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Artist concept of Mars Reconnaissance Orbiter
July 14, 2009
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NASA/JPL-Caltech
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This area at the base of Mount Sharp on Mars includes a pale outcrop, called "Pahrump Hills," that NASA's Curiosity Mars rover investigated from September 2014 to March 2015, and the "Artist's Driv...
Curiosity Heading Away from 'Pahrump Hills'
Well-Preserved Crater with Central Peak in Chryse Planitia
Well-Preserved Crater with Central Peak in Chryse Planitia
The Coloe Fossae region is a series of enclosed, intersecting canyons. The floors of the canyons in this image contain complex set of ridges and grooves that are generally parallel to the canyon wa...
Coloe Fossae Region (3-D)
These long, smooth features are sand ridges shaped by the constant martian wind. They run perpendicular, or at right angles to, the direction of the wind and often found in channels and crater inte...
MRO Spots Sand Stripes
The annotated area of Mars in this illustration holds near-surface water ice that would be easily accessible for astronauts to dig up. The water ice was identified as part of a map using data from ...
Water Ice Marked on Mars Globe
Why does HiRISE take so many repeat images of the same area? Repeat coverage actually serves a special purpose, such as detecting seasonal changes (frost deposition and sublimation) and temporal ch...
Frost on Crater Slope
This comparison of before-and-after images shows two spots that likely appeared in connection with the Oct. 19, 2016, Mars arrival of the European Space Agency's Schiaparelli test lander. The image...
Signs of Schiaparelli Test Lander Seen From Orbit
NASA's Mars Exploration Rover Opportunity has been on the western rim of Endeavour Crater in Meridiani Planum for about two years.
Color View From Orbit Showing Opportunity in 'Botany Bay' (Unannotated)
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
NASA’s Mars Reconnaissance Orbiter captured this image of a meteoroid impact that was first detected by the agency’s InSight lander using its seismometer. This crater was formed on Aug. 30, 2021.
InSight-Detected Impact in August 2021
Intra-Crater Structure in NW Hellas Basin, Mars
Intra-Crater Structure in NW Hellas Basin, Mars
Tantalus Fossae are a set of faults on the eastern flank of Alba Mons, one of the great Tharsis Montes volcanoes. Here a fault cuts into this crater, indicating that the fault formed after the crat...
Crater in Tantalus Fossae (3-D)
This map of Mars shows relative locations of three types of findings related to salt or frozen water, plus a new type of finding that may be related to both salt and water.
Ice, Salt and Warm-Season Flows on Mars
This image shows layered blocks tilted at high angles, diverse color and textures and dark dunes. Some of the bedrock may have originated at great depths, uplifted first by Becquerel Crater and lat...
Tilted and Layered Bedrock Blocks in a Large Crater inside Becquerel Crater (3-D)
This image contrasts gullies and recurring warm-season slope flows appearing in the same crater, in the middle southern latitudes of Mars.
Gullies and Newly Identified Flow Features in Same Mars Crater
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'
The largest crater in this mosaic of images taken by the Context Camera on NASA's Mars Reconnaissance Orbiter is Endeavour Crater, which is 22 kilometers (14 miles) in diameter.
Endeavour Crater in Context
The long, sinuous raised ridges on this fan of material are thought to be inverted stream channels. These ridges may have been low-lying streambeds that hardened and then turned into ridges when th...
Fan in the Aeolis Region (3-D)
This series of images shows warm-season features that might be evidence of salty liquid water active on Mars today.
Warm-Season Flows in Well-Preserved Crater in Terra Sirenum (Six-Image Sequence)
NASA's Mars Reconnaissance Orbiter has revealed Martian rocks containing a hydrated mineral similar to opal. The rocks are light-toned and appear cream-colored in this false-color image taken by th...
Gemstone of the Year - Labeled
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
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 image acquired on January 27, 2019 by NASAs Mars Reconnaissance Orbiter, shows the extensive central peak complex of Hale Crater.
Bedrock in the Central Peaks of Hale Crater
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 mid-November 2015, approaching examples of dunes in the "Bagnold D...
Curiosity Rover's Traverse, First 1,163 Sols on Mars
Eberswalde Crater was one of the four final landing sites considered for the MSL rover. A channel leads into the crater and the lithified remains of a delta, a fan-like feature formed when sediment...
Eberswalde Delta (3-D)
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