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This image, from NASA Mariner 10 spacecraft which launched in 1974, is of the Borealis area H-1, located in Mercury northern hemisphere. The north pole is visible at the top of the image.
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Taken about 40 minutes before NASA Mariner 10 made its close approach to Mercury on Sept. 21,1974, this picture shows a large double-ringed basin center of picture located in the planet south polar region
Ver en NASA ↗NASA Mariner 10 shows a close-up view of one-half of a circular basin the largest observed on Mercury. Hills and valleys extend in a radial fashion outward from the main ring.
Ver en NASA ↗This double ring basin top center of image was photographed during NASA Mariner 10 second encounter and shows two craters about 30 km in diameter which have been engulfed by smooth plains on the floor of the inner ring.
Ver en NASA ↗During its second encounter with Mercury on Sept. 21, 1974, NASA Mariner 10 took this picture of the planet South Polar Region. Many of the craters have denuded rims peppered by smaller craters.
Ver en NASA ↗As NASA Mariner 10 passed by Mercury on its second encounter with the planet on Sept. 21, 1974, this picture of a large circular 350 kilometer, 220 mile diameter basin was obtained near the morning terminator.
Ver en NASA ↗This image was taken by NASA Mariner 10 during it first encounter with Mercury in 1974. The scarp forms a broad lobe whose southern end abuts against and follows closely the irregular contour of the crater wall.
Ver en NASA ↗This computer generated mosaic from NASA Mariner 10 is of Mercury Tolstoj Quadrangle, named for the ancient Tolstoj crater located in the lower center of the image.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, shows a scarp upper left corner of the image about 130 kilometers long cutting two craters older crater is at extreme left corner, younger is diagonally below.
Ver en NASA ↗One of NASA Mariner 10 two TV cameras took this picture of a densely cratered region of Mercury on Sept. 21, 1974, 80 minutes prior to the spacecraft second close encounter with the planet.
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 ↗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 ↗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 ↗This computer photomosaic is of the Caloris Basin, the largest basin on Mercury. NASA Mariner 10 spacecraft imaged the region during its initial flyby of the planet after its launch in 1974.
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 ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, is a high-resolution picture of a 65-kilometer diameter crater and the scarp transecting its floor.
Ver en NASA ↗Cratered terrain very similar to that on the Moon is shown in this TV photo of Mercury taken by NASA Mariner 10. Numerous small craters and linear grooves radial to the crater can be seen.
Ver en NASA ↗NASA Mariner 10 took this picture some 2 1/2 hours before it passed Mercury on March 29, 1974. The bright-floored crater is the center of a very large bright area which could be seen in pictures from more than two million miles distant
Ver en NASA ↗NASA Mariner 10 took this picture about an hour after it passed under the South Pole of Mercury in 1974.
Ver en NASA ↗NASA Mariner 10 photo reveals a heavily cratered terrain on Mercury with a prominent scrap extending several hundred kilometers across the upper left. A crater, nested in a larger crater, is at top center.
Ver en NASA ↗This image, from NASA Mariner 10 spacecraft which launched in 1974, includes part of the floor of the Caloris basin showing the ridges and fractures.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.