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This image of Olympia Undae was collected early in north polar spring. The crests of the dunes are light colored, indicative of a frost covering. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
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This image of Olympia Undae from NASA's 2001 Mars Odyssey spacecraft was collected early in north polar spring. The crests of the dunes are light colored, indicative of a frost covering.
Ver en NASA ↗This image captured by NASA's 2001 Mars Odyssey spacecraft of Olympia Undae was collected during north polar spring. The crests of the dunes and other surfaces are light colored, indicative of a frost covering.
Ver en NASA ↗This image of Olympia Undae from NASA's 2001 Mars Odyssey spacecraft was collected during north polar summer. The dunes are now completely frost free and are dark in color due to being made of basaltic sand.
Ver en NASA ↗This image captured by NASA's 2001 Mars Odyssey spacecraft was collected at the height of summer. It is during this season that winds are able to move sand sized particles, slowly modifying the dunes.
Ver en NASA ↗This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the western flank of Pavonis Mons. The linear features are faults. Faulting usually includes change of elevation, where blocks of material slide down the fault.
Ver en NASA ↗Ius Chasma is unique from the other chasmata of Valles Marineris in possessing mega gullies on both sides of the chasma. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
Ver en NASA ↗This image from NASA's 2001 Mars Odyssey spacecraft shows the western part of the smaller summit caldera on Pavonis Mons. Pavonis Mons is one of the three aligned Tharsis Volcanoes.
Ver en NASA ↗Ius Chasma is unique from the other chasmata of Valles Marineris in possessing mega gullies on both sides of the chasma. The largest mega gullies are located in Sinai Planum. This image was obtained by NASA's 2001 Mars Odyssey spacecraft.
Ver en NASA ↗This image of Olympia Undae was collected during north polar spring. The crests of the dunes and other surfaces are light colored, indicative of a frost covering. 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 the southern flank of Pavonis Mons. Several faults run from the left to the right side of the image.
Ver en NASA ↗This image of Olympia Undae captured by NASA's 2001 Mars Odyssey spacecraft was collected during north polar summer. The dunes are now completely frost free and are dark in color due to being made of basaltic sand.
Ver en NASA ↗On Feb. 11, 2020, Mars 2020 Assembly, Test and Launch Operations Manager David Gruel watched as members of his team loaded NASA's next Mars rover onto an Air Force C-17 at March Air Reserve Base in Riverside, California.
Ver en NASA ↗Stars in the upper portion of the constellation Orion the Hunter, including the bright shoulder star Betelgeuse and Orion three-star belt, appear in this image taken from the surface of Mars by the panoramic camera on NASA rover Spirit.
Ver en NASA ↗Engineers install the SuperCam instrument on Mars 2020's rover. This image was taken on June 25, 2019.
Ver en NASA ↗In this image, taken on June 13, 2019, engineers at JPL install the starboard legs and wheels on NASA's Mars 2020 rover.
Ver en NASA ↗This image of the flank of Ascraeus Mons obtained by NASA's 2001 Mars Odyssey spacecraft shows several individual flows where the sides are higher than the center.
Ver en NASA ↗This image captured by NASA's 2001 Mars Odyssey spacecraft shows the side of the large mesa at the top of the image and the southern canyon cliff face at the bottom.
Ver en NASA ↗This map shows the route driven by NASA Curiosity Mars rover from the location where it landed in August 2012 to its location in December 2015.
Ver en NASA ↗This image from July 2008 shows the aeroshell for NASA Mars Science Laboratory while it was being worked on by spacecraft technicians at Lockheed Martin Space Systems Company near Denver.
Ver en NASA ↗In late October 2004, NASA Mars Reconnaissance Orbiter was moved from the High Bay 100,000-class clean room at Lockheed Martin Space Systems, Denver, to the facility Reverberant Acoustic Lab.
Ver en NASA ↗This image shows the approximate true position of NASA Curiosity rover on Mars. A 3-D virtual model of Curiosity is shown inside Gale Crater, near Mount Sharp, Curiosity ultimate destination.
Ver en NASA ↗The Sample Analysis at Mars SAM instrument will analyze samples of Martian rock and soil collected by the rover arm to assess carbon chemistry through a search for organic compounds, and to look for clues about planetary change.
Ver en NASA ↗This image shows laser plasmas in a test lab at Los Alamos National Laboratory, N.M., under typical atmospheric pressures on Earth and Mars. A plasma is an ionized, glowing gas.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.