A Study in Contrasts

A Study in Contrasts
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Meridiani Outcrops
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This image from NASA's Magellan shows part of the interior of Ovda Regio, one of the large highlands ringing the equator of Venus. Several tectonic events formed this complex block fractured terrain.
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Rivers of Xanadu on Titan
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Polar Polygon Patterns
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Polygon/Cracked Sedimentary Rock
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Tectonic Features
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NASA's Cassini spacecraft surveys the surface of Saturn's moon Enceladus in this image, which shows newly created terrain in the upper right meeting older, cratered terrain in the lower left.
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February 10, 2004 - This full-resolution Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows details on the floor of an ancient meteor crater in the northeastern part of Noachis Terra. After the crater formed, layers of material, perhaps sediment, were deposited in the crater. These materials became somewhat solidified, but later were eroded to form the patterns shown here. Many windblown ripples in the scene indicate the presence of coarse-grained sediment that was not completely s
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During its final close flyby of Saturn's moon Enceladus, NASA's Cassini orbiter shows this view featuring the nearly parallel furrows and ridges of the feature named Samarkand Sulci.
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Europa Triple Band
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The shallow, scalloped depression in the center of this picture from NASA's Galileo spacecraft is a caldera-like feature 5 to 20 kilometers wide on Jupiter's largest moon, Ganymede. Galileo.
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Meridiani Sedimentary Rocks
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Close-up of Europa's Surface
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This close-up image of the Vinalia Faculae in Occator Crater was obtained by NASA's Dawn spacecraft on June 14, 2018 from an altitude of about 24 miles (39 kilometers). This image reveals the intricate pattern between bright and dark material across this flow feature. The complex structure of the dark background is reminiscent of lava flows observed on Earth. However, in the case of Ceres, the flow material likely involved a lot of ice. The bright material is mostly composed of sodium carbonate, a salt whose exposure onto the crater floor involved a liquid source. The center of this picture is located at about 21.0 degrees north latitude and 241.3 degrees east longitude.
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Stair-step Scarps in Dark Terrain on Ganymede
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Southwest Lakshmi Planum (plains) is bounded on the south by the Danu Montes (mountains) as shown by NASA's Magellan spacecraft.
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This electron microscope image shows tubular structures of likely Martian origin. These structures are very similar in size and shape to extremely tiny microfossils found in some Earth rocks.
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This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a spectacular summertime view of a portion of the south polar residual cap
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North Polar Dune Patterns
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Toe of Ganges Chasma Landslide ( 8.0 S, 44.4W)
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In this image taken by NASA's Cassini radar system, a previously unseen style of lakes is revealed. The lakes here assume complex shapes and are among the darkest seen so far on Titan.
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DETAILS
Image Number: 6145-44918456Royalty FreeCredit Line:Piemags/PL Photography Limited/SuperStockCollection:PL Photography LimitedStory:Planetary Surface TexturesContributor:PiemagsModel Release:NoProperty Release:NoResolution:1020×1024
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