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Artist concept of Glaciers on Mars
November 20, 2008
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NASA/JPL-Caltech
ENLARGE
[51, 178, 188]
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This image from NASA's Mars Reconnaissance Orbiter shows an impact crater that triggered a slope streak. When a meteoroid hit the surface and exploded to make the crater, it destabilized the slope ...
Bang and Whoosh!
Sand dunes are among the most widespread wind-formed (aeolian) features present on Mars.
Dune Composition (3-D)
This image shows layered blocks tilted at high angles, diverse color and textures and dark dunes. Some of the bedrock may have originated at great depths, uplifted first by Becquerel Crater and lat...
Tilted and Layered Bedrock Blocks in a Large Crater inside Becquerel Crater (3-D)
This image acquired on March 29, 2011 by NASAs Mars Reconnaissance Orbiter, shows dunes with ripples on their upwind slopes and dark streaks on their downwind slopes.
Active Dunes in Wirtz Crater
This DLE [double layer ejecta] crater formed at the edge of an older/pre-existing crater, the rim of which deflected some of its ejecta.
Double Layer Ejecta in an Arabia Region Crater (3-D)
This HiRISE image shows a mixture of bright and dark units. The bright units have a mineral called sulfate (salty sulfuric acid) that on Earth typically forms in the presence of water as an evapori...
Jumbled Terrain in Ius Chasma (3-D)
Deposits on the floor of Palos Crater
Deposits on the floor of Palos Crater
On this map of Mars, areas indicated in green are where spectrometers on spacecraft orbiting Mars have detected clay minerals and areas indicated in blue are where those spectrometers have detected...
Regions of Mars with Clays and Hydrated Minerals Identified from Orbit
Mars Reconnaissance Orbiter Project Manager Jim Graf shakes the hand of Andrew Dantzler, Director of NASA's Solar System Division, after a successful orbit insertion on March 10, 2006. Fuk Li, Dire...
Mars Reconnaissance Orbiter Mission Team Members Celebrate Orbit Insertion Success
This image shows layered sedimentary rocks and ripples that fill and surround an impact crater in Meridiani Planum, an equatorial region where the rover Opportunity has been exploring the Martian s...
Crater in Meridiani Planum (2.3 N, 2.6 W) [3-D]
Back-and-forth blinking of this two-image animation shows movement of a sand dune on Mars. The images are part of a study published by Nature on May 9, 2012, reporting movement of Martian sand dune...
Advancing Dune in Nili Patera, Mars
This false-color animation simulates a fly-around look at one of the places on Mars where dark streaks advance down slopes during warm seasons, possibly involving liquid water or brine. This site i...
Animation of Site of Seasonal Flows in Hale Crater, Mars
This HiRISE image covers the southwest portion of the terraces and floor of Holden Crater situated in southwest Margaritifer Terra.
Holden Crater Megabreccia: A Telltale Sign of a Sudden and Violent Event
Blue dots on this map indicate sites of recurring slope lineae (RSL) in part of the Valles Marineris canyon network on Mars. RSL are seasonal dark streaks that may be indicators of liquid water. Th...
Sites with Seasonal Streaks on Slopes in Mars Canyons
This image shows the context for orbital observations of exposed rocks that had been buried an estimated 5 kilometers (3 miles) deep on Mars.
Nature's Drilling Exposes Deeply Buried Minerals
This global map of Mars was acquired on Aug. 4, 2012, by the Mars Color Imager instrument on NASA's Mars Reconnaissance Orbiter.
Mars Weather Map, Aug. 4
This set of images shows "before" and "after" images of NASA's Phoenix Mars Lander taken by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter.
Image from Mars Orbit Indicates Solar Panels on Phoneix Lander may have Collapsed
Diagonal striping on this map of a portion of Mars' Utopia Planitia region indicates the area where a large subsurface deposit rich in water ice was assessed using the Shallow Radar (SHARAD) instru...
Location of Large Subsurface Water-Ice Deposit in Utopia Planitia, Mars
Curiosity performs the first investigation of active sand dunes on another planet. Studying the Bagnold Dunes on Mars will help scientists understand the physics of Martian dunes and how they move.
Curiosity Rover Report (Dec. 15, 2015): First Visit to Martian Dunes
This image covers a region of Mars near Nili Fossae that contains some of the best exposures of ancient bedrock on Mars.
A Wild Assortment of Jumbled Rocks
This view of a portion of the Eridania region of Mars shows blocks of deep-basin deposits that have been surrounded and partially buried by younger volcanic deposits. The image was taken by the Con...
Possible Floor of an Ancient Martian Sea
An oblique, northward-looking view based on stereo orbital imaging, shows the location of Opportunity on its journey from Cape York to Solander Point when HiRISE took the new color image.
Location of Opportunity Rover
The eastern margin of a rippled dune in Herschel Crater on Mars moved an average distance of three meters (about three yards) between March 3, 2007 and December 1, 2010, as seen by NASA's Mars Reco...
Shifting Sand in Herschel Crater
This image captures a fairly rare situation. In general, as lava flows along, it fills in low points and holes it encounters in its path and flows around high points such as hills and ridges. In th...
Lava Flow Oozing Into a Crater (3-D)
Two pairs of side-by-side, before and after images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter illustrate changes in the shape of edges...
Changes at Edges of Dark Dunes in Nili Patera, Mars
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