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…
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To read more about the 2012 Venus Transit go to: sunearthday.nasa.gov/transitofvenus Add your photos of the Transit of Venus to our Flickr Group here: www.flickr.com/groups/venustransit/ NASA FILE PHOTO Date: 8 Jun 2004 NASA's TRACE satellite captured …
Ver en NASA ↗This color image of the sun, Earth and Venus was taken by the Voyager 1 spacecraft Feb. 14, 1990, when it was approximately 32 degrees above the plane of the ecliptic and at a slant-range distance of approximately 4 billion miles.
Ver en NASA ↗These radar images show an identical area on Venus (centered at 110 degrees longitude and 64 degrees north latitude) as imaged by the U.S. NASA Magellan spacecraft in 1991 (left) and the U.S.S.R. Venera 15/16 spacecraft in the early 1980's (right).
Ver en NASA ↗This image from NASA Magellan spacecraft is in the Lavinia Region of Venus. Volcanic vent areas in this part of the plains west of Alpha Regio consist of domes and pits up to nearly 3 kilometers across.
Ver en NASA ↗This image from NASA Magellan spacecraft is of the eastern Navka Region of Venus. The crater, which is approximately 8 kilometers 5 miles in diameter, displays a butterfly symmetry pattern.
Ver en NASA ↗As NASA Magellan mission progressed, areas of Venus became accessible for a second look. During Magellan second 243-day global mapping cycle, the spacecraft was rotated 180 degrees to view the surface from the opposite direction.
Ver en NASA ↗This image compares NASA Magellan data acquired in August 1990 during the initial test of the radar system black and white insets with data acquired by the spacecraft in April 1991 color background. The area is in the southern hemisphere of Venus.
Ver en NASA ↗This global view of the surface of Venus is centered at 0 degrees east longitude. 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 ↗Transit of Venus as seen at 762nm in the CO Module. This image is from NASA Astronaut Don Petttit shot from onboard the International Space Station on June 5, 2012. Petttit, who had the foresight to bring a solar filter for his camera, will be capturing the…
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 Liz Heller and Andriel Mesznik were able to catch a glimpse of the transit …
Ver en NASA ↗This perspective view of Venus, generated by computer from NASA Magellan data and color-coded with emissivity, shows part of Sedna Planitia and illustrates a common phenomenon of the lowland plains of Venus.
Ver en NASA ↗This perspective view of Ishtar Terra was derived from data obtained by NASA Pioneer Venus spacecraft altimetry radar instrument.
Ver en NASA ↗This crater in the Navka region of Venus was mapped by NASA Magellan on Sept. 26-27, 1990 during orbits 459 and 460. It has the terraced walls, flat radar-dark floor, and central peak that are characteristic of craters classified as complex.
Ver en NASA ↗This image from NASA Magellan spacecraft is from the northeastern Atalanta Region of Venus. The image shows the complex impact crater, Dickinson, characterized by a partial central ring and a floor flooded by radar-dark and radar-bright materials.
Ver en NASA ↗This image from NASA Magellan spacecraft shows an impact crater in the central Eistla Region of the equatorial highlands of Venus. The crater is slightly irregular in platform and its walls appear terraced.
Ver en NASA ↗This image from NASA Magellan spacecraft shows an irregular crater of approximately 14- kilometer 8.7-mile mean diameter. The crater is actually a cluster of four separate craters that are in rim contact.
Ver en NASA ↗The Moon and Venus, left, are seen in conjunction, Monday, May 18, 2026, from the Mary W. Jackson NASA Headquarters Building in Washington. Photo Credit: (NASA/Bill Ingalls)
Ver en NASA ↗The Moon and Venus, left, are seen in conjunction, Monday, May 18, 2026, from the Mary W. Jackson NASA Headquarters Building in Washington. Photo Credit: (NASA/Bill Ingalls)
Ver en NASA ↗A "transit of Venus" occurs when the planet Venus passes directly between the sun and the Earth. During the event, Venus will be seen from Earth as a small black sphere moving across the face of the sun. Such an event won’t occur again until the ye…
Ver en NASA ↗This image from NASA Magellan spacecraft is of Sachs Patera on Venus. Defined as a sag-caldera, Sachs is an elliptical depression 130 meters 81 feet in depth, spanning 40 kilometers 25 miles in width along its longest axis.
Ver en NASA ↗This image covers part of the 150 kilometer (90 mile) wide, 1 to 1.5 kilometer (0.6 to 0.9 mile) deep valley, Devana Chasma. The image is a composite of the first two orbits recorded by NASA's Magellan spacecraft in August 1990 superimposed on Pioneer Venus t…
Ver en NASA ↗During orbits 404 through 414 on 19-20 September 1990, Magellan imaged a peak-ring crater that is 50 kilometers in diameter located at latitude 27.4 degrees north and longitude 337.5 degrees east named Barton.
Ver en NASA ↗In September 1990, Magellan imaged this impact crater that is representative of Venusian craters that are of the proper diameter about 15 kilometers to be transitional in their morphology between complex and irregular craters.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.