This image of Ceres, taken by NASA's Dawn spacecraft, shows cratered terrain at high northern latitudes. Ghanan Crater is seen at upper-right. A distinctive flow feature extends into the crater from its northern rim.

This image of Ceres, taken by NASA's Dawn spacecraft, shows cratered terrain at high northern latitudes. Ghanan Crater is seen at upper-right. A distinctive flow feature extends into the crater from its northern rim.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of This image of Ceres, taken by NASA's Dawn spacecraft, shows cratered terrain at high northern latitudes. Ghanan Crater is seen at upper-right. A distinctive flow feature extends into the crater from its northern rim. by Piemags/PL Photography Limited is available for licensing today.

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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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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 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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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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Image Number: 6145-45101528Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Lunar and Ceres Surface FeaturesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1024×1024
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