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Storm Chaser on Mars
March 20, 2012
Mars Reconnaissance Orbiter Catches a Twister in Action.
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This crater, formed in 2008, exposes shallow, clean ice that is not uncommon in the middle-to-high latitudes on Mars.
Icy New Impact
This image from the HiRISE camera on NASA's Mars Reconnaissance Orbiter shows a location associated with the novel and movie, "The Martian." It is the tale's planned landing site for the Ares 4 mis...
'The Martian' Story's Ares 4 Landing Site
This image reveals exposed layers in Noctis Labyrinthus which may contain signatures of iron bearing sulfates and phyllosilcate (clay) minerals.
Eastern Floor of Aram Chaos
A rippled dune front in Herschel Crater on Mars moved an average of about one meter (about one yard) between March 3, 2007 and December 1, 2010, as seen in these images from NASA's Mars Reconnaissa...
Rippling Dune Front in Herschel Crater on Mars
There are steep scarps facing the poles of both hemispheres that expose thick (up to 100 meters or more) sections of nearly pure water ice.
Ice-Exposing Scarps
Unfrozen brine in cryopegs and fracture networks provides habitats for the survival and growth of organisms both within and under frozen rocky materials on Earth and, by analogy, could provide habi...
Plausible Martian Habitats
This scene shows dark sand dunes marching over the ridges created by an alluvial (water-deposited) fan in an impact crater.
Dunes on Ridges
These images from the NASA Mars Reconnaissance Orbiter show several impact scars on Mars made by pieces of the NASA Mars Science Laboratory spacecraft that the spacecraft shed just before entering ...
Impact Scars from MSL Cruise Stage and Two Balance Weights
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 a spectrum recorded by the Chemistry and Camera instrument (ChemCam) in NASA's Curiosity Mars rover.
ChemCam Spectrum from Martian Rock Target 'Ithaca'
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
A new map of Mars' gravity made with three NASA spacecraft is the most detailed to date, providing a revealing glimpse into the hidden interior of the Red Planet. Satellites always orbit a planet's...
Mars Gravity Map
Download a PDF of the Mars Reconaissance Orbiter Fact Sheet.
Mars Reconnaissance Orbiter Fact Sheet
This image acquired on October 28, 2018 by NASAs Mars Reconnaissance Orbiter, shows that gullies probably formed along the bouldery layers in the upper slopes of this unnamed crater.
Multi-Elevation Gullies
The smaller, narrow ridges oriented vertically are yardangs, which are created by wind erosion; the wind strips away the surrounding terrain, and the ridges remain because they contain more hardene...
Meanders and Tributaries in Ridge Form in the Zephyria Region (3-D)
This mosaic, taken with the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter, shows the planned route (in yellow) of NASA's Curiosity rover from "Pah...
Curiosity Rover Planned Route
This movie sequence of images from NASA's Mars Reconnaissance Orbiter (MRO) shows comet C/2013 A1 Siding Spring before and after its close pass by Mars in October 2014. False color enhances subtle ...
Mars-Flyby Comet in False Color
NASA's Curiosity rover and its parachute were spotted by NASA's Mars Reconnaissance Orbiter as Curiosity descended to the surface on Aug. 5 PDT (Aug. 6 EDT).
Curiosity Spotted on Parachute by Orbiter
Dark, narrow streaks on Martian slopes such as these at Hale Crater are inferred to have been formed by seasonal flow of water on contemporary Mars. Detection of hydrated salts at the streaks suppo...
Recurring 'Lineae' on Slopes at Hale Crater, Mars
CRISM observations of this region of the Noctis Labyrinthus formation have shown indications of iron-bearing sulfates and phyllosilicate (clay) minerals.
MRO Sees Light-Toned Deposits in Noctis Labyrinthus
Recurring slope lineae (RSL) are active flows on warm Martian slopes that might be caused by seeping water.
Seasonal Flows in the Central Mountains of Hale Crater
Mysterious features on slopes hint there could be water flows on Mars.
Possible Water Flows on Mars
This color view of the parachute and back shell that helped deliver NASA's Curiosity rover to the surface of the Red Planet was taken by the High-Resolution Imaging Science Experiment (HiRISE) came...
Relics of Rover's Landing
A newly found, buried deposit of frozen carbon dioxide -- dry ice -- near the south pole of Mars contains about 30 times more carbon dioxide than previously estimated to be frozen near the pole.
Thickness Map of Buried Carbon-Dioxide Deposit
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
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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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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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