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Venus. September 23, 1996 - This global view of the surface of Venus is
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Venus. September 23, 1996 - This global view of the surface of Venus is
September 23, 1996 - This global view of the surface of Venus is centered at 90 degrees east longitude. Magellan synthetic aperture radar mosaics from the three eight-month cycles of Magellan radar mapping are mapped onto a computer-simulated globe to create this image. Magellan obtained coverage of 98 percent of the surface of Venus. Remaining gaps are filled with data from previous Venus missions, the Venera 15 and 16 radar and Pioneer-Venus Orbiter altimetry, and data from Earth-based radar observations from the Arecibo radio telescope. Simulated color is used to enhance small-scale structures. The simulated hues are based on color images obtained by the Venera 13 and 14 landing craft. The bright feature near the center of the image is Ovda Regio, a mountainous region in the western portion of the great Aphrodite equatorial highland. The dark areas scattered across the Venusian plains consist of extremely smooth deposits associated with large meteorite impacts
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Circle Composite Crater Deposit Equator Full Geography Geology Global Globe Highlands Impact Impact Craters Land Feature Landform Meteor Meteorite Meteoroid Mosaic Mountainous Plains Regions Round Solar System Sphere Square Image Surface Terrain Territory Texture Topography Venus Venusian View From Space
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This stunning print captures a global view of the enigmatic planet Venus, taken on September 23,1996. Created using synthetic aperture radar mosaics from the Magellan mission, this composite image provides an unprecedented glimpse into Venus' surface. The Magellan radar mapping covered an impressive 98 percent of the planet's terrain, with remaining gaps filled by data from previous missions and Earth-based observations. Enhanced with simulated color based on images obtained by Venera landing craft, this print showcases intricate small-scale structures across Venus' landscape. At its center lies Ovda Regio, a mountainous region within the Aphrodite equatorial highland – a bright feature that captivates viewers. The dark areas scattered throughout the plains are smooth deposits resulting from massive meteorite impacts over time. These impact craters contribute to Venusian geology and add depth to its unique topography. Displayed in a square format, this print offers a comprehensive visual representation of Venus' spherical shape and diverse land features. With no people present in the frame, it allows us to appreciate the beauty and complexity of our neighboring planet as seen from space. A true testament to human exploration and scientific achievement, this image serves as a reminder of our ongoing quest for knowledge about our solar system's celestial bodies.
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