Crossing Paths. At the left edge of this color view is a relatively fresh crater as seen by NASA's MESSENGER spacecraft.

Crossing Paths. At the left edge of this color view is a relatively fresh crater as seen by NASA's MESSENGER spacecraft.
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NASA's Dawn spacecraft views a portion of the northern rim of Urvara Crater (101 miles, 163 kilometers wide) in this scene from Ceres taken on June 3, 2016, at a distance of about 240 miles (385 kilometers) above the surface.
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This image from NASA's Dawn spacecraft shows craters of different sizes and shapes in Vesta's southern hemisphere. The freshest craters can be classified as fresh scarp rimmed craters and the less fresh classified as partly degraded subdued rim craters.
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This image, taken by NASA's Dawn spacecraft, shows a portion of the southern rim of Jarovit Crater in the northern hemisphere of Ceres. Compacted material forms spurs along the upper part of the crater wall, near the center of the image.
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Patches of bright material can be seen on the walls of a relatively fresh crater on Ceres in this view from NASA's Dawn spacecraft.
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Another Small Volcano
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NASA's Dawn spacecraft captured this portion of the southern hemisphere of Ceres on Dec. 20, 2015. The image is centered at approximately 46 degrees south latitude, 101 degrees east longitude.
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This image, taken by NASA's Dawn spacecraft, shows dwarf planet Ceres from an altitude of 2,700 miles (4,400 kilometers). The image, with a resolution of 1,400 feet (410 meters) per pixel, was taken on June 24, 2015.
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This image from NASA's Dawn spacecraft shows the largest crater on Ceres, called Kerwan. The crater has an appearance scientists refer to as relaxed, meaning its sharp features have softened since Kerwan formed. Its overall shape looks something like a pancake, especially when viewed near Ceres' limb. The origin of its polygonal shape is not yet well understood; it might be due to large faults in the subsurface generated by other large impacts, as has been suggested for other craters. The smaller crater named Insitor sits in the center of Kerwan. The dark material seen at top right is ejecta from Dantu crater. At 174 miles (280 kilometers) wide, Kerwan is so large that it would have taken about 50 images at Dawn's low-altitude mapping orbit (called LAMO, at 240 miles or 385 kilometers altitude) to cover the crater from one side to the other. Kerwan was also too wide to fit within the camera's field of view at Dawn's high-altitude mapping orbit (called HAMO, at 915 miles, 1,470 kilomete
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Eratosthenes Central Peak
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NASA's Lunar Reconnaissance Orbiter catches the edge of Mare Moscoviense.
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Image of the Vesta Ateroid. This Dawn framing camera (FC) image of Vesta shows linear grooves and ridges in Vesta's regolith. These linear features generally run diagonally across the image from the top left to the bottom right. They are less than 1 kilometer (0.6 mile) in width and some have lengths that extend across the entire image. This image is located in Vesta's Tuccia quadrangle, in Vesta's southern hemisphere. NASA's Dawn spacecraft obtained this image on April 8, 2012.
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This image, taken by NASA's Dawn spacecraft on June 24, 2015, shows Dantu crater on dwarf planet Ceres from an altitude of 2,700 miles (4,400 kilometers); Dantu crater as small patches of bright material sprinkled around it.
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Contact between Archimedes crater wall and floor.
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This view from NASA's Dawn spacecraft shows part of the southwestern rim of Yalode Crater on Ceres. Yalode is one of the largest impact basins on Ceres. A great deal of material has slumped down the walls of the crater. a phenomenon called mass wasting.
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This view from NASA's Dawn spacecraft shows a portion of Mondamin Crater, an impact feature 78 miles (126 kilometers) in diameter, in the southern hemisphere of Ceres.
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Maximum Thrust
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NASA's Dawn spacecraft took this moody scene on Ceres, located within Zadeni Crater, named for the ancient Georgian god of bountiful harvest. Dawn saw Zadeni at approximately 76 miles (120 kilometers) in diameter on June 15, 2016.
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This image of asteroid Vesta from NASA's Dawn spacecraft shows a relatively smooth area of Vesta's surface. This region is smooth because it is mostly covered by fine-grained debris, known as regolith.
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