/NASA’s%20Artemis%20III%20Announcement%20(Official%20NASA%20Trailer)~thumb.jpg)
This image shows changes in the target landing area for Curiosity, NASA Mars Science Laboratory rover. The larger ellipse for the target area has been revised to the smaller ellipse centered nearer to the foot of Mount Sharp, inside Gale Crater.
Ver en NASA ↗🚀 Biblioteca espacial oficial
Imágenes y vídeos de NASA
Explora el catálogo multimedia público de NASA sin salir de TuPortalNews.
Explora temas destacados
Selecciona un tema o realiza una búsqueda personalizada.
26.836 resultados en NASA
This map shows in red the route driven by NASA Curiosity Mars rover from its landing site at Bradbury Landing. The white line shows the planned route to reach destinations on Mount Sharp. Sol 669 will complete one Martian year.
Ver en NASA ↗These MOC images capture what Mars typically looks like in mid-afternoon at Ls 121°. In other words, with the exception of occasional differences in weather and polar frost patterns, this is what the red planet looks like this month October 2006
Ver en NASA ↗This annotated image taken on Dec. 15, 2014 by NASA Mars Reconnaissance Orbiter shows a bright feature interpreted as the United Kingdom Beagle 2 Lander, which was never heard from after its expected Dec. 25, 2003, landing.
Ver en NASA ↗This hole, with a diameter slightly smaller than a U.S. dime, was drilled by NASA Curiosity Mars rover into a rock target called Telegraph Peak. The rock is located within the basal layer of Mount Sharp. The hole was drilled on Feb. 24, 2015.
Ver en NASA ↗Dust Devils Seen Streaking Across Mars: PART II--Theyre the Work of the Devil!
Ver en NASA ↗Layers within the Valles Marineris: Clues to the Ancient Crust of Mars - High Resolution Image
Ver en NASA ↗Mars Global Surveyor View of Gusev Crater During Spirit Entry, Descent, and Landing
Ver en NASA ↗Evidence for Recent Liquid Water on Mars: Channeled Aprons in a Small Crater within Newton Crater
Ver en NASA ↗Evidence for Recent Liquid Water on Mars: Clues Regarding the Relative Youth of Martian Gullies
Ver en NASA ↗Evidence for Recent Liquid Water on Mars: Gullies at 70°S in Polar Pit Walls
Ver en NASA ↗MOC Observes Changes in the South Polar Cap: Evidence for Recent Climate Change on Mars
Ver en NASA ↗Evidence for Recent Liquid Water on Mars: Channeled Aprons in a Small Crater within Newton Crater
Ver en NASA ↗Doug McCuiston, Director, Mars Exploration Program, talks during a Mars Program Update where prominent scientists discussed evidence of water on Mars, current Program status, including the 7th Anniversary of the Mars rovers and the upcoming Mars Science Labor…
Ver en NASA ↗Dr, Michael Meyer, NASA Mars lead scientist, talks during a Mars Program Update where prominent scientists discussed evidence of water on Mars, current Program status, including the 7th Anniversary of the Mars rovers and the upcoming Mars Science Laboratory m…
Ver en NASA ↗Guest attending the National Geographic “Mars Up Close” panel discussion, look at full scale models of the Spirit/Opportunity, left, and Curiosity, Mars rovers, Tuesday, August 5, 2014, at the National Geographic Society headquarters in Washington. Guest list…
Ver en NASA ↗This image from NASA's 2001 Mars Odyssey spacecraft shows part of the southeastern flank of Arsia Mons, including the flat lying flows around the base of the volcano. These flows are located at the bottom of the image.
Ver en NASA ↗This image from NASA's 2001 Mars Odyssey spacecraft shows the eastern section of the large landslide deposit seen in Ius Chasma. A landslide is a failure of slope due to gravity.
Ver en NASA ↗This image from NASA's 2001 Mars Odyssey spacecraft shows part of Tithonium Chasma. A lobate 'tongue' visible between the ridge and the top of the canyon is the deposit left by a landslide event.
Ver en NASA ↗Tithonium Chasma has numerous large landslide deposits, as shown in this image from NASA's 2001 Mars Odyssey spacecraft. The resistant material of the plateau surface forms the linear ridges of the canyon wall.
Ver en NASA ↗The three large aligned Tharsis volcanoes are Arsia Mons, Pavonis Mons and Ascreaus Mons (from south to north). This image from NASA's 2001 Mars Odyssey spacecraft shows part of the northeastern flank of Arsia Mons.
Ver en NASA ↗This image from NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the top of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.
Ver en NASA ↗This section of the canyon floor of Ius Chasma has been completely filled by blocky deposits from large volume landslides. A landslide is a failure of slope due to gravity. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
Ver en NASA ↗This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of eastern Candor Chasma. At the top of the image is the steep cliff between the upper surface elevation and the depths of Candor Chasma.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.