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Artist concept of Mars Reconnaissance Orbiter
July 14, 2009
Credits
NASA/JPL-Caltech
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This is a small volcano superimposed on the flanks of a larger one of the Cerberus Tholi.
Small Floral-Shaped Volcano
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
Image of Hesperia Planum from the HiRISE camera on Mars Reconnaissance Orbiter.
Hesperia Planum
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Clay Minerals in Mawrth Vallis Region of Mars
Countdown Nears: Final Tests
Countdown Nears: Final Tests
This close-up image of a dust storm on Mars was acquired by the Mars Color Imager instrument on NASA's Mars Reconnaissance Orbiter on Nov. 7, 2007
MARCI Sees a Martian Dust Storm
This vertically exaggerated view shows scalloped depressions in a part of Mars where such textures prompted researchers to check for buried ice, using ground-penetrating radar aboard NASA's Mars Re...
Scalloped Terrain Led to Finding of Buried Ice on Mars
The High Resolution Imaging Science Experiment (HiRISE) camera would make a great backyard telescope for viewing Mars, and we can also use it at Mars to view other planets. This is an image of Eart...
Earth and Moon as Seen from Mars
This observation from NASA's Mars Reconnaissance Orbiter shows a sand dune field in the Nili Fossae region of Mars. The dark lines swirling over the surface of the dunes are the tracks of dust devi...
Dust Devils on Mars
Mars' north polar deposits comprise a thick stack of icy layers. Part of this image from NASA's Mars Reconnaissance Orbiter (MRO) has lingering seasonal frost, which serves to accentuate those laye...
Lingering Frost
The total distance driven by NASA's Mars rover Curiosity passed the one-mile mark a few days before the first anniversary of the rover's landing on Mars.
Full Curiosity Traverse Passes One-Mile Mark
This terrain is covered by pits and scallops (pits open on one side), perhaps due to collapse after sublimation of subsurface ice.
Utopia Planitia Scallops, Polygons, and Boulders (3-D)
A Martian dust devil roughly 12 miles (20 kilometers) high was captured winding its way along the Amazonis Planitia region of Northern Mars on March 14, 2012 by the High Resolution Imaging Science ...
Mars' Whirling Dust Devil
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
Artist's concept of Mars Reconnaissance Orbiter en route to Mars.
Artist's concept of Mars Reconnaissance Orbiter en route to Mars.
This image, taken with the High Resolution Imaging Science Experiment (HiRISE) camera, shows the transition between the "Murray Formation," in which layers are poorly expressed and difficult to tra...
Geological Transition
This image, taken with the High Resolution Imaging Science Experiment (HiRISE) camera, shows the transition between the "Murray Formation," in which layers are poorly expressed and difficult to tra...
Geological Transition
NASA's Mars Reconnaissance Orbiter observes many slopes in the middle latitudes of Mars showing icy flows or glaciers. The region shown here, in the south-facing slope of a crater, is unusual becau...
Go with the (Bright) Flow
This image from the HiRISE camera on NASA's Mars Reconnaissance Orbiter shows a location associated with the novel and movie, "The Martian." It is the tale's planned landing site for the Ares 4 mis...
'The Martian' Story's Ares 4 Landing Site
The Mars Color Imager test view looks northward and includes the large Argyre Basin in Mars' southern hemisphere.
View of Argyre Basin from Test of Mars Color Image
This graphic shows the ongoing contributions of NASA’s rovers and orbiters during a Martian dust storm that began on May 30, 2018.
Mars Storm Watch Observations
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 diagram illustrates an interpretation for the origin of some deposits in the Eridania basin of southern Mars as resulting from seafloor hydrothermal activity more than 3 billion years ago.
A Geologic Model for Eridania Basin on Ancient Mars
This inner slope of a Martian crater has several of the seasonal dark streaks called "recurrent slope lineae," or RSL, that a November 2017 report interprets as granular flows, rather than darkenin...
Seasonal Dark Streaks in Tivat Crater, Mars
This is a close-up of the area in the vicinity of the Pathfinder landing site. Major features are named. The white box outlines the area of the image, where hardware is seen.
Landing Site Region
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