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Lismore Crater

This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.

July 17, 2012

This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.

Credit

NASA/JPL-Caltech/ASU

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This region of Terra Sabaea contains areas with high densities of small craters.
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This region of Terra Sabaea contains areas with high densities of small craters.
Lot of Craters in Terra Sabaea
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
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This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
Oblique view of Gale Crater from the North (Unannotated)
Although it is 45 kilometers (28 miles) wide, countless layers of ice and dust have all but buried Udzha Crater.
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Although it is 45 kilometers (28 miles) wide, countless layers of ice and dust have all but buried Udzha Crater.
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This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT).
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This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT).
Downslope of the Fan
Wind shadow and real shadow combine to give a striking image of a comet.
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Wind shadow and real shadow combine to give a striking image of a comet.
THEMIS Images as Art
A lunar eclipse, a solar eclipse and Mars has a close encounter with a comet.
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What's Up for October?
This image superimposes Gamma-Ray Spectrometer data from NASA's Mars Odyssey orbiter onto topographic data from the laser altimeter on NASA's Mars Global Surveyor.
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Potassium Concentrations on Mars
A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 meters (3,300 feet) wide.
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A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 meters (3,300 feet) wide.
Mars Odyssey All Stars: Dunes Engulf Crater
Fly Through Mariner Valley
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Fly Through Mariner Valley
Fly Through Mariner Valley
This animation shows how NASA's Curiosity rover communicates with Earth via two of NASA's Mars orbiters, Mars Reconnaissance Orbiter (MRO) and Odyssey, and the European Space Agency's Mars Express....
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Curiosity Communicates with Help From Its 'Friends'
Curiosity Communicates with Help From Its 'Friends'
A small impact crater on Mars named Gratteri, 4.3 miles (6.9 km) wide, lies at the center of large dark streaks.
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A small impact crater on Mars named Gratteri, 4.3 miles (6.9 km) wide, lies at the center of large dark streaks.
Mars Impact Crater Gratteri
Olympica Fossae is a complex channel located on the volcanic plains between Alba Mons and Olympus Mons. The sinuosity of the large channel in the middle of this image from NASA's 2001 Mars Odyssey ...
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Olympica Fossae
Olympica Fossae
On the southwest edge of the immense volcanic region of Tharsis, lava from its giant volcanoes flowed down to meet the old cratered landscape of Terra Sirenum.
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On the southwest edge of the immense volcanic region of Tharsis, lava from its giant volcanoes flowed down to meet the old cratered landscape of Terra Sirenum.
Terra Sirenum
This lunar-like scene occurs along the southeastern rim of the Isidis Planitia basin. The Isidis basin is an ancient impact crater some 1200 km across that is found along the boundary separating th...
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This lunar-like scene occurs along the southeastern rim of the Isidis Planitia basin. The Isidis basin is an ancient impact crater some 1200 km across that is found along the boundary separating the heavily-cratered southern highland terrain of Mars from the northern lowlands. Elements of both terrains are evident in this image as an island of rugged highland terrain surrounded by smoother lowland terrain. The resurfacing of the Isidis basin produced a system of wrinkle ridges, some of which are seen on the lowland terrain in the image. Wrinkle ridges are a common feature on the surface of the moon and add to the lunar-like quality of this image. Layers are visible in the large island, the most resistant of which likely are from lava flows that created the highland terrain. The process by which the global-scale highland/lowland dichotomy was created remains a mystery.
Isidis Rim
This artist's animation shows how orbiters over Mars will monitor the landing of NASA's Curiosity rover. (No audio)
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Great Convergence of Spacecraft around Mars
A false-color mosaic focuses on one junction in Noctis Labyrinthus where canyons meet to form a depression 4,000 meters (13,000 feet) deep.
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A false-color mosaic focuses on one junction in Noctis Labyrinthus where canyons meet to form a depression 4,000 meters (13,000 feet) deep.
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This movie shows three views of the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter. The apparent motion is due to movement by Odyssey's infrared camera, Thermal ...
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This movie shows three views of the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter.
Odyssey's Three Views of Phobos in Visible Light
Planum Boreum crater
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Planum Boreum crater
Planum Boreum crater
A large sandsheet with surface dune forms is shown in today's image of Aonia Terra.
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A large sandsheet with surface dune forms is shown in today's image of Aonia Terra.
Dunes in Aonia Terra
The channels in this VIS image are part of Tyrrhena Fossae on the northern flank of Tyrrhenus Mons.
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The channels in this VIS image are part of Tyrrhena Fossae on the northern flank of Tyrrhenus Mons.
Tyrrhena Fossae
This mosaic image of Valles Marineris - colored to resemble the martian surface - comes from the Thermal Emission Imaging System (THEMIS), a visible-light and infrared-sensing camera on NASA's Mars...
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This mosaic image of Valles Marineris - colored to resemble the martian surface - comes from the Thermal Emission Imaging System (THEMIS), a visible-light and infrared-sensing camera on NASA's Mars Odyssey orbiter.
The Grand Canyon of Mars-Valles Marineris
This mosaic of daytime infrared images of Gusev Crater, taken by the camera system on the Mars Odyssey spacecraft, has been draped over topography data obtained by Mars Global Surveyor.
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This mosaic of daytime infrared images of Gusev Crater, taken by the camera system on the Mars Odyssey spacecraft, has been draped over topography data obtained by Mars Global Surveyor.
Gusev Crater
Ninth-grade, high-school students from Peoria, AZ analyze images of Mars.
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Artist rendering of commercial Mars satellites providing communications back to Earth.
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Artist rendering of commercial Mars satellites providing communications back to Earth.
Artist's Concept of Mars Satellites
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This view combines information from two instruments on a NASA Mars orbiter to map color-coded composition over the shape of the ground within the Nili Fossae plains region of Mars. Carbonate-rich deposits in this area (coded green) hold some carbon formerly in the atmosphere's carbon dioxide.
Rocks Here Sequester Some of Mars' Early Atmosphere

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