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Mars InSight team members all react after receiving confirmation that the Mars InSight lander successfully touched down on the surface of Mars, Monday, Nov. 26, 2018 inside the Mission Support Area at NASA's Jet Propulsion Laboratory in Pasadena, California. …

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Re-analysis of data from a hydrogen-finding instrument on NASA's Mars Odyssey orbiter increased the resolution of maps of hydrogen abundance. The reprocessed data shows more 'water-equivalent hydrogen'in some parts of this equatorial region of Mars.

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This panorama from the Mast Camera (Mastcam) of NASA's Curiosity Mars rover shows details of 'Vera Rubin Ridge,' which stretches about 4 miles (6.5 kilometers), end-to-end, on the northwestern flank of lower Mount Sharp.

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This view of a test rover at NASA Jet Propulsion Laboratory, Pasadena, California, results from advance testing of arm positions and camera pointings for taking a low-angle self-portrait of NASA Curiosity Mars rover.

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This composite image of Earth and its moon, as seen from Mars, combines the best Earth image with the best moon image from four sets of images acquired on Nov. 20, 2016, by NASA's Mars Reconnaissance Orbiter. Mars was about 127 million miles from Earth.

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This wide panorama was taken by NASA's Curiosity Mars rover on Dec. 19, 2019. On the righthand foreground is Western Butte. The ridge with a crusty cap in the background is the Greenheugh pediment.

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NASA astronaut Zena Cardman answers a question during a Mars 2020 NASA Social at Kennedy Space Center’s News Center in Florida on July 29, 2020. At right is NASA Administrator Jim Bridenstine. The Mars Perseverance rover and Ingenuity helicopter are scheduled…

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NASA Deputy Administrator Jim Morhard answers questions during a Mars 2020 NASA Social at Kennedy Space Center’s News Center in Florida on July 29, 2020. The Mars Perseverance rover and Ingenuity helicopter are scheduled to launch July 30, on a United Launch …

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NASA Administrator Jim Bridenstine answers a question during a Mars 2020 NASA Social at Kennedy Space Center’s News Center in Florida on July 29, 2020. At left is NASA astronaut Zena Cardman. The Mars Perseverance rover and Ingenuity helicopter are scheduled …

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Brian Clement, Planetary Protection lead for MarCO, NASA JPL, talks about Mars Cube One (MarCO) during an Mars InSight pre-landing briefing, Sunday, Nov. 25, 2018 at NASA's Jet Propulsion Laboratory in Pasadena, California. InSight, short for Interior Explor…

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Brian Clement, Planetary Protection lead for MarCO, NASA JPL, talks about Mars Cube One (MarCO) during an Mars InSight pre-landing briefing, Sunday, Nov. 25, 2018 at NASA's Jet Propulsion Laboratory in Pasadena, California. InSight, short for Interior Explor…

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This frame from an animation portrays the unfolding of all three booms making up the antenna for the radar instrument on the European Space Agency Mars Express orbiter.

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Tithonium Chasma has numerous large landslide deposits. At the bottom of this image captured by NASA's 2001 Mars Odyssey spacecraft is the high plateau between Tithonium Chasma and Ius Chasma.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows part of the western end of Ius Chasma. Both the north and south canyon walls are visible in this image. At the top of the frame paired faults have created a graben.

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This image of Tithonium Chasma captured by NASA's 2001 Mars Odyssey spacecraft shows the canyon wall at the top of the frame, a series of landslide deposits in the middle, and an eroded mound of materials at the bottom.

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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the eastern end of Ius Chasma. Geryon Montes are located in the bottom half of the image. Between the montes and the southern wall face is a region of sand and sand dunes.

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This image of Tithonium Chasma from NASA's 2001 Mars Odyssey spacecraft shows the canyon wall at the top of the frame and the cliff face of the opposite side of the canyon at the bottom of the image.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows the eastern end of Ius Chasma. The southern canyon wall is at the bottom of the image, with dark sand and sand dunes.

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This image captured by NASA's 2001 Mars Odyssey spacecraft shows a section of Ius Chasma that is not dominated by landslide deposits. Geryon Montes has several visible faults, including a pair of faults that divide the uppermost ridge into two sections.

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In this image captured by NASA's 2001 Mars Odyssey spacecraft a complex region of multiple overlapping landslide deposits fills most the the frame. The very top layer has the lobate edges and radial surface grooves of a low volume slide.

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An artist's rendition of NASA's InSight lander operating on the surface of Mars.

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A full-scale mockup of NASA’s Mars 2020 Perseverance rover is on display at the News Center at the agency’s Kennedy Space Center in Florida on July 29, 2020. A Mars 2020 NASA Social is in progress featuring, right to left, Kennedy Space Center Deputy Director…

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These are more wispy blue clouds from Sol 39, Aug. 12, 1997, as seen by the Imager for NASA's Mars Pathfinder. The bright clouds near the bottom are about 30 degrees above the horizon. The clouds are thought to be made of small water ice particles.

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Full-Circle Color Panorama of Phoenix Landing Site on Northern Mars, Polar Projection

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