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Boulder Strewn Plain in Northern Utopia Planitia
Boulder Strewn Plain in Northern Utopia Planitia
Full Resolution
This image shows NASA's Mars Exploration Rover Opportunity perched on the edge of "Concepción" crater in Meridiani Planum, Mars.
Opportunity at 'Concepción' Crater, Seen from Orbit
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This image from the panoramic camera on NASA's Mars Exploration Rover Opportunity shows a rock called "Chocolate Hills," which the rover found and examined at the edge of a young crater called "Concepción."
Rock with Odd Coating Beside a Young Martian Crater, False Color
Full Resolution
Changes on Dune Slip Face, Nili Patera, Mars
Changes on Dune Slip Face, Nili Patera, Mars
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Changes in Ripples on Martian Dunes in Nili Patera
Changes in Ripples on Martian Dunes in Nili Patera
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Location Map for Images of Changing Martian Dunes
Location Map for Images of Changing Martian Dunes
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Changes at Edges of Dark Dunes in Nili Patera, Mars
Changes at Edges of Dark Dunes in Nili Patera, Mars
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Dunes and Inverted Crater in Arabia Terra
Dunes and Inverted Crater in Arabia Terra
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Glacial Ice Deposits in Mid-Latitudes of Mars
Glacial Ice Deposits in Mid-Latitudes of Mars
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Stages in the seasonal disappearance of surface ice from the ground around the Phoenix Mars Lander are visible in these images taken on Feb. 8, 2010, (left) and Feb. 25, 2010, during springtime on northern Mars.
Ice Around Phoenix Lander Continues to Lessen in Spring
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A digital terrain model generated from a stereo pair of images provides this synthesized, oblique view of a portion of the wall terraces of Mojave Crater in the Xanthe Terra region of Mars.
Terrain Model of Mars' Mojave Crater
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Layers in Upper Formation of Gale Crater Mound
Layers in Upper Formation of Gale Crater Mound
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Layers in Lower Formation of Gale Crater Mound
Layers in Lower Formation of Gale Crater Mound
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Perspective View of Layered Mound in Gale Crater, Mars (non labeled)
Perspective View of Layered Mound in Gale Crater, Mars
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Perspective View of Layered Mound in Gale Crater, Mars
Perspective View of Layered Mound in Gale Crater, Mars (Labeled)
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In the middle of this picture, the robotic arm is bent at nearly a 90-degree angle, with the instruments on the end of the arm reaching to the right. Behind the arm is the laboratory where it is being tested. One engineer is hidden behind a bank of computers, while another with a goatee stands watching in the back, beneath a yellow ceiling crane. Both engineers wear white lab coats. Metal lab equipment is scattered throughout the room.
Robotic Arm Testing Image #2
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In the middle of this image, the long robotic arm rises straight up toward the ceiling of the lab where it is being tested. The arm is white, and is flexible at several gray round 'joints.' Red wires dangle and are strung along various parts of the arm. At the end of the arm is a complicated set of instruments. In the background, a yellow crane for lifting equipment up to 2 tons (4,000 pounds) can slide along the ceiling to place heavy equipment anywhere in the room. A metal garage-like door and computer stations lie behind the area where the arm is extended.
Robotic Arm Testing Image #1
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Image of MAVEN spacecraft, annotated to identify instruments
MAVEN Instrument Panel
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Dune Symmetry Inside Martian Crater
Dune Symmetry Inside Martian Crater
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NASA's Phoenix Mars Lander, its backshell and its heatshield are visible within this enhanced-color image of the Phoenix landing site taken on Jan. 6, 2010 by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.

With early spring at the Phoenix landing site comes progressive sublimation of carbon-dioxide frost that has blanketed the lander and surrounding terrain throughout the winter. During the long polar-winter night, atmospheric carbon dioxide freezes onto the surface, building up a layer of frost roughly 30 centimeters (about one foot) thick. In the spring this frost returns to atmosphere gas (sublimates) over the course of several months. This image, part of a seasonal frost monitoring sequence, shows some areas of bare ground are beginning to be exposed. However, extensive frost patches remain in the topographic lows, such as the troughs of the local polygonally patterned surface.
Phoenix Lander Amid Disappearing Spring Ice
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Phoenix Lander Amid Disappearing Spring Ice
Phoenix Lander Amid Disappearing Spring Ice
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Turbulent Lava Flow in Mars' Athabasca Valles
Turbulent Lava Flow in Mars' Athabasca Valles
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bright layered deposits on a plateau near Juventae Chasma in the Valles Marineris region of Mars
Bright Layered Deposits with Clues of Acidic Water
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Image of Jennifer Eigenbrode using a soil simulant
Scientist Jennifer Eigenbrode using a soil simulant for testing
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