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January 11, 2007
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NASA/JPL/Univ. of Arizona
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This 3D, or stereo anaglyph, view shows the parachute and back shell that helped guide NASA's Curiosity to the surface of Mars.
Parachute and Back Shell in 3D
This map shows the route driven by NASA's Mars rover Curiosity through the 56th Martian day, or sol, of the rover's mission on Mars (Oct. 2, 2012).
Curiosity's Travels Through Sol 56
This image covers part of the floor of a large ancient impact crater, near the western rim.
Layers of Water-Deposited Sediment (3-D)
This enhanced-color image shows sand dunes trapped in an impact crater in Noachis Terra, Mars.
Dunes in Noachis Terra Region of Mars
This image from NASA's Mars Reconnaissance Orbiter (MRO) shows sand dunes on the slopes of Nectaris Montes within Coprates Chasma.
Dunes in Nectaris Montes
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
A regional dust storm visible in the southern hemisphere of Mars in this nearly global mosaic of observations made by the Mars Color Imager on NASA's Mars Reconnaissance Orbiter on Nov. 25, 2012.
Regional Dust Storm Weakening, Nov. 25, 2012
The Eridania basin of southern Mars is believed to have held a sea about 3.7 billion years ago, with seafloor deposits likely resulting from underwater hydrothermal activity. This graphic shows est...
Estimated Water Depths in Ancient Martian Sea
What appear to be spiders scampering across the martian landscape are actually cracks in the surface of the southern polar region on Mars, seen by the Mars Reconnaissance Orbiter on August 23, 2009...
South Pole Spiders
This picture was taken during the Martian summer with only small patches of ice remaining at the surface; they show up as bright, somewhat blue, spots on slopes that provide some shading from the Sun.
Sand Dunes Near the North Pole
This map indicates geological units in the region of Mars around a smaller area where NASA's Mars Exploration Rover Opportunity has driven from early 2004 through late 2010.
Geologic Setting of Opportunity Traverse and Meridiani Planum
This graph shows changes in apparent brightness of comet C/2013 A1 Siding Spring as it approached and receded from Mars, as seen by the High Resolution Imaging Science Experiment (HiRISE) camera on...
Brightness Rhythm of Mars Flyby Comet Is Clue to Rotation Rate
The insert in this image is a simulation of what the Mars Reconnaissance Orbiter's optical navigation camera images of the Martian moons Phobos and Deimos will look like.
Phobos and Deimos, Prepare to Say 'Cheese!'
This image from NASA's Mars Reconnaissance Orbiter shows a hill with a central crater. Such features have been interpreted as both mud volcanoes (really a sedimentary structure) and as actual volca...
A Volcano of Mud or Lava?
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 Newton Crater (Five-Image Sequence)
In Aureum Chaos, the OMEGA experiment on Mars Express indicated the presence of phyllosilicates (clay minerals) which have been detected in a variety of bright outcrops and scarps. The subimage sho...
Light-Toned Outcrop in Aureum Chaos
This graphic maps locations of the sites where NASA's Curiosity Mars rover collected its first 19 rock or soil samples for laboratory analysis inside the vehicle. It also presents images of the dri...
Curiosity's Rock or Soil Sampling Sites on Mars, Through November 2016
This map shows the route driven by NASA's Curiosity Mars rover from the location where it landed in August 2012 to its location in December 2015, at examples of the Bagnold Dunes.
Curiosity Rover's Traverse, First 1,185 Sols on Mars
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
This map shows the frequency of carbon dioxide frost's presence at sunrise on Mars, as a percentage of days year-round. Carbon dioxide ice more often covers the ground at night in some mid-latitude...
Where on Mars Does Carbon Dioxide Frost Form Often?
This is a small volcano superimposed on the flanks of a larger one of the Cerberus Tholi.
Small Floral-Shaped Volcano
Images like this from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter show portions of the Martian surface in unprecedented detail.
True Gullies on Mars
This pit crater was created by an empty lava tube in Mars’ Arsia Mons region. The image was captured by NASA’s Mars Reconnaissance Orbiter on Aug. 16, 2020.
HiRISE Spots the Mouth of a Martian Lava Tube
This image shows part of Ladon Vallis that is located within Ladon basin.
Light-Toned Layered Rock Outcrop in Ladon Valles (3-D)
This HiRISE image shows fractured mounds on the southern edge of Elysium Planitia.
Fractured Mounds in Elysium Planitia
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