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CTX Mosaic Shows Geographic Locations on Mars

The Global CTX Mosaic of Mars allows scientists and the public to explore the planet like never before.

April 05, 2023

The Global CTX Mosaic of Mars allows scientists and the public to explore the planet like never before. It includes different layers of data that can be turned on or off, like these labels for named geographic features on the planet.

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NASA/JPL-Caltech/MSSS

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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...
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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 drilled holes where 15 rock-powder samples were acquired, most recently at "Sebina," on Oct. 20, 2016.
Curiosity's Rock or Soil Sampling Sites on Mars, Through November 2016
From one side of the country to the other, through a snowstorm and other delays, the Mars Reconnaissance Orbiter made its way to Kennedy Space Center in Florida for final processing and rehearsals ...
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Challenges of Getting to Mars: Getting to the Launch Pad
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This HiRISE image covers the southwest portion of the terraces and floor of Holden Crater situated in southwest Margaritifer Terra.
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This HiRISE image covers the southwest portion of the terraces and floor of Holden Crater situated in southwest Margaritifer Terra.
Holden Crater Megabreccia: A Telltale Sign of a Sudden and Violent Event
The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) aboard NASA's Mars Reconnaissance Orbiter obtained this spectrum for comet C/2013 A1 Siding Spring during the comet's close approach...
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The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) aboard NASA's Mars Reconnaissance Orbiter obtained this spectrum for comet C/2013 A1 Siding Spring during the comet's close approach to Mars.
Mars-Orbiting Spectrometer Shows Dusty Comet's Spectrum
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...
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Estimated Water Depths in Ancient Martian Sea
Estimated Water Depths in Ancient Martian Sea
This HiRISE image shows erosional features formed by seasonal frost near the south pole of Mars.
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This HiRISE image shows erosional features formed by seasonal frost near the south pole of Mars.
Erosion Features near the South Pole of Mars
This graphic shows the route that NASA's Mars Exploration Rover Opportunity drove in its final approach to "Perseverance Valley" on the western rim of Endeavour Crater during spring 2017.
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This graphic shows the route that NASA's Mars Exploration Rover Opportunity drove in its final approach to "Perseverance Valley" on the western rim of Endeavour Crater during spring 2017.
From 'Tribulation' to 'Perseverance' on Mars
This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles).
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This image is of a portion of the Southern plains region within Hellas, the largest impact basin on Mars, with a diameter of about 2300 kilometers (1400 miles).
Pitted Landforms in Southern Hellas Planitia
This map of the region around NASA's Mars Exploration Rover Opportunity shows the relative locations of several craters and the rover in May 2010.
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Opportunity Rover Amid Mars Craters
Opportunity Amid Mars Craters
Crater in Thaumasia Fossae
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Crater in Thaumasia Fossae
Crater in Thaumasia Fossae
Mars Reconnaissance Orbiter is Off to Mars!
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Mars Reconnaissance Orbiter is Off to Mars!
Mars Reconnaissance Orbiter is Off to Mars!
This map shows five locations where fresh impact cratering has excavated water ice from just beneath the surface of Mars (sites 1 through 5) and the Viking Lander 2 landing site (VL2), in the conte...
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Expected Depths to Ice, Mid-Latitude Northern Mars
Expected Depths to Ice, Mid-Latitude Northern Mars
These dark streaks, also known as “slope streaks,” resulted from dust avalanches on Mars. The HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter captured them on Dec. 26, 2017.
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These dark streaks, also known as “slope streaks,” resulted from dust avalanches on Mars. The HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter captured them on Dec. 26, 2017.
HiRISE Spots Slope Streaks Fanning Out on Mars
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...
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The formation of the large outflow channels on Mars have been attributed to catastrophic discharges of ground water. Many of the channels start in areas where the ground has apparently collapsed: the surface is now well below the surrounding undisturbed ground. Within the collapsed region, blocks of undisturbed material can often be seen and this has led to such regions being called chaotic terrain. 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 shows such an outcrop in a chaotic terrain region. At the highest resolution, layering can be seen. The image will be used to assess at what stage in Mars's history these clays minerals were formed and how. The area referred to as Aureum Chaos is located at 334 degrees East, 4 degrees South on the West side of the Margaritifer Terra region of Mars.
Light-Toned Outcrop in Aureum Chaos
Details such as the shadow of the mast on NASA's Mars rover Curiosity appear in an image taken Aug. 17, 2012, by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconn...
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Details such as the shadow of the mast on NASA's Mars rover Curiosity appear in an image taken Aug. 17, 2012, by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter, from more directly overhead than previous HiRISE images of Curiosity.
Orbiter View of Curiosity From Nearly Straight Overhead
Several types of downhill flow features have been observed on Mars. This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is an exampl...
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Several types of downhill flow features have been observed on Mars. This image from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter is an example of a type called "linear gullies."
Linear Gullies Inside Russell Crater, Mars
Shalbatana Vallis is a large channel with steep walls and a flat floor that may have formed by water draining from nearby Ganges Chasma. Here a section of the wall collapsed and produced a landslid...
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Shalbatana Vallis is a large channel with steep walls and a flat floor that may have formed by water draining from nearby Ganges Chasma.
Landslide in Shalbatana Vallis (3-D)
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...
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a concentrated cloud of dust on Mars
A Mars Dust Tower Stands Out
Deposits on the floor of Palos Crater
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Deposits on the floor of Palos Crater
Deposits on the floor of Palos Crater
This global map of Mars was acquired on July 31, 2012, by the Mars Color Imager instrument on NASA's Mars Reconnaissance Orbiter.
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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 image, taken with the High Resolution Imaging Science Experiment (HiRISE) camera, shows a mesa within the "Murray Buttes" area on Mars showing a complex fracture pattern (black arrow) protrudi...
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This image shows a mesa (grayish) within the "Murray Buttes" area on Mars showing a complex fracture pattern (black arrow) protruding from the eroding rock.
'Murray Buttes' Mesa
An oblique, northward-looking view based on stereo orbital imaging, shows the location of Opportunity on its journey from Cape York to Solander Point when HiRISE took the new color image.
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An oblique, northward-looking view based on stereo orbital imaging, shows the location of Opportunity on its journey from Cape York to Solander Point when HiRISE took the new color image.
Location of Opportunity Rover
The Mars Reconnaissance Orbiter took this photo of the Curiosity rover in September 2015, as Curiosity was exploring the boundary between two rock units: the light-toned Murray Formation and the ov...
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The Mars Reconnaissance Orbiter took this photo of the Curiosity rover in September 2015, during an exciting traverse of Mars.
Mars Reconnaissance Orbiter Checks Curiosity's Trek
Dunes on Floor of Samara Valles, Mars
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Dunes on Floor of Samara Valles, Mars
Dunes on Floor of Samara Valles, Mars
Lucus Planum is a part of the enigmatic Medusa Fossae Formation, a broad, soft, and easily eroded deposit. Here this deposit is thin and considerably rougher than elsewhere, implying that it is hea...
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Lucus Planum is a part of the enigmatic Medusa Fossae Formation, a broad, soft, and easily eroded deposit.
Channel in Lucus Planum (3-D)

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