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Opportunity's Surroundings After Sol 2363 Drive (Polar)

This image from NASA's Curiosity rover shows the inlet covers for the Sample Analysis at Mars instrument as the rover continues to check out its instruments in the first phase after landing.
This image from NASA's Curiosity rover shows the inlet covers for the Sample Analysis at Mars instrument as the rover continues to check out its instruments in the first phase after landing.

Opening and Closing SAM

This image as seen by NASA's 2001 Mars Odyssey spacecraft shows the layering of the ice at the north pole.
This image as seen by NASA's 2001 Mars Odyssey spacecraft shows the layering of the ice at the north pole.

Polar Layers

This plot segregates various minerals examined by NASA's Mars Exploration Rover Opportunity according to their different compositions; for example, those with more iron and magnesium oxides are located in the lower right corner.
This plot segregates various minerals examined by NASA's Mars Exploration Rover Opportunity according to their different compositions; for example, those with more iron and magnesium oxides are located in the lower right corner.

Mineral Plot from 'Esperance' Target

The hole that NASA's Curiosity Mars rover drilled into target rock 'John Klein' provided a view into the interior of the rock, as well as obtaining a sample of powdered material from the rock.
The hole that NASA's Curiosity Mars rover drilled into target rock 'John Klein' provided a view into the interior of the rock, as well as obtaining a sample of powdered material from the rock.

View into 'John Klein' Drill Hole in Martian Mudstone

This graph shows the atmospheric pressure at the surface of Mars, as measured by the Rover Environmental Monitoring Station on NASA's Curiosity rover. Pressure is a measure of the amount of air in the whole column of atmosphere sitting above the rover.
This graph shows the atmospheric pressure at the surface of Mars, as measured by the Rover Environmental Monitoring Station on NASA's Curiosity rover. Pressure is a measure of the amount of air in the whole column of atmosphere sitting above the rover.

Pressure Cycles on Mars

This image from NASA's 2001 Mars Odyssey spacecraft shows the dunes located on the floor of Gale Crater.
This image from NASA's 2001 Mars Odyssey spacecraft shows the dunes located on the floor of Gale Crater.

Gale Crater Dunes

As seen by NASA's 2001 Mars Odyssey spacecraft, the dunes in this image are located on the western margin of Hellas Planitia.
As seen by NASA's 2001 Mars Odyssey spacecraft, the dunes in this image are located on the western margin of Hellas Planitia.

Hellas Dunes

This image from NASA's Mars Odyssey shows the western end of Candor Chasma, including a large landslide deposit.
This image from NASA's Mars Odyssey shows the western end of Candor Chasma, including a large landslide deposit.

Candor Chasma

Northern Terra Sabea is dissected by numerous fractures and channels as shown by this image from NASA's 2001 Mars Odyssey.
Northern Terra Sabea is dissected by numerous fractures and channels as shown by this image from NASA's 2001 Mars Odyssey.

Terra Sabaea

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

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