This image of asteroid Vesta, from NASA's Dawn spacecraft, calculated from a shape model, shows a tilted view of the topography of the south polar region. This perspective removes the overall curvature of Vesta, as if the giant asteroid were flat and not

This image of asteroid Vesta, from NASA's Dawn spacecraft, calculated from a shape model, shows a tilted view of the topography of the south polar region. This perspective removes the overall curvature of Vesta, as if the giant asteroid were flat and not
SuperStock offers millions of photos, videos, and stock assets to creatives around the world. This image of This image of asteroid Vesta, from NASA's Dawn spacecraft, calculated from a shape model, shows a tilted view of the topography of the south polar region. This perspective removes the overall curvature of Vesta, as if the giant asteroid were flat and not by Piemags/PL Photography Limited is available for licensing today.

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Kepler's Rim
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This image from NASA's Mars Reconnaissance Orbiter spacecraft contains interesting examples of crosscutting, sinuous and straight ridges. Both ridges may be ancient river deposits.
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The North Polar layered deposits (NPLD) are a stack of layers of ice and dust at the North Pole of Mars. The layers are thought to have been deposited over millions of years. This image is from NASA's Mars Reconnaissance Orbiter.
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During periods in Mars' history when the planet had greater axial tilt, shifts in atmospheric circulation may have favored the extensive accumulation of snow in some locations. Protonilus Mensae is just such a site of extensive glaciation. We can see a flow of material through the valleys between a complex of small mesas. Streamlines and flow fronts appear as subtle ridges. Some ridges appear perpendicular to the mesas indicating flow direction. Others appear concentric to the mesas and parallel to the valleys, where debris and now-underlying ice bunched up and moved down valley. Deflation of the ice has led to a rich collection of small-scale features. Polygonal patterns of fractures and fissures may be related to a combination of thermal contraction cycles and overall subsidence of the surface. Larger fractures may be glacial crevasses, caused by differential flow rates in the underlying ice. Other more complex patterns of swirled pits and hummocks may result from the continual loss
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Ancient Paleo-Dunes Battered by Impact Craters
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Image Number: 6145-45016548Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Martian Geological FeaturesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1500×600
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