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Caloris Basin on Mercury, is one of the largest basins in the solar system, its diameter exceeds 1300 kilometers and is in many ways similar to the great Imbrium basin on the Moon. This image is from NASA Mariner 10 spacecraft which launched in 1974.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows young craters superposed on smooth plains. Larger young craters have central peaks, flat floors, terraced walls, and radial ejecta deposits.
Ver en NASA ↗After passing Mercury the first time and making a trip around the Sun, NASA Mariner 10 again flew by Mercury on Sept. 21, 1974. This encounter brought the spacecraft in front of Mercury in the southern hemisphere.
Ver en NASA ↗Updated calibration and subsequent mosaicing led to substantial improvements in NASA Mariner 10 color image data; the spacecraft launched in 1974.
Ver en NASA ↗This photograph of Mercury, taken by NASA Mariner 10, shows two prominent rayed craters. Bright halos extend as far as 2 crater diameters beyond crater rims. Individual rays extend from halo.
Ver en NASA ↗NASA Mariner 10 took this picture of the densely cratered surface of Mercury when the spacecraft was 18,200 kilometers 8085 miles from the planet on March 29, 1974.
Ver en NASA ↗This crater illustrates the narrow hummocky rim facies, radial ridges, and surrounding extensive field of secondary craters. This image of Mercury was taken by NASA Mariner 10.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows intercrater plains and heavily cratered terrain typical of much of Mercury outside the area affected by the formation of the Caloris basin.
Ver en NASA ↗NASA Mariner 10 was launched on November 3, 1973, 12:45 am PST, from Cape Canaveral on an Atlas/Centaur rocket a reconditioned Intercontinental Ballistic Missile - ICBM.
Ver en NASA ↗After passing Mercury the first time and making a trip around the Sun, NASA Mariner 10 again flew by Mercury on Sept. 21, 1974. This encounter brought the spacecraft in front of Mercury in the southern hemisphere.
Ver en NASA ↗This computer generated photomosaic from NASA Mariner 10 is of the southern half of Mercury Shakespeare Quadrangle, named for the ancient Shakespeare crater located on the upper edge to the left of center.
Ver en NASA ↗This photograph of Mercury was taken by NASA Mariner 10 spacecraft shows smooth plains areas on Mercury that are thought to be volcanic in origin with lava flows filling in heavily cratered areas.
Ver en NASA ↗NASA Mariner 10 spacecraft was coaxed into a third and final encounter with Mercury in March of 1975. This is one of the highest resolution images of Mercury acquired by the spacecraft.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows an old basin hummocky rim is partly degraded and cratered by later events.
Ver en NASA ↗After passing Mercury the first time and making a trip around the Sun, NASA Mariner 10 again flew by Mercury on Sept. 21, 1974. The south pole is located on the right hand edge of Chao Meng Fu crater that has only its rim sticking up into the light.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows that several west-facing lobate scarps occur in the hummocky plains interpreted as Caloris ejecta.
Ver en NASA ↗A scarp, or cliff, extends diagonally from upper left to lower right in this picture of Mercury taken by NASA Mariner 10. The structures are believed to be formed by the compressive forces due to crustal shortening.
Ver en NASA ↗This mosaic, made from over 140 individual TV frames taken about two hours after encounter, shows the planet Mercury as seen by NASA Mariner 10 as it sped away from the planet on March 29, 1974.
Ver en NASA ↗NASA Mariner 10 spacecraft was coaxed into a third and final encounter with Mercury in March of 1975. This is one of the highest resolution images of Mercury acquired by the spacecraft. The prominent scarp snaking up the image was named Discovery Rupes.
Ver en NASA ↗A dark, smooth, relatively uncratered area on Mercury was photographed two hours after NASA Mariner 10 flew by the planet. The prominent, sharp crater with a central peak is 30 kilometers 19 miles across.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows a broadly curved lobate scarp running from left to right in the large crater to the right of center in this image.
Ver en NASA ↗A fresh new crater in the center of an older crater basin is shown in this picture of the surface of Mercury taken March 29, 1974 by NASA Mariner 10.
Ver en NASA ↗One of the most prominent lobate scarps Discovery Scarp, photographed by NASA Mariner 10 during it first encounter with Mercury, is located at the center of this image extending from the top to near bottom.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.