These images from NASA's Dawn spacecraft are located in asteroid Vesta's Numisia quadrangle, a few degrees below Vesta's equator.

These images from NASA's Dawn spacecraft are located in asteroid Vesta's Numisia quadrangle, a few degrees below Vesta's equator.
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This high resolution image taken by NASA's Lunar Reconnaissance Orbiter shows the floor of the Apollo Basin, a large (538 km diameter) double-ringed impact crater in the southern hemisphere of the far side.
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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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An Eraser Mark on Eros
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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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