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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.

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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.

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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.

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Photographed are models of early rocketry: The Atlas Mercury, Redstone Mercury; and Saturn C-1.

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At approximately 1.1 meters/pixel, this image is among the highest-resolution views MESSENGER has ever taken of the surface of Mercury.

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Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

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Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

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Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
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Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
Ver en NASA ↗

Visit to Glenn Research Center at Lewis Field by Mercury 13 Astronaut Trainee, Wally Funk

GRC
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S64-14286 (11 Feb. 1964) --- An artist's concept of Mercury: Medical effects; develop technology. Photo credit: NASA

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Testing of Mercury Capsule Shape A by the Hydrodynamics Division of Langley. Joseph Shortal wrote (vol. 3, p. 19): The Hydrodynamics Division provided assistance in determining landing loads. In this connection, after PARD engineers had unofficially approach…

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In mid-February, before and after MESSENGER latest perihelion closest approach to the Sun, an imaging campaign was conducted to search for vulcanoids, small rocky bodies that have been postulated to exist in orbits between Mercury and the Sun.

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This false-color image of Mercury captured by NASA MESSENGER spacecraft shows the great Caloris impact basin, visible here as a large, circular, orange feature in the center of the picture.

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The cliff-like feature crossing this image from NASA MESSENGER spacecraft from top to bottom is one of Mercury famed lobate scarps, and is called Pourquoi-Pas Rupes.

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Hemingway crater is seen in this color view of Mercury surface as seen by NASA MESSENGER spacecraft. Hemingway is the 130-km 81-mile diameter crater with a relatively brown floor and small patch of dark blue in its center.

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Lermontov crater was first observed by Mariner 10 and seen here by MESSENGER during its second flyby of Mercury. The crater floor is somewhat brighter than the exterior surface and is smooth with several irregularly shaped depressions.

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On Mercury, NASA MESSENGER shows the smooth floor of Titian is a brighter orange color than the surrounding area, likely due to being filled with volcanic material. Ejecta from Titian appears blue.

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Contenido y metadatos proporcionados por la NASA Image and Video Library.