Follow this link to skip to the main content National Aeronautics and Space Administration Logo
NASA Banner
Mars Exploration Program
Home
  • navtop_search.png
MULTIMEDIA
<< First Page     < Previous  |   35   |  36   |  37   |  38   |  39   |  40   |  41   |  42   |  43   |  44   |  45   |  46   |  47   |  48   |  49   |  Next >     Last Page >>
Image of Hesperia Planum from the HiRISE camera on Mars Reconnaissance Orbiter.
Hesperia Planum
Okubo_figure_6.jpg
Deformation Bands in Martian Bedrock
20080807_PR.jpg
Clay Minerals in Mawrth Vallis Region of Mars
Crater Floor Deposits in Promethei Terra
Crater Floor Deposits in Promethei Terra
This map shows the thickness of the north polar layered deposits on Mars as measured by the Shallow Radar instrument on NASA's Mars Reconnaissance Orbiter.
How Thick is the North Polar Ice Cap on Mars?
Eridania Basin Light-Toned Outcrops
Eridania Basin Light-Toned Outcrops
20080506_p18_008130_subfig_i.jpg
Phoenix Landing Area Viewed by Mars Color Imager
Sample Noachis Terra
Sample Noachis Terra
Phobos in Stereo
'Marsshine' on Shadowed Part of Phobos
PIA10370-with-inset.jpg
'Marsshine' on Shadowed Part of Phobos
'Marsshine' on Shadowed Part of Phobos
Phobos from 5,800 Kilometers
PIA10369.jpg
NASA Spacecraft Images Mars Moon in Color and in 3D
PIA10368-cropV2.jpg
Phobos from 6,800 Kilometers (Color)
PIA10368.jpg
NASA Spacecraft Images Mars Moon in Color and in 3D
Phobos from 5,800 Kilometers
Phobos from 6,800 Kilometers
Phobos from 6,800 Kilometers
Phobos from 5,800 Kilometers (Color)
Caught in Action: This image shows avalanches on North Polar Scarps.
Caught in Action: Avalanches on North Polar Scarps
Chloride Salt Deposit in Southern Highlands of Mars
Bright Exposures of Chloride Salt on Southern Mars
Bright Exposures of Chloride Salt on Southern Mars
Bright Exposures of Chloride Salt on Southern Mars
PSP_006477_1745.jpg
Dust-Devil Tracks in Southern Schiaparelli Basin
This observation shows a wrinkle ridge in Solis Planum, located in the Thaumasia region of Mars, a high-elevation volcanic plain located south of the Valles Marineris canyon system and east of the Tharsis volcanic complex. Solis Planum contains some of the most distinct and well studied arrays of wrinkle ridges on Mars. Wrinkle ridges are long, winding topographic highs and are often characterized by a broad arch topped with a crenulated ridge. These features have been identified on many other planetary bodies such as the Moon, Mercury, and Venus. On Mars, they are many tens to hundreds of kilometers long, tens of kilometers wide, and have a relief of a few hundred meters. Wrinkle ridges are most commonly believed to form from horizontal compression or shortening of the crust due to faulting and are often located in volcanic plains. They commonly have asymmetrical cross sectional profiles and an offset in elevation on either side of the ridge. Large dunes are also visible bordering the wrinkle ridge. The reddish colors seen in this image most likely indicate the presence of dust (or indurated dust) and the darker, bluish colors most likely indicate the presence of larger rocks and boulders on the wrinkle ridge.
Wrinkle Ridge in Solis Planum
PSP_002622-002675_0945_RGB_zoom2.jpg
Global View of Candor Chasm Study Location
20071019_CRISM-Images.jpg
Spectrometer on NASA Orbiter Maps Minerals at Possible Landing Sites
Color Image of Nili Fossae Trough, a Candidate MSL Landing Site
Color Image of Layers in Holden Crater, a Candidate MSL Landing Site
The team developing NASA's Mars Science Laboratory calls this test rover "Scarecrow" because the vehicle does not include a computer brain. Mobility engineers use this test rover to evaluate mobility and suspension performance.
"Scarecrow"
<< First Page     < Previous  |   35   |  36   |  37   |  38   |  39   |  40   |  41   |  42   |  43   |  44   |  45   |  46   |  47   |  48   |  49   |  Next >     Last Page >>

USA.gov
PRIVACY     FAQ     SITEMAP     FEEDBACK     IMAGE POLICY