Mars Topography

Mars Topography
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NASA's Dawn spacecraft obtained this image of the surface of asteroid Vesta with its framing camera on August 12, 2011. This image was taken through the framing camera's clear filter. The image has a resolution of about 260 meters per pixel.
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These images from NASA's Dawn spacecraft are dominated by the 35km diameter Bellicia crater on asteroid Vesta, after which Bellicia quadrangle is named.
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NASA's Lunar Reconnaissance Orbiter captures frozen impact melt flows on the floor of Moore F, a farside highlands crater.
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These images from NASA's Dawn spacecraft are located in asteroid Vesta's Floronia quadrangle, in Vesta's northern hemisphere. Licinia is the large, bowl shaped crater in the center with a sharp rim, which has a scalloped edge.
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This pair of maps based on albedo information from NASA's Mars Odyssey orbiter and topographical information from NASA's Mars Global Surveyor orbiter indicates locations of confirmed sites of recurrent slope linea on Mars.
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These images from NASA's Dawn spacecraft show the Domitia crater in Vesta's northern hemisphere and the topography of the surrounding region, which includes the 'Snowman' craters.
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These images from NASA's Dawn spacecraft shows a region around the asteroid Vesta's equatorial troughs with two different resolutions. More details are visible in the right-hand image such as small linear grooves running roughly parallel to the troughs.
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These images from NASA's Dawn spacecraft show many craters, which have different states of preservation, in Vesta's Bellicia quadrangle in the northern hemisphere.
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These images from NASA's Dawn spacecraft show part of asteroid Vesta's equatorial region, which contains a prominent, deep impact crater (lower center of images) and large troughs (linear depressions).
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NASA's Dawn spacecraft obtained this albedo image of asteroid Vesta with its framing camera on August 11th 2011.
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This map of Ceres, made from images taken by NASA's Dawn spacecraft, shows the locations of about 130 bright areas across the dwarf planet's surface, highlighted in blue. Most of these bright areas are associated with craters.
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These images from NASA's Dawn spacecraft are located in asteroid Vesta's Marcia quadrangle, a few degrees below Vesta's equator. Octavia Crater looks remarkably like a terrestrial landslide.
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NASA's Dawn spacecraft shows the central area of the south polar basin. This view is rotated by approximately 90°.
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These images from NASA's Dawn spacecraft are located in asteroid Vesta's Lucaria Tholus quadrangle, in Vesta's southern hemisphere.
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This image from NASA's Mars Odyssey spacecraft shows part of Ganges Chasma in Valles Marineris. The colors indicate compositional variations in the rocks exposed in the wall and floor of Ganges and in the dust and sand on the rim of the canyon.
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These images from NASA's Dawn spacecraft show Oppia crater on asteroid Vesta, after which Oppia quadrangle is named. Oppia crater is a distinctive crater because it has an unusually shaped rim, which is almost rectangular in form.
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These images from NASA's Dawn spacecraft show Sextilia crater on asteroid Vesta.
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Map of Mars' Topography
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These images from NASA's Dawn spacecraft show Pinaria crater on asteroid Vesta, after which Pinaria quadrangle is named. Many young fresh impact craters are visible on the slumped material.
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NASA's Dawn spacecraft shows the central area of the south polar basin. This view is rotated by approximately 60°.
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This image shows Cornelia Crater on the large asteroid Vesta. On the right is an inset image showing an example of curved gullies, indicated by the short white arrows, and a fan-shaped deposit, indicated by long white arrows.
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DETAILS
Image Number: 1889-60383487Royalty FreeCredit Line:Steve Nagy/Design Pics/SuperStockCollection:Design PicsStory:Asteroid Surfaces and CratersContributor:Steve NagyModel Release:NoProperty Release:NoResolution:4800×4376
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