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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Maja Valles.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Maja Valles.

Maja Valles

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Lycus Sulci, a complex region of ridges located on the northern side of Olympus Mons. The term sulci means subparallel furrows and ridges.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of Lycus Sulci, a complex region of ridges located on the northern side of Olympus Mons. The term sulci means subparallel furrows and ridges.

Lycus Sulci

This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Olympia Undae, the vast dune field near the north pole.
This image from NASA's 2001 Mars Odyssey spacecraft shows a small portion of Olympia Undae, the vast dune field near the north pole.

Olympia Undae

The small, dark sand dunes at the bottom of this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Escalante Crater.
The small, dark sand dunes at the bottom of this image captured by NASA's 2001 Mars Odyssey spacecraft are located on the floor of Escalante Crater.

Escalante Dunes

This image from NASA's 2001 Mars Odyssey spacecraft shows small sets of dunes on the plains of Aonia Terra.
This image from NASA's 2001 Mars Odyssey spacecraft shows small sets of dunes on the plains of Aonia Terra.

Dunes

This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the weathering of the eastern side of Mt. Sharp.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows more of the weathering of the eastern side of Mt. Sharp.

Images of Gale #10

This image from NASA's Mars Reconnaissance Orbiter captures light-toned ridges found in a large fracture located east of Holden Crater forming a curious box-like pattern.
This image from NASA's Mars Reconnaissance Orbiter captures light-toned ridges found in a large fracture located east of Holden Crater forming a curious box-like pattern.

Many Small Interesting Ridges in Erythraea Fossa

The complex channel and streamlined islands are part of Maja Valles as seen by NASA's 2001 Mars Odyssey spacecraft.
The complex channel and streamlined islands are part of Maja Valles as seen by NASA's 2001 Mars Odyssey spacecraft.

Maja Valles

The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft were most likely created by lava flows from Alba Mons, located in the northern Tharsis region.
The channels in this image captured by NASA's 2001 Mars Odyssey spacecraft were most likely created by lava flows from Alba Mons, located in the northern Tharsis region.

Channels

More dunes are encountered surrounding the north polar cap by NASA's 2001 Mars Odyssey spacecraft.
More dunes are encountered surrounding the north polar cap by NASA's 2001 Mars Odyssey spacecraft.

More Polar Dunes

This set of images illustrates how the science filters of the Mast Camera (Mastcam) on NASA's Mars rover Curiosity can be used to investigate aspects of the composition and mineralogy of materials on Mars.
This set of images illustrates how the science filters of the Mast Camera (Mastcam) on NASA's Mars rover Curiosity can be used to investigate aspects of the composition and mineralogy of materials on Mars.

Drill Hole Image and Spectra Acquired by Mastcam

The unnamed channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is located on the northeastern margin of Tempe Terra.
The unnamed channel in this image captured by NASA's 2001 Mars Odyssey spacecraft is located on the northeastern margin of Tempe Terra.

Tempe Terra

A surprise landslump in Melas Chasma was observed by NASA's Mars Reconnaissance Orbiter.
A surprise landslump in Melas Chasma was observed by NASA's Mars Reconnaissance Orbiter.

A Surprise Landslump in Melas Chasma

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

Rim Channels

This image from NASA's Mars Odyssey spacecraft shows Gale crater, which is east of the landing site. It shows the northern extent of the dunes, and the layers in Mt. Sharp are visible at the bottom of the image.
This image from NASA's Mars Odyssey spacecraft shows Gale crater, which is east of the landing site. It shows the northern extent of the dunes, and the layers in Mt. Sharp are visible at the bottom of the image.

Images of Gale #3

Channels are a common feature on the margin of Terra Cimmeria where the elevation changes from highland to northern lowlands in this image captured by NASA's Mars Odyssey.
Channels are a common feature on the margin of Terra Cimmeria where the elevation changes from highland to northern lowlands in this image captured by NASA's Mars Odyssey.

Channels on Terra Cimmeria

NASA's Mars Odyssey captured this image of Ulysses Fossae, located in the Tharsis Volcanic region. Cross cutting tectonic fractures indicate that this region underwent stresses in multiple directions.
NASA's Mars Odyssey captured this image of Ulysses Fossae, located in the Tharsis Volcanic region. Cross cutting tectonic fractures indicate that this region underwent stresses in multiple directions.

Ulysses Fossae

At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.
At Mars' North Pole is a dome of icy layers ranging up to 2 kilometers thick, roughly analogous to the Earth's ice caps in Greenland or Antarctica. This image is from NASA's Mars Reconnaissance Orbiter.

The Icy Surface of the North Polar Cap

This image shows a portion of the dunes on the floor of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft.
This image shows a portion of the dunes on the floor of Rabe Crater captured by NASA's 2001 Mars Odyssey spacecraft.

Rabe Crater Dunes

The channels in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are called Hephaestus Fossae and were most likely formed by lava flow and erosion rather than being eroded by water.
The channels in this image, taken by NASA's 2001 Mars Odyssey spacecraft, are called Hephaestus Fossae and were most likely formed by lava flow and erosion rather than being eroded by water.

Hephaestus Fossae

This NASA 2001 Mars Odyssey image of the southwestern flank of Alba Mons shows lava flows and collapse features.
This NASA 2001 Mars Odyssey image of the southwestern flank of Alba Mons shows lava flows and collapse features.

Alba Mons

Streamlined islands indicate the direction of flow in this image of Shalbatana Vallis. taken by NASA's 2001 Mars Odyssey spacecraft.
Streamlined islands indicate the direction of flow in this image of Shalbatana Vallis. taken by NASA's 2001 Mars Odyssey spacecraft.

Shalbatana Vallis

Several gullies located on the rim of this unnamed crater in Terra Sirenum are seen in this image taken by NASA's 2001 Mars Odyssey spacecraft.
Several gullies located on the rim of this unnamed crater in Terra Sirenum are seen in this image taken by NASA's 2001 Mars Odyssey spacecraft.

Gullies in Terra Sirenum

This series of images spanning a period of 15 weeks shows a pair of fresh craters taken by NASA's Mars Reconnaissance Orbiter. Bright, bluish material apparent in the earliest images disappears by the later ones.
This series of images spanning a period of 15 weeks shows a pair of fresh craters taken by NASA's Mars Reconnaissance Orbiter. Bright, bluish material apparent in the earliest images disappears by the later ones.

Ice in Pair of Fresh Craters on Mars Fades with Time

NASA's Mars Exploration Rover Opportunity combined images into this stereo, 360-degree view on March 28-30, 2009. In this view, the western edge of Home Plate is on the portion of the horizon farthest to the left. 3D glasses are necessary.
NASA's Mars Exploration Rover Opportunity combined images into this stereo, 360-degree view on March 28-30, 2009. In this view, the western edge of Home Plate is on the portion of the horizon farthest to the left. 3D glasses are necessary.

View Ahead After Spirit's Sol 1861 Drive (Stereo)

Currently displaying images 1926-1950 of 2607
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