One of two images that NASA's Mars Reconnaissance Orbiter took of the Martian moon Phobos on March 23, 2008, this view was captured from about 3,600 miles away from the moon.
The largest feature on the Martian moon Phobos is the crater named Stickney, with is about 9 kilometers (5.6 miles) in diameter, in the lower right of this image taken by NASA's Mars Reconnaissance Orbiter.
Combining exposures taken in blue-green, red and near-infrared light yields this color image of the Martian moon Phobos, in which the bluer material around the edge of the largest crater may be some of the most freshly exposed surface of the small moon.
In this image from NASA's Mars Reconnaissance Orbiter, craters on part of the surface of the Martian moon Phobos that is shaded from direct sunlight are visible because the moon also is illuminated by sunlight reflected off Mars, or "Marsshine."
This image provides higher-resolution views of a site where another observation indicates the presence of chloride salt deposits.
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.
Amazingly, this image has captured at least four Martian avalanches, or debris falls, in action.
Dust-devils are vortices of wind that form when air rising from a warm surface encounters shear in the above atmosphere.
This movie, constructed by overlaying a time series of images taken by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM), shows seasonal changes and unearthly processes that occur in Mars' south polar seasonal frost cap.
A regional landscape near Mars' south pole is called "cryptic terrain" because it once defied explanation, but new observations bolster and refine interpretations of how springtime outbursts of carbon-dioxide gas there sculpt intricate patterns and paint seasonal splotches.
Candor Chasma forms part of the large Martian canyon system named Valles Marineris.
This view, covering an area approximately 580 kilometers (360 miles) wide, shows the location of a study area within Mars' Candor Chasma within regional context.
This is a perspective view of a scene within Mars' Candor Chasma based on stereo imaging by the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter.
This is a perspective view of a scene within Mars' Candor Chasma based on stereo imaging by the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter.
This is a eastward-looking perspective view of a scene within Mars' Candor Chasma based on stereo imaging by the High Resolution Imaging Science Experiment (HiRISE) camera aboard NASA's Mars Reconnaissance Orbiter.
The south polar region of Mars is covered every year by a layer of carbon dioxide ice.
There is an enigmatic region near the south pole of Mars known as the "cryptic" terrain.
Every year seasonal carbon dioxide ice, known to us as "dry ice," covers the poles of Mars.
Translucent carbon dioxide ice covers the polar regions of Mars seasonally.
The south polar region of Mars is covered seasonally with translucent carbon dioxide ice.