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This mosaic from NASA's Magellan spacecraft shows an area of the Lakshmi region on Venus. It is known that this region is located on the low rise that separates Sedna Planitia and Guinevere Planitia, just to the west of Eistla Regio.
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This view of the surface of Venus acquired by NASA Magellan spacecraft shows a geographically young region of lowland plains. The location is near the equator between two highland areas known as Asteria Regio and Phoebe Regio.
Ver en NASA ↗These two radar images from NASA Magellan spacecraft are centered about 60.5 degrees south latitude and 348.8 degrees east longitude in the eastern Lavinia Region of Venus.
Ver en NASA ↗Three impact craters are displayed in this three-dimensional perspective view from NASA Magellan spacecraft of the surface of Venus. The center of the image is located in the northwestern portion of Lavinia Planitia.
Ver en NASA ↗This radar image mosaic of Venus from NASA Magellan spacecraft, is in the Lada region. The mosaic shows a system of east-trending radar-bright and dark lava flows encountering and breaching a north-trending ridge belt left of center.
Ver en NASA ↗This image from NASA Magellan spacecraft is from the eastern Ovda region of Venus. The image shows some small volcanic domes on the flank of the volcano Maat.
Ver en NASA ↗Venus is seen as disappears behind the Moon, at the start of occultation, on Wednesday, June 17, 2026, from the Mary W. Jackson NASA Headquarters building in Washington. The Moon occulted, or passed in front of, Venus for the first of three time this year. P…
Ver en NASA ↗Venus is seen as disappears behind the Moon, at the start of occultation, on Wednesday, June 17, 2026, from the Mary W. Jackson NASA Headquarters building in Washington. The Moon occulted, or passed in front of, Venus for the first of three time this year. P…
Ver en NASA ↗Venus is seen, during daylight, as it disappears behind the Moon, at the start of occultation, on Wednesday, June 17, 2026, from the Mary W. Jackson NASA Headquarters building in Washington. The Moon occulted, or passed in front of, Venus for the first of thr…
Ver en NASA ↗This full resolution mosaiced image from NASA Magellan spacecraft is located in the Lakshmi region of Venus at 47 degrees north latitude and 334 east longitude.
Ver en NASA ↗NASA Magellan full-resolution image shows Maxwell Montes, centered at 65 degrees north latitude and 6 degrees east longitude. Maxwell is the highest mountain on Venus, rising almost 11 kilometers 6.8 miles above mean planetary radius.
Ver en NASA ↗It appeared that New Yorkers were not going to be able to see the transit of the planet Venus across the Sun, but just before the transit was over the sun broke through the clouds and Yvette Lee Kang was able to catch a glimpse of the transit on Tuesday, June…
Ver en NASA ↗The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA 1990-1994 Magellan mission, is centered at 0 degrees east longitude.
Ver en NASA ↗The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA 1990-1994 Magellan mission, is centered at 90 degrees east longitude.
Ver en NASA ↗This radar image from NASA Magellan spacecraft is of a half crater located in the rift between Rhea and Theia Montes in Beta Regio on Venus and has been cut by many fractures or faults since it was formed by the impact of a large asteroid.
Ver en NASA ↗This image is a false color version of a near infrared map of lower level clouds on the night side of Venus, obtained by the Near Infrared Mapping Spectrometer aboard NASA's Galileo spacecraft as it approached the planet Feb. 10, 1990.
Ver en NASA ↗These images are two versions of a near-infrared map of lower-level clouds on the night side of Venus, obtained by the Near Infrared Mapping Spectrometer aboard NASA Galileo spacecraft as it approached the planet February 10, 1990.
Ver en NASA ↗The northern hemisphere is displayed in this global view of the surface of Venus. NASA Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping were mapped onto a computer-simulated globe to create this image.
Ver en NASA ↗These images are two versions of a near-infrared map of lower-level clouds on the night side of Venus, obtained by the Near Infrared Mapping Spectrometer aboard NASA Galileo spacecraft as it approached the planet February 10, 1990.
Ver en NASA ↗Leslie Lowes from the NASA Jet Propulsion Laboratory in Pasadena, Calif., views the June 5, 2012, Venus transit through a solar telescope. Lowes participated in an education workshop at the INFINITY at NASA Stennis Space Center visitor center and joined other…
Ver en NASA ↗Guests at the INFINITY at NASA Stennis Space Center visitor center use special solar sunglasses to catch a lifetime view of the Venus transit June 5, 2012. The rare celestial event in which the planet Venus traverses the face of the sun will not be visible fr…
Ver en NASA ↗Leslie Lowes from the NASA Jet Propulsion Laboratory in Pasadena, Calif., views the June 5, 2012, Venus transit through a solar telescope. Lowes participated in an education workshop at the INFINITY at NASA Stennis Space Center visitor center and joined other…
Ver en NASA ↗Leslie Lowes from the NASA Jet Propulsion Laboratory in Pasadena, Calif., views the June 5, 2012, Venus transit through a solar telescope. Lowes participated in an education workshop at the INFINITY at NASA Stennis Space Center visitor center and joined other…
Ver en NASA ↗Guests at the INFINITY at NASA Stennis Space Center visitor center use special solar sunglasses to catch a lifetime view of the Venus transit June 5, 2012. The rare celestial event in which the planet Venus traverses the face of the sun will not be visible fr…
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.