssey spacecraft shows a weathered region of the lower elevations of Mt. Sharp.

Images of Gale #5

This image shows numerous gullies that dissect the rim of Bunge Crater as seen by NASA's 2001 Mars Odyssey spacecraft.
This image shows numerous gullies that dissect the rim of Bunge Crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Bunge Gullies

The dark material in this VIS image of Danielson Crater are dunes at the foot of the fill material located on the southwestern end of the crater floor.
The dark material in this VIS image of Danielson Crater are dunes at the foot of the fill material located on the southwestern end of the crater floor.

Danielson Crater

This map indicates some of the geological information gained from orbital observations of Endeavour Crater, which has been the long-term destination for NASA's Mars Exploration Rover Opportunity since mid-2008.
This map indicates some of the geological information gained from orbital observations of Endeavour Crater, which has been the long-term destination for NASA's Mars Exploration Rover Opportunity since mid-2008.

Geologic Map, West Rim of Endeavour Crater, Mars

This observation from NASA's Mars Reconnaissance Orbiter shows a Southern hemisphere crater with gullies, dunes, periglacial modification, bright rock deposits, and dust devil tracks.
This observation from NASA's Mars Reconnaissance Orbiter shows a Southern hemisphere crater with gullies, dunes, periglacial modification, bright rock deposits, and dust devil tracks.

Southern Hemisphere Crater with Dune Field

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Olympus Rupes, part of the steep margin surrounding Olympus Mons. The term rupes means scarp.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Olympus Rupes, part of the steep margin surrounding Olympus Mons. The term rupes means scarp.

Olympus Rupes

This image captured by NASA's 2001 Mars Odyssey spacecraft of Daedalia Planum contains a narrow lava flow and shows the end of the flow. The end of a lava flow is often called the 'toe' and is formed when the eruption creating the flow slows down or stops
This image captured by NASA's 2001 Mars Odyssey spacecraft of Daedalia Planum contains a narrow lava flow and shows the end of the flow. The end of a lava flow is often called the 'toe' and is formed when the eruption creating the flow slows down or stops

Flow Margin

This image of Baltisk Crater shows a sand sheet on the crater floor and channels dissecting the outer rim as seen by NASA's 2001 Mars Odyssey spacecraft.
This image of Baltisk Crater shows a sand sheet on the crater floor and channels dissecting the outer rim as seen by NASA's 2001 Mars Odyssey spacecraft.

Baltisk Crater

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

Currently displaying images 2076-2100 of 3082
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