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This map of a portion of the western rim of Endeavour Crater on Mars shows the area where NASA's Mars Exploration Rover Opportunity worked for 20 months.
This map of a portion of the western rim of Endeavour Crater on Mars shows the area where NASA's Mars Exploration Rover Opportunity worked for 20 months.

Opportunity Heads Toward Next Destination, 'Solander Point'

NASA's Mars Exploration Rover Opportunity inspected this mineral vein, called 'Homestake,' in November 2011 at the northern end of the 'Cape York' section of Endeavour Crater's western rim.
NASA's Mars Exploration Rover Opportunity inspected this mineral vein, called 'Homestake,' in November 2011 at the northern end of the 'Cape York' section of Endeavour Crater's western rim.

'Homestake' Vein on 'Cape York,' Color Enhanced

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are part of Olympia Undae.

Polar Dunes

The channel in the bottom part of this image captured by NASA's 2001 Mars Odyssey spacecraft was created by lava flow rather than water flow. This feature is located in the Tharsis plains east of Olympus Mons.
The channel in the bottom part of this image captured by NASA's 2001 Mars Odyssey spacecraft was created by lava flow rather than water flow. This feature is located in the Tharsis plains east of Olympus Mons.

Lava Channel

This image captured by NASA's 2001 Mars Odyssey spacecraft continues to follow the channel seen in the past two images. The rover landing site is at the top margin of this image.
This image captured by NASA's 2001 Mars Odyssey spacecraft continues to follow the channel seen in the past two images. The rover landing site is at the top margin of this image.

Images of Gale #17

Dark slope streaks mark the rim of this unnamed crater as seen by NASA's 2001 Mars Odyssey spacecraft.
Dark slope streaks mark the rim of this unnamed crater as seen by NASA's 2001 Mars Odyssey spacecraft.

Dark Slope Streaks

This image from NASA's Curiosity rover just after discarding a soil sample as part of its first 'decontamination' exercise. A small amount of remnant material is visible inside the delivery tube, which is magnified in the blow-up at lower right.
This image from NASA's Curiosity rover just after discarding a soil sample as part of its first 'decontamination' exercise. A small amount of remnant material is visible inside the delivery tube, which is magnified in the blow-up at lower right.

Thanks for the Scrub

Gale Crater contains a large layered deposit, part of which is shown in this image captured by NASA's 2001 Mars Odyssey spacecraft. This deposit is the target of the Curiosity Lander due to land in early August 2012.
Gale Crater contains a large layered deposit, part of which is shown in this image captured by NASA's 2001 Mars Odyssey spacecraft. This deposit is the target of the Curiosity Lander due to land in early August 2012.

Gale Crater

Ceraunius Fossae is the region of fractures and volcanic flows south of Alba Mons shown in this image captured by NASA's Mars Odyssey.
Ceraunius Fossae is the region of fractures and volcanic flows south of Alba Mons shown in this image captured by NASA's Mars Odyssey.

Ceraunius Fossae

Researchers used the Pancam on NASA's Mars Exploration Rover Opportunity to capture this view of comet C/2013 A1 Siding Spring as it flew near Mars on Oct. 19, 2014.
Researchers used the Pancam on NASA's Mars Exploration Rover Opportunity to capture this view of comet C/2013 A1 Siding Spring as it flew near Mars on Oct. 19, 2014.

Mars Rover Opportunity's View of Passing Comet (Short Exposure)

This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Arabia Terra.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows sand dunes on the floor of an unnamed crater in Arabia Terra.

Dunes

This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.
This mantle observed by NASA's Mars Reconnaissance Orbiter is thought to be deposited as snow during periods when the angle of the tilt of Mars' rotational axis-called obliquity-is much higher, which last happened around 10 million years ago.

Mantled Terrain in the Southern Mid-Latitudes

The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are near the large dune field called Olympia Undae.
The dunes in this image captured by NASA's 2001 Mars Odyssey spacecraft are near the large dune field called Olympia Undae.

Polar Dunes

A delta deposit sits on the floor of this unnamed crater in Arabia Terra, as shown in this image from NASA's 2001 Mars Odyssey spacecraft. The channel that created the delta dissects the crater rim.
A delta deposit sits on the floor of this unnamed crater in Arabia Terra, as shown in this image from NASA's 2001 Mars Odyssey spacecraft. The channel that created the delta dissects the crater rim.

Crater Delta

The volcanic flows in this image captured by NASA's Mars Odyssey spacecraft are part of Daedalia Planum, an extensive flow field originating from Arsia Mons.
The volcanic flows in this image captured by NASA's Mars Odyssey spacecraft are part of Daedalia Planum, an extensive flow field originating from Arsia Mons.

Daedalia Planum

The volcanic flow in this image from NASA's 2001 Mars Odyssey spacecraft appears to have flowed in one layer. The surface texture is blocks of lava which cooled and still moved on molten lava below, producing the plate-like texture.
The volcanic flow in this image from NASA's 2001 Mars Odyssey spacecraft appears to have flowed in one layer. The surface texture is blocks of lava which cooled and still moved on molten lava below, producing the plate-like texture.

Lava

The main agent of erosion on Mars today is the wind. Wind has sculpted the surface in this region into a set of hills and valleys called yardangs on Earth. This image is from NASA's 2001 Mars Odyssey spacecraft.
The main agent of erosion on Mars today is the wind. Wind has sculpted the surface in this region into a set of hills and valleys called yardangs on Earth. This image is from NASA's 2001 Mars Odyssey spacecraft.

Erosion

This VIS image shows dunes in a topographic low within Aonia Terra.
This VIS image shows dunes in a topographic low within Aonia Terra.

Dunes

Daedalia Planum is comprised of lava flows from Arsia Mons. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
Daedalia Planum is comprised of lava flows from Arsia Mons. This image was captured by NASA's 2001 Mars Odyssey spacecraft.

Daedalia Planum

This scene shows the 'Murray Ridge' portion of the western rim of Endeavour Crater on Mars, as seen by NASA's Opportunity rover. It is presented in false color to make some differences between materials easier to see.
This scene shows the 'Murray Ridge' portion of the western rim of Endeavour Crater on Mars, as seen by NASA's Opportunity rover. It is presented in false color to make some differences between materials easier to see.

'Murray Ridge' on Rim of Endeavour Crater on Mars, False Color

Do you see what I see in this image from NASA's Mars Odyssey spacecraft? These layered deposits look like a giant bear facing to the left.
Do you see what I see in this image from NASA's Mars Odyssey spacecraft? These layered deposits look like a giant bear facing to the left.

THEMIS Art #120

This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the huge dune field located at the north polar cap. As spring continues to deepen, the dunes are becoming darker and darker as they lose their winter frost cover.
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a portion of the huge dune field located at the north polar cap. As spring continues to deepen, the dunes are becoming darker and darker as they lose their winter frost cover.

North Polar Dunes

This image from NASA's Curiosity Rover shows a high-resolution view of an area that is known as Goulburn Scour, a set of rocks blasted by the engines of Curiosity's descent stage on Mars.
This image from NASA's Curiosity Rover shows a high-resolution view of an area that is known as Goulburn Scour, a set of rocks blasted by the engines of Curiosity's descent stage on Mars.

Best View of Goulburn Scour

This radargram profile from ESA's Mars Express and NASA's Mars Global Surveyor orbiter shows data from the subsurface of Mars in the ice-rich north polar plateau of Mars.
This radargram profile from ESA's Mars Express and NASA's Mars Global Surveyor orbiter shows data from the subsurface of Mars in the ice-rich north polar plateau of Mars.

Radargram of Mars North Polar Plateau from Mars Express

This image from NASA's Mars Odyssey shows different flow surfaces in Daedalia Planum.
This image from NASA's Mars Odyssey shows different flow surfaces in Daedalia Planum.

Daedalia Planum

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