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This image from NASA Dawn spacecraft shows numerous linear chains and clusters of small craters on asteroid Vesta. These chains and clusters of craters were created by material that was ejected during the formation of a large crater.
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These images from NASA Dawn spacecraft, located in asteroid VestaFloronia quadrangle, in Vesta northern hemisphere, demonstrate a special analytical technique, which results in shadowed areas of Vesta surface becoming illuminated.
Ver en NASA ↗These two images taken one day apart by the MARCI weather camera on NASA Mars Reconnaissance Orbiter reveal when an asteroid impact made the scar seen in the right-hand image.
Ver en NASA ↗These images from NASA Dawn spacecraft are located in asteroid Vesta Numisia quadrangle, southern hemisphere; layers can be seen slumping towards the crater center and there is slightly brighter material overlying slightly less bright material.
Ver en NASA ↗This image from NASA Dawn spacecraft shows a young, fresh crater, which is about 7 km in diameter, on asteroid Vesta. This crater has both dark and bright rays fanning out from it.
Ver en NASA ↗This image from NASA Dawn spacecraft shows a large crater with several smaller craters at the edge on the giant asteroid Vesta. Rough texture in the crater wall at far right may be the underlying bedrock.
Ver en NASA ↗This image from NASA Dawn spacecraft of asteroid Vesta shows Aquilia crater located in Pinaria quadrangle, in Vesta southern hemisphere. The especially degraded bottom rim was probably formed by debris slumping into the crater.
Ver en NASA ↗This image from NASA Mars Mars Reconnaissance Orbiter shows a triple impact crater in Elysium Planitia near Tartarus Montes, which probably formed when a binary-or even triple-asteroid struck the surface.
Ver en NASA ↗These images from NASA Dawn spacecraft, located in asteroid Vesta Marcia quadrangle, in Vesta northern hemisphere, demonstrate a special analytical technique, which results in shadowed areas of Vesta surface becoming illuminated.
Ver en NASA ↗This colorized image from the visible and infrared mapping spectrometer onboard NASA Dawn spacecraft shows temperature variations at Tarpeia crater, near the south pole of the giant asteroid Vesta.
Ver en NASA ↗This anaglyph image from NASA Dawn spacecraft shows the topography of the mountain-central complex in asteroid Vesta south polar region. You need 3D glasses to view this image.
Ver en NASA ↗In this image from NASA Dawn spacecraft, bright material extends out from the crater Canuleia on asteroid Vesta. The bright material appears to have been thrown out of the crater during the impact that created it.
Ver en NASA ↗This non-circular pit seen in this image from NASA Mars Reconnaissance Orbiter is due to a low angle impact from an asteroid or comet. The raised plateau west of the crater was where most of the impact debris landed.
Ver en NASA ↗This composite-color view from NASA Dawn mission shows Cornelia Crater, streaked with dark materials, on the giant asteroid Vesta. You need 3D glasses to view this image.
Ver en NASA ↗These images from NASA Dawn spacecraft are located in asteroid Vesta Numisia quadrangle, in Vesta northern hemisphere. The bottom part of the rim of Fabia crater is much fresher than the top part of the rim.
Ver en NASA ↗This is the first global map of the giant asteroid Vesta composed from images recorded by the framing camera aboard NASA Dawn spacecraft. The equator is running parallel to the upper image border, approximately above the bright, smooth band of troughs.
Ver en NASA ↗This image of asteroid Vesta from NASA Dawn spacecraft shows an area of the surface that is both grooved and smooth, which gives it an undulating appearance. This image is located in Vesta Numisia quadrangle, near the Vestan equator.
Ver en NASA ↗This image from NASA Dawn spacecraft of asteroid Vesta shows Helena crater, which is the crater that resembles the shape of a butterfly wings center, and Laelia crater bottom right.
Ver en NASA ↗These images from NASA Dawn spacecraft show Gegania crater on asteroid Vesta, after which Gegania quadrangle is named. The image at left shows the albedo brightness/darkness of the surface.
Ver en NASA ↗NASA Dawn spacecraft has spiraled closer and closer to the surface of the giant asteroid Vesta. These images were obtained by Dawn framing camera in the three phases of its campaign since arriving at Vesta in mid-2011.
Ver en NASA ↗This image from NASA Dawn spacecraft shows a sharp, fresh crater rim of a large crater that is only partly in the bottom right corner of this image and is located in Vesta Numisia quadrangle, near asteroid Vesta equator.
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 shows the brightest area seen on asteroid Vesta so far. It shows a crater located inside the rim of the Rheasilvia basin at the south pole of Vesta.
Ver en NASA ↗Many types of craters exist on Mars. Most are generated by impacts of asteroids and comets. However, in this image captured by NASA Mars Reconnaissance Orbiter, the craters may be due to steam explosions.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.