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This image from NASA Magellan spacecraft shows part of the northern boundary of Ovda Regio, one of the large highlands ringing the equator of Venus.
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This full resolution radar mosaic from NASA Magellan spacecraft shows a 200 kilometer 124 mile segment of a sinuous channel on Venus.
Ver en NASA ↗Sif Mons is displayed in this computer-simulated view obtained by NASA's Magellan spacecraft of the surface of Venus.
Ver en NASA ↗A corona is displayed in this computer-simulated view from NASA Magellan spacecraft of the surface of Venus.
Ver en NASA ↗Gula Mons is displayed in this computer-simulated view from NASA Magellan spacecraft of the surface of Venus.
Ver en NASA ↗The northern hemisphere is displayed in this global view of the surface of Venus as seen by NASA Magellan spacecraft.
Ver en NASA ↗This colorized picture of Venus was taken Feb. 14, 1990, from a distance of almost 1.7 million miles, about 6 days after NASA Galileo made it closest approach to the planet.
Ver en NASA ↗This image from NASA 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.
Ver en NASA ↗This area of Venus northeast of Ushas Mons measures 40 by 112 kilometers 25 by 70 miles and shows evidence of possible explosive volcanism as seen by NASA Magellan spacecraft.
Ver en NASA ↗The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.
Ver en NASA ↗This radar image from NASA Magellan is of part of the Phoebe region of Venus. It is a mosaic of parts of revolutions 146 and 147 acquired in the first radar test on Aug. 16, 1990.
Ver en NASA ↗This radar image from NASA Magellan is of part of the Phoebe region of Venus. It is a mosaic of parts of revolutions 146 and 147 acquired in the first radar test on Aug. 16, 1990.
Ver en NASA ↗NASA MESSENGER spacecraft snapped a series of images as it approached Venus on June 5. The planet is enshrouded by a global layer of clouds that obscures its surface to the MESSENGER Dual Imaging System MDIS cameras.
Ver en NASA ↗Crater Isabella is seen in this radar image from NASA Magellan spacecraft. The second largest impact crater on Venus, the crater is named in honor of the 15th Century queen of Spain, Isabella of Castile.
Ver en NASA ↗After acquiring hundreds of high-resolution images during close approach to Venus, NASA MESSENGER turned its wide-angle camera back to the planet and acquired a departure sequence.
Ver en NASA ↗The eastern half of the planet is displayed in this simple cylindrical map of the surface of Venus obtained by NASA Magellan spacecraft.
Ver en NASA ↗The western half of the planet is displayed in this simple cylindrical map of the surface of Venus obtained by NASA Magellan spacecraft.
Ver en NASA ↗A portion of western Eistla Regio is displayed in this three-dimensional perspective view from NASA Magellan spacecraft of the surface of Venus.
Ver en NASA ↗Sapas Mons is displayed in the center of this computer-generated three-dimensional perspective view from NASA Magellan spacecraft of the surface of Venus.
Ver en NASA ↗A portion of western Eistla Regio is displayed in this three-dimensional perspective view of the surface of Venus as seen by NASA Magellan spacecraft.
Ver en NASA ↗This synthetic aperture radar mosaic from NASA Magellan spacecraft is a global view of the surface of Venus.
Ver en NASA ↗As it sped away from Venus, NASA's Mariner 10 spacecraft captured this seemingly peaceful view of a planet the size of Earth, wrapped in a dense, global cloud layer.
Ver en NASA ↗This image from the Atla region of Venus obtained by NASA Magellan spacecraft shows several types of volcanic features and superimposed surface fractures.
Ver en NASA ↗This picture of Venus was taken by the NASA Galileo spacecraft Solid State Imaging System on February 14, 1990, at a range of almost 1.7 million miles from the planet.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.