This image NASA's Dawn spacecraft shows is located in Vesta's Rheasilvia quadrangle, near Vesta's south pole. Severina crater has a fresh, sharp rim and a smaller, presumably younger, crater on its rim.

This image NASA's Dawn spacecraft shows is located in Vesta's Rheasilvia quadrangle, near Vesta's south pole. Severina crater has a fresh, sharp rim and a smaller, presumably younger, crater on its rim.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of This image NASA's Dawn spacecraft shows is located in Vesta's Rheasilvia quadrangle, near Vesta's south pole. Severina crater has a fresh, sharp rim and a smaller, presumably younger, crater on its rim. by Piemags/PL Photography Limited is available for licensing today.

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This image from NASA's Dawn spacecraft shows a part of the surface of asteroid Vesta, which is mantled (covered) by an ejecta blanket, evident as smoothly textured surface visible across the image.
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This image captured by NASA's Dawn spacecraft shows small craters within Meanderi Crater on Ceres, which measures 64 miles (103 kilometers) in diameter.
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A faint double ring crater is seen at upper right in this picture of Mercury taken one hour and 40 minutes before NASA's Mariner 10's second rendezvous with the planet Sept. 21, 1975
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NASA's Lunar Reconnaissance Orbiter's sees hummocks and blocks on the ejecta blanket of Tsiolkovskiy crater.
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This image, taken on June 6, 2015 by NASA's Dawn spacecraft, shows a mountain on Ceres at center-left that is 4 miles (6 kilometers) high, from an altitude of 2,700 miles (4,400 kilometers) with a resolution of 1,400 feet (410 meters) per pixel.
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This image from NASA's Dawn spacecraft shows an ejecta blanket mantling the surface and obscuring older caters. The bright crater rim, seen in the middle right edge, is one of a group of craters which are the source of this ejecta blanket.
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This image of the region between Urvara Crater's eastern rim and Yalode Crater's western rim was obtained by NASA's Dawn spacecraft on May 20, 2018 from an altitude of about 1070 miles (1720 kilometers). The center of this picture is located at about 54 degrees south in latitude and 272 degrees east in longitude.
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A wrinkle ridge within Brisbane Z crater in Mare Australe. This wrinkle ridge is located within the crater Brisbane Z.
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NASA's Dawn mission has found that craters on Ceres show a diversity of shapes that provide important clues about the structure of Ceres' subsurface; shown here is Fejokoo, a polygonal crater.
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This scene viewed by NASA's Dawn spacecraft on Oct. 20, 2016, from Ceres features terrain near the rim of the large crater named Kerwan, at lower left. A much smaller, fresher crater called Cacaguat is seen in the lower right corner.
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NASA's Dawn spacecraft obtained this view of Azacca Crater on Ceres. The rim of this crater has terraces descending from its rim down to its floor. The crater's floor is relatively free of large impact scars and is named for the Haitian god of agriculture
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Textured Terrain
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Final Eros Images: Range 1,150 meters (3,773 feet)
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This view from NASA's Dawn spacecraft captures the northern rim of Toharu Crater on Ceres. Dawn captured the scene on Dec. 24, 2015 from its low-altitude mapping orbit (LAMO), at an approximate altitude of 240 miles (385 kilometers) above Ceres.
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One of the most prominent lobate scarps (Discovery Scarp), photographed by NASA's Mariner 10 during it's first encounter with Mercury, is located at the center of this image (extending from the top to near bottom).
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This image, taken by NASA's Dawn spacecraft, shows a portion of the northern hemisphere of dwarf planet Ceres from an altitude of 915 miles (1,470 kilometers). The image was taken on Sept. 22, 2015, and has a resolution of 450 feet (140 meters) per pixel.
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This Dawn framing camera (FC) image of the Asteroid Vesta, shows the Arruntia crater, which is the large crater offset to the top right of the center of the image. Slightly over half of Arruntia crater is covered in a large shadow. But, the non-shadowed part of Arruntia shows impressive details. There is bright material cropping out slightly below the left rim and just below the top and bottom rims there are distinct ridges of material, which are probably formed by material from the rim cascading down towards the center of Arruntia. This image is located in Vesta's Bellicia quadrangle, in Vesta's northern hemisphere. NASA's Dawn spacecraft obtained this image with its framing camera on Oct. 24, 2011.
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Where the Craters Have No Name
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This image, taken by NASA's Dawn spacecraft, shows a portion of the southern hemisphere of dwarf planet Ceres from an altitude of 915 miles (1,470 kilometers). Urvara crater, named for the Indian and Iranian deity of plants and fields, is featured.
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This image from NASA's Dawn spacecraft shows a portion of Ceres known as Erntedank Planum, a broad plateau 345 miles (555 kilometers) wide. The terrain seen here lies just to the southeast of Occator Crater, home of Ceres' brightest region.
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Image Number: 6145-44881014Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Asteroid and Planetary SurfacesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1024×1024
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