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This image from NASA Magellan spacecraft is of Crater Stephania in northern Sedna Planitia on Venus. It is one of the smaller craters on Venus.
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This portion of NASA Magellan radar image strip shows a small region on Venus 20 kilometers 12.4 miles wide and 75 km 50 miles long on the east flank of a major volcanic upland called Beta Regio.
Ver en NASA ↗Many of the impact craters of Venus revealed by NASA Magellan spacecraft have characteristics unlike craters on any other planetary body. This crater, named Adivar, is located just north of the western Aphrodite highland.
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 ↗Ushas Mons, a volcano in the southern hemisphere of Venus is shown in this radar image from NASA Magellan spacecraft. The volcano is marked by numerous bright lava flows and a set of north-south trending fractures.
Ver en NASA ↗This false color image from NASA Magellan spacecraft shows a portion of Leda Planitia plains in the northern hemisphere of Venus, centered at 41 degrees north latitude, 52 degrees east longitude.
Ver en NASA ↗This false-color image is a near-infrared map of lower-level clouds on the night side of Venus, obtained by NASA Galileo spacecraft as it approached the planet night side on Feb. 10, 1990.
Ver en NASA ↗Observations of the total solar irradiance made with the ACRIM3 instrument on NASA ACRIMSAT satellite on June 5 and 6, 2012, tracked the effect of the transit of Venus, which lasted about six hours.
Ver en NASA ↗This false color Magellan image shows a portion of Eistla Regio region in the northern hemisphere of Venus, centered at 1 degrees south latitude, 37 degrees east longitude.
Ver en NASA ↗This mosaic of NASA Magellan data in the Fortuna region of Venus, centered at 49 degrees north latitude, 2 degrees longitude, shows two coronae. Coronae are large circular or oval structures first identified in Soviet radar images 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 hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered on the North Pole. NASA Magellan spacecraft imaged more than 98% of Venus.
Ver en NASA ↗NASA Magellan radar image shows Alpha Regio, a topographic upland. In 1963 Alpha Regio was the first feature on Venus to be identified from Earth based radar.
Ver en NASA ↗A portion of western Eistla Regio is shown in this three dimensional, computer-generated view of the surface of Venus. This NASA Magellan image was released on April 22, 1992.
Ver en NASA ↗The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 180 degrees east longitude.
Ver en NASA ↗Maat Mons is displayed in this 3-dimensional perspective view of the surface of Venus taken by NASA Magellan. The viewpoint is located north of Maat Mons.
Ver en NASA ↗The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 270 degrees east longitude.
Ver en NASA ↗These two images of Venus from NASA Galileo spacecraft show the global structure of cloud patterns at two different depths in the upper cloud layers.
Ver en NASA ↗Maat Mons is displayed in this computer generated three-dimensional perspective of the surface of Venus. This NASA Magellan image was released on April 22, 1992.
Ver en NASA ↗NASA Magellan image mosaic shows the largest impact crater known to exist on Venus at this point in the Magellan mission. The crater is located north of Aphrodite Terra and east of Eistla Regio and was imaged during orbit 804 on November 12, 1990.
Ver en NASA ↗This global view from NASA Magellan spacecraft is of the surface of Venus is centered at 180 degrees east longitude.
Ver en NASA ↗This computer-generated perspective view of Latona Corona and Dali Chasma on Venus shows NASA Magellan radar data superimposed on topography.
Ver en NASA ↗A portion of the eastern edge of Alpha Regio is displayed in this three-dimensional perspective view of the surface of Venus from NASA Magellan spacecraft.
Ver en NASA ↗This image is a mosaic of 24 orbits of the Navka region of Venus. 'Behepa 8' marks the approximate landing site of the Soviet Venera 8 lander, which took measurements at the surface of Venus in 1972.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.