This image shows the final flight path for NASA's twin Gravity Recovery and Interior Laboratory (GRAIL) mission spacecraft, which will impact the moon on Dec. 17, 2012, around 2:28 p.m. PST.

This image shows the final flight path for NASA's twin Gravity Recovery and Interior Laboratory (GRAIL) mission spacecraft, which will impact the moon on Dec. 17, 2012, around 2:28 p.m. PST.
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of This image shows the final flight path for NASA's twin Gravity Recovery and Interior Laboratory (GRAIL) mission spacecraft, which will impact the moon on Dec. 17, 2012, around 2:28 p.m. PST. by Piemags/PL Photography Limited is available for licensing today.

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These images from NASA's Dawn spacecraft shows a region around the asteroid Vesta's equatorial troughs with two different resolutions. More details are visible in the right-hand image such as small linear grooves running roughly parallel to the troughs.
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These images from NASA's Dawn spacecraft show many craters, which have different states of preservation, in Vesta's Bellicia quadrangle in the northern hemisphere.
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These images from NASA's Dawn spacecraft show part of asteroid Vesta's equatorial region, which contains a prominent, deep impact crater (lower center of images) and large troughs (linear depressions).
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NASA's Dawn spacecraft obtained this albedo image of asteroid Vesta with its framing camera on August 11th 2011.
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This map of Ceres, made from images taken by NASA's Dawn spacecraft, shows the locations of about 130 bright areas across the dwarf planet's surface, highlighted in blue. Most of these bright areas are associated with craters.
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These images from NASA's Dawn spacecraft are located in asteroid Vesta's Marcia quadrangle, a few degrees below Vesta's equator. Octavia Crater looks remarkably like a terrestrial landslide.
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NASA's Dawn spacecraft shows the central area of the south polar basin. This view is rotated by approximately 90°.
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These images from NASA's Dawn spacecraft are located in asteroid Vesta's Lucaria Tholus quadrangle, in Vesta's southern hemisphere.
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This image from NASA's Mars Odyssey spacecraft shows part of Ganges Chasma in Valles Marineris. The colors indicate compositional variations in the rocks exposed in the wall and floor of Ganges and in the dust and sand on the rim of the canyon.
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These images from NASA's Dawn spacecraft show Oppia crater on asteroid Vesta, after which Oppia quadrangle is named. Oppia crater is a distinctive crater because it has an unusually shaped rim, which is almost rectangular in form.
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These images from NASA's Dawn spacecraft show Sextilia crater on asteroid Vesta.
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Map of Mars' Topography
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These images from NASA's Dawn spacecraft show Pinaria crater on asteroid Vesta, after which Pinaria quadrangle is named. Many young fresh impact craters are visible on the slumped material.
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NASA's Dawn spacecraft shows the central area of the south polar basin. This view is rotated by approximately 60°.
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This image shows Cornelia Crater on the large asteroid Vesta. On the right is an inset image showing an example of curved gullies, indicated by the short white arrows, and a fan-shaped deposit, indicated by long white arrows.
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Image Number: 6145-44918485Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Asteroid Surfaces and CratersContributor:PiemagsModel Release:NoProperty Release:NoResolution:1280×720
Gravity Recovery and Interior Laboratory (GRAIL),Lunar Reconnais
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