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A double crater, called a crater doublet, is seen in the bottom right part of this image from NASA Dawn spacecraft of asteroid Vesta. This crater doublet was likely formed by the simultaneous impact of two fragments of a split projectile.
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These images from NASA Dawn spacecraft are located in asteroid Vesta Lucaria Tholus quadrangle, in Vesta northern hemisphere; the fine-scale of streaks of bright and dark material can be seen originating from the rim of Publicia crater.
Ver en NASA ↗These images from NASA Dawn spacecraft are located in asteroid Vesta Floronia quadrangle, in Vesta northern hemisphere. Licinia is the large, bowl shaped crater in the center with a sharp rim, which has a scalloped edge.
Ver en NASA ↗This colorful composite image from NASA Dawn mission shows the flow of material inside and outside a crater called Aelia on the giant asteroid Vesta. To the naked eye, these structures would not be seen. But here, they stand out in blue and red.
Ver en NASA ↗This image shows a close-up of long, narrow, sinuous gullies that scientists on NASA Dawn mission have found on the giant asteroid Vesta. The crater shown here is called Cornelia.
Ver en NASA ↗This image from NASA Dawn spacecraft show a slightly curved chain of small craters in the bottom half of the image. This chain is located on the floor of asteroid Vesta large south-polar impact structure, Rheasilvia.
Ver en NASA ↗This image of asteroid Vesta from NASA Dawn spacecraft shows a relatively smooth area of Vesta surface. This region is smooth because it is mostly covered by fine-grained debris, known as regolith.
Ver en NASA ↗NASA Dawn spacecraft obtained this image of asteroid Vesta with its framing camera on Aug. 28, 2011. This image of the south polar region was taken through the camera clear filter at a distance of 1,700 miles 2,740 kilometers.
Ver en NASA ↗This image from the framing camera aboard NASA Dawn spacecraft shows surface details beginning to resolve as the spacecraft closes in on the giant asteroid Vesta on June 1, 2011, from a distance of about 300,000 miles 483,000 kilometers.
Ver en NASA ↗This first image of asteroid 951 Gaspra was taken by NASA Galileo spacecraft on October 29, 1991, from a distance of 16,200 kilometers 10,000 miles. The Sun is shining from the right.
Ver en NASA ↗This image from NASA Dawn spacecraft shows Cornelia crater on asteroid Vesta with a sharp, fresh rim. Cornelia crater has a spectacular internal structure, which consists of bright and dark material.
Ver en NASA ↗This false-color image obtained by NASA Dawn spacecraft shows a crater on the giant asteroid Vesta. The reddish coloring below the crater points to material that was hurled from Vesta interior during an impact or originated from the impactor itself.
Ver en NASA ↗This image of a dark-rayed impact crater and several dark spots was obtained by NASA Dawn spacecraft. The dark materials are located near an older, larger crater in the Sextilia quadrangle of asteroid Vesta southern hemisphere.
Ver en NASA ↗The left-hand image from NASA Dawn spacecraft shows the apparent brightness of asteroid Vesta surface. The right-hand image is based on this apparent brightness image, with a color-coded height representation of the topography overlain onto it.
Ver en NASA ↗This 3D image of the asteroid Vesta was taken on July 9, 2011 by the framing camera instrument aboard NASA Dawn spacecraft. You need 3D glasses to view this image.
Ver en NASA ↗This color-coded topography map from NASA Dawn mission shows the giant asteroid Vesta in an equirectangular projection at 32 pixels per degree, relative to an ellipsoid of 177 miles by 177 miles by 142 miles.
Ver en NASA ↗NASA Dawn spacecraft obtained this image of a central mound in a large structure at the south pole of asteroid Vesta with its framing camera on August 12, 2011. This image was taken through the camera clear filter.
Ver en NASA ↗These images from NASA Dawn spacecraft show Lucaria Tholus on asteroid Vesta, after which Lucaria quadrangle is named. Lucaria Tholus is the large, roughly elliptically shaped hill in the center of the image.
Ver en NASA ↗This image from NASA Dawn spacecraft of asteroid Vesta shows Sossia and Canuleia craters. Sossia is surrounded by dark material in the bottom left of the image and Canuleia is the larger crater surrounded by bright material at bottom right.
Ver en NASA ↗This composite image is a simulated true color image of part of asteroid Vesta northern region, which contains the nowman craters. Images such as these greatly help the process of understanding Vesta geological history.
Ver en NASA ↗These images from NASA Dawn spacecraft are located in asteroid Vesta Oppia quadrangle, just south of Vesta equator; Claudia was chosen to anchor the coordinate system for Vesta used in the scientific investigations of the Dawn team.
Ver en NASA ↗The impact of an asteroid or comet several hundred million years ago left scars in the landscape that are still visible in this spaceborne radar image of an area in the Sahara Desert of northern Chad.
Ver en NASA ↗These images from NASA Dawn spacecraft are located in asteroid Vesta Numisia quadrangle, in Vesta southern hemisphere. fine-scale structure of the slumping-related features on Drusilla sloping sides.
Ver en NASA ↗These images from NASA Dawn spacecraft are located in asteroid Vesta Numisia quadrangle, just south of Vesta equator; there is a large slump of material covering the top rim of Teia crater, which makes it appear degraded.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.