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Storm Chaser on Mars
March 20, 2012
Mars Reconnaissance Orbiter Catches a Twister in Action.
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This global map of Mars was acquired on July 31, 2012, by the Mars Color Imager instrument on NASA's Mars Reconnaissance Orbiter.
Mars Weather Map, July 31
This graph shows a spectrum recorded by the Chemistry and Camera instrument (ChemCam) in NASA's Curiosity Mars rover.
ChemCam Spectrum from Martian Rock Target 'Ithaca'
This 3D, or stereo anaglyph, view shows the parachute and back shell that helped guide NASA's Curiosity to the surface of Mars. The view was produced from images taken by the High Resolution Imagin...
Parachute and Back Shell in 3-D
This April 6, 2014, image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter shows numerous landslides in the vicinity of where an impact crat...
Landslides Near Fresh Crater on Mars
This sinuous raised ridge is thought to be an inverted stream channel. These are formerly low-lying streambeds that became elevated because the original depression is filled with materials (such a...
Sinuous Ridge in the Aeolis Region (3-D)
NASA's Phoenix Mars Lander, its backshell and its heatshield are visible within this enhanced-color image of the Phoenix landing site taken on Jan. 6, 2010 by the High Resolution Imaging Science Ex...
Phoenix Lander Amid Disappearing Spring Ice
This proposed future Mars landing site in Acidalia Planitia targets densely occurring mounds thought to be mud volcanoes.
Proposed Future Mars Landing Site: Acidalia Planitia Mud Volcanoes
This area of Mars is shaped by lava flows from volcanic eruptions.
Flow and Flow Features in Amazonis Planitia
Gullies and Flow Features along Crater Wall in Promethei Terra
Gullies and Flow Features along Crater Wall in Promethei Terra
A dune in the northern polar region of Mars shows significant changes between two images taken on June 25, 2008 and May 21, 2010 by NASA's Mars Reconnaissance Orbiter.
Movement in Martian Dune Field
This series of images shows warm-season features that might be evidence of salty liquid water active on Mars today.
Dark Flows in Newton Crater Extending During Summer (Six-Image Sequence)
NASA's Curiosity Mars rover can be seen in this image taken from space on May 31, 2019, by the HiRISE camera aboard the Mars Reconnaissance Orbiter. In the image, Curiosity appears as a bluish speck.
HiRISE Spots Curiosity Rover at Mars' 'Woodland Bay'
As on the Earth, many processes can move material down a Martian slope. This graphic compares seven different types of features observed on Mars that appear to result from material flowing or slidi...
Martian Features Formed When Material Moves Downslope
This picture of a crater resembling a "happy face" was taken by the Mars Reconnaissance Orbiter's Context Camera. The unnamed crater is almost 2 miles (about 3 kilometers) across That's a BIG smile!
A Smile a Day....
Curiosity performs the first investigation of active sand dunes on another planet. Studying the Bagnold Dunes on Mars will help scientists understand the physics of Martian dunes and how they move.
Curiosity Rover Report (Dec. 15, 2015): First Visit to Martian Dunes
The enhanced-color subimage shows a great variety of colors and textures in the bedrock, where it is exposed from beneath a dark fine-grained mantle. The mantle is sometimes modified by the wind in...
Uplifted Jumble of Ancient Bedrock (3-D)
The black speck circled in the lower left corner of this image is a cluster of recently formed craters spotted on Mars using a new machine-learning algorithm. This image was taken by the Context Ca...
Machine Learning Spots a Cluster of Mars Craters: Context Camera's View
A small channel cuts across the floor of a gigantic 1100-mile (1780-kilometer)-long set of flood-carved channels in a region on Mars called "Kasei Valles."
Lava Coating, Flood-Carved Kasei Valles (3-D)
This image, acquired on May 15, 2018, by NASA's Mars Reconnaissance Orbiter, shows relatively bright mounds scattered throughout darker and diverse surfaces in Chryse Planitia.
Pitted Cones: Possible Methane Sources?
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
Common to the northern plains of Mars are rock and boulder strewn landscapes otherwise devoid of major features except a few impact craters. This image in the Cydnus Rupes region of northern Utopia...
Boulder Strewn Plain in Northern Utopia Planitia
This map shows the route driven by NASA's Mars rover Curiosity through the 29th Martian day, or sol, of the rover's mission on Mars (Sept. 4, 2012).
Curiosity Traverse Map Through Sol 29
Small impact craters usually have simple bowl shapes, but sometimes more complicated shapes can occur if the target is unusual.
Craters in an Icy Surface
This HiRISE image shows diverse layers in a region near Mawrth Vallis, a channel that was probably carved by water in Mars' ancient past. The color subimage shows details of layers exposed in a cra...
Diverse Layers and Mineralogy Near Mawrth Vallis (3-D)
NASA's Curiosity Mars rover and tracks left by its driving appear in this portion of a Dec. 11, 2013, observation by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Re...
Curiosity Trekking, Viewed from Orbit in December 2013
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A pair of quakes in 2021 sent seismic waves deep into the Red Planet’s core, giving scientists the best data yet on its size and composition.
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Ten sample tubes, capturing an amazing variety of Martian geology, have been deposited on Mars’ surface so they could be studied on Earth in the future.
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Filled with rock, the sample tube will be one of 10 forming a depot of tubes that could be considered for a journey to Earth by the Mars Sample Return campaign.
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The mission has concluded that the solar-powered lander has run out of energy after more than four years on the Red Planet.
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The 10 sample tubes being dropped on Mars’ surface so they can be studied on Earth in the future carry an amazing diversity of Red Planet geology.
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