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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.
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This image, from NASA Mariner 10 spacecraft which launched in 1974, is of the southern hemisphere of Mercury.
Ver en NASA ↗A faint double ring crater is seen at upper right in this picture of Mercury taken one hour and 40 minutes before NASA Mariner 10 second rendezvous with the planet Sept. 21, 1975
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, is located about 500 km east of the Caloris basin and shows hummocky plains interpreted as Caloris ejecta in the upper half of the picture and smooth plains in the lower half.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, features a 140 kilometer diameter crater and its surrounding zone of secondary craters. T
Ver en NASA ↗A field of bright rays, created by ejecta from a crater, radiating to the north top from off camera lower right is seen in this view of Mercury taken Sept. 21, 1974 by NASA Mariner 10.
Ver en NASA ↗Intercrater plains and heavily cratered terrain typical of much of Mercury outside the area affected by the formation of the Caloris basin are shown in this image taken during the NASA Mariner 10 first encounter with Mercury in 1974.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows plains filling this basin are uniformly brighter and slightly redder than the surrounding cratered terrain.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows several scarps, which appear to be confined to crater floors. The scarp in the crater at the upper left of the image has been diverted by the central peaks.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, is of the northern half of Mercury Shakespeare Quadrangle.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, is of the H-7 Beethoven Quadrangle, and lies in Mercury Equatorial Mercator. NASA Mariner 10 spacecraft imaged the region during its initial flyby of the planet.
Ver en NASA ↗After passing on the darkside of the planet, NASA Mariner 10 photographed the other, somewhat more illuminated hemisphere of Mercury. The north pole is at the top, two-thirds down from which is the equator.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows hilly and lineated terrain and a patch of smooth plains in a large degraded crater.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, is of the Michelangelo Quadrangle, which lies in Mercury southern polar region. The Mercurian surface is heavily marred by numerous impact craters.
Ver en NASA ↗A cratered area near Mercury South Pole was photographed by NASA Mariner 10 during its second flyby of the planet of Sept. 21, 1974 the spacecraft made its first encounter with Mercury on March 19, 1974.
Ver en NASA ↗Antoniadi Ridge, over 450 kilometers long, runs along the right side of this acquired image during NASA Mariner 10 first encounter with Mercury after its launch in 1974.
Ver en NASA ↗This picture, taken only minutes after NASA Mariner 10 made its closest approach to Mercury, is one of the highest resolution pictures obtained. Abundant craters in various stages of degradation dot the surface.
Ver en NASA ↗The craters in this image NASA Mariner 10 spacecraft, which launched in 1974, have interior rings of mountains and ejecta deposits which are scarred by deep secondary crater chain groves.
Ver en NASA ↗Moon North Pole
Ver en NASA ↗As NASA Mariner 10 approached Mercury at nearly seven miles per second on March 29, 1974, its TV camera took this picture from an altitude of 35,000 kilometers 21,700 miles The picture shows a heavily-cratered surface with many low hills
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, is of the northeastern quadrant of the Caloris basin and shows the smooth hills and domes between the inner and outer scarps and the well-developed radial system east of the outer scarp
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 ↗Mercury south pole was photographed by one of NASA Mariner 10 TV cameras; the pole is located inside the large crater on Mercury limb lower center.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows a crater just north of the Caloris Planitia displays interior and central peaks rising up from a hilly floor.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.