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Artist concept of Mars Reconnaissance Orbiter
July 14, 2009
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NASA/JPL-Caltech
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This image taken by NASA’s Mars Reconnaissance Orbiter shows ice sheets at Mars’ south pole. The spacecraft detected clays nearby this ice; scientists have proposed such clays are the source of rad...
MRO Spots Clays and Ice
This observation shows a portion of the wall (light-toned material) and floor of a trough in the Acheron Fossae region of Mars. Many dark and light-toned slope streaks are visible on the wall of th...
Slope Streaks in Acheron Fossae
Mars has extremely large temperature changes from winter to summer compared to the Earth. It gets cold enough to freeze carbon dioxide out of the atmosphere during the winter, but this ice is unsta...
Carbon Dioxide Ice in the Late Summer
Getting a spacecraft to Mars is no walk in the park - as launch engineers are well aware. But when the spacecraft in question is among the largest ever sent to the red planet, there are specific ch...
Challenges of Getting to Mars: Heavy Lifting
This set of images from NASA’s Mars Reconnaissance Orbiter shows a fierce dust storm is kicking up on Mars, with rovers on the surface indicated as icons.
2018 Giant Dust Storm on Mars
This set of images shows what might be hardware from the Soviet Union's 1971 Mars 3 lander, seen in a pair of images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Ma...
Could This Be the Mars Soviet 3 Lander?
A newly found, buried deposit of frozen carbon dioxide -- dry ice -- near the south pole of Mars contains about 30 times more carbon dioxide than previously estimated to be frozen near the pole.
Thickness Map of Buried Carbon-Dioxide Deposit
This proposed future Mars landing site in Acidalia Planitia targets densely occurring mounds thought to be mud volcanoes.
Proposed Future Mars Landing Site: Acidalia Planitia Mud Volcanoes
Download a PDF of the Mars as Art Booklet.
Mars as Art (2013)
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
Here is a view of Earth and its moon, as seen from Mars. It combines two images acquired on Nov. 20, 2016, by the HiRISE camera on NASA's Mars Reconnaissance Orbiter, with brightness adjusted separ...
Earth and Its Moon, as Seen From Mars
This image (top) taken by the Shallow Radar instrument on NASA's Mars Reconnaissance Orbiter reveals the layers of ice, sand and dust that make up the north polar ice cap on Mars
What Lies Below a Martian Ice Cap
Three pairs of before and after images from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter illustrate movement of ripples on dark sand dunes in...
Changes in Ripples on Martian Dunes in Nili Patera
On Nov. 1, 2016, the HiRISE camera on NASA's Mars Reconnaissance Orbiter observed the impact site of Europe's Schiaparelli test lander, gaining the first color view of the site since the lander's O...
Schiaparelli Impact Site on Mars, in Color
This image acquired on October 7, 2020 by NASAs Mars Reconnaissance Orbiter, shows a deposit draping the surface like a blanket.
A Slice of Ice
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
NASA's Mars Exploration Rover Opportunity has been working on Mars since landing inside Eagle Crater on Jan. 25, 2004 (Universal Time; evening of Jan. 24, Pacific Standard Time).
Opportunity's First Decade of Driving on Mars
Two types of wind-blown sedimentary deposits are pictured in this scene of the floor of Ius Chasma in the Valles Marineris.
Dunes and Ripples in Valles Marineris (3-D)
Dry ice causes "Swiss Cheese" terrain on Mars.
"Swiss Cheese" Terrain on Mars
This series of images shows warm-season features that might be evidence of salty liquid water active on Mars today.
Warm-Season Flows on Slope in Horowitz Crater (Eight-Image Sequence)
Image of Hesperia Planum from the HiRISE camera on Mars Reconnaissance Orbiter.
Hesperia Planum
This animation demonstrates the salty ponds and streams that scientists think may have been left behind as Gale Crater dried out over time. The bottom of the image is the floor of Gale Crater, with...
Sutton Island Model of Drying Lakes
Dark, narrow streaks on Martian slopes such as these at Hale Crater are inferred to have been formed by seasonal flow of water on contemporary Mars. Detection of hydrated salts at the streaks suppo...
Recurring 'Lineae' on Slopes at Hale Crater, Mars
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 image covers part of the floor of a large ancient impact crater, near the western rim.
Layers of Water-Deposited Sediment (3-D)
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