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Landing Site Region
January 11, 2007
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NASA/JPL/Univ. of Arizona
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This image, taken with the High Resolution Imaging Science Experiment (HiRISE) camera, shows distinct bands of alternating tone and brightness within the "Murray Formation" on Mars.
Bands on the 'Murray Formation'
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
Mysterious features on slopes hint there could be water flows on Mars.
Possible Water Flows on Mars
These dunes may be active today, but we haven't yet observed them at significantly different times to measure the movement.
Dunes on Ridges (3-D)
This color thumbnail image was obtained by NASA's Curiosity rover during its descent to the surface of Mars on Aug. 5 PDT (Aug. 6 EDT).
Curiosity's Heat Shield in View
This image acquired on December 9, 2018 by NASAs Mars Reconnaissance Orbiter, shows Athabasca Valles with lava flows originating from Elysium Mons to the northwest.
Almost Like Water
Mawrth Vallis contains clay minerals that formed by chemical alteration of rocks by water. The central part of the image is dominated by light-toned materials with curving fractures of many differe...
Mawrth Vallis Closeup (3-D)
This photograph from Shiprock in northwestern New Mexico shows a ridge roughly 30 feet (about 10 meters) tall that formed from lava filling an underground fracture then resisting erosion better tha...
'Wing' Dike of Hardened Lava in New Mexico
The HiRISE camera on the Mars Reconnaissance Orbiter is the most powerful telescope to have left Earth orbit. HiRISE is capable of some interesting astronomical observations such as this image of J...
Jupiter Viewed From Mars
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
This is the first image of Mars taken by the Context Camera on NASA's Mars Reconnaissance Orbiter.
First Context Camera Image of Mars
Phobos from 5,800 Kilometers
Phobos from 6,800 Kilometers
This image shows details of the lava covered plains near the equator of Mars. The darker looking area has a rough lava surface with all the shadows giving the region a darker appearance.
Lava Flow Front in Elysium Planitia
The Global CTX Mosaic of Mars allows scientists and the public to explore the planet like never before.
CTX Mosaic Shows Geographic Locations on Mars
Gullies on Martian sand dunes, like these in Matara Crater, have been very active, with many flows in the last ten years. In this image from NASA's Mars Reconnaissance Orbiter frost in and around t...
Gullies of Matara Crater
Intra-Crater Structure in NW Hellas Basin, Mars
Intra-Crater Structure in NW Hellas Basin, Mars
Nili Patera is a region on Mars in which dunes and ripples are moving rapidly. HiRISE continues to monitor this area every couple of months to see changes over seasonal and annual time scales.
Dunes and Ripples in Nili Patera
NASA's Opportunity Mars rover, working on Mars since January 2004, passed marathon distance in total driving on March 24, 2015. This map shows the rover's entire traverse from landing to that point.
Opportunity Rover's Full Marathon-Length Traverse
The yellow-white cloud in the bottom-center of this image is a Mars "dust tower" — a concentrated cloud of dust that can be lofted dozens of miles above the surface. The blue-white plumes are water...
A Mars Dust Tower Stands Out
This image shows dunes near the north pole of Mars. The north pole is surrounded by a vast "sea" of basaltic sand dunes, and the dunes imaged here are similar to barchan dunes that are commonly fo...
Mars' Shifting Sands
NASA's Mars Reconnaissance Orbiter passes above a portion of the planet called Nilosyrtis Mensae in this artist's concept illustration.
Mars Reconnaissance Orbiter over Nilosyrtis
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)
Ring and Cone Structures and Platy-Ridged Terrain in Amazonis Planitia
Ring and Cone Structures and Platy-Ridged Terrain in Amazonis Planitia
This view of layered rocks on the floor of McLaughlin Crater shows sedimentary rocks that contain spectroscopic evidence for minerals formed through interaction with water.
Layers with Carbonate Content Inside McLaughlin Crater on Mars
Mars Reconnaissance Orbiter captures the springtime thaw of seasonal carbon dioxide ice on Mars.
Mars: Dry Ice and Dunes
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