Mars InSight Mission
Skip Navigation
menu

INSIGHT MISSION IMAGES

Canyon Junction

A false-color mosaic focuses on one junction in Noctis Labyrinthus where Mars canyons meet to form a depression 4,000 meters (13,000 feet) deep.

April 01, 2012

Credit

NASA/JPL-Caltech/University of Arizona

ENLARGE

Related

NASA's Mars Odyssey spacecraft passes above a portion of the planet that is rotating into the sunlight in this artist's concept illustration. The spacecraft has been orbiting Mars since October ...
More
NASA's Mars Odyssey spacecraft passes above a portion of the planet that is rotating into the sunlight in this artist's concept illustration
Odyssey over Martian Sunrise, 3-D (Artist Concept)
Dr. Phil Varghese, Odyssey Project Manager.
More
Dr. Phil Varghese, Odyssey Project Manager.
Dr. Phil Varghese
Getting to Mars is difficult enough -- staying there is even more challenging. Odyssey met up with Mars on October 24 02:26 UTC (October 23: 7:26 p.m. PDT/10:26 p.m.EDT).
More
Orbit Insertion
Orbit Insertion
Fans and ribbons of dark sand dunes creep across the floor of Bunge Crater in response to winds blowing from the direction at the top of the picture.
More
Fans and ribbons of dark sand dunes creep across the floor of Bunge Crater in response to winds blowing from the direction at the top of the picture.
Mars Odyssey All Stars: Bunge Crater Dunes
Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is one of both tectonically fractured rocks (top of image) and volcanic flows (mi...
More
Echus Chasma forms the boundary between the Tharsis volcanoes to the west and Lunae Planum to the east. This region is one of both tectonically fractured rocks (top of image) and volcanic flows (middle and bottom of image). Echus Chasma empties into Kasei Valles.
Echus Chasma
A lunar eclipse, a solar eclipse and Mars has a close encounter with a comet.
More
What's Up for October?
What's Up for October?
This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.
More
This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.
Lismore Crater
This graphic depicts the relative shapes and distances from Mars for five active orbiter missions plus the planet's two natural satellites. It illustrates the potential for intersections of the spa...
More
This graphic depicts the relative shapes and distances from Mars for five active orbiter missions plus the planet's two natural satellites. It illustrates the potential for intersections of the spacecraft orbits.
Diverse Orbits Around Mars
This map shows unprecedented detail of local variations in Mars' gravitational pull on orbiters. The gravitational mapping has been applied to map variations in the thickness of the planet's crust ...
More
This map shows unprecedented detail of local variations in Mars' gravitational pull on orbiters. The gravitational mapping has been applied to map variations in the thickness of the planet's crust and to deduce information about its deeper interior.
Local Variations in the Gravitational Pull of Mars
This movie shows three views of the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter. The apparent motion is due to movement by Odyssey's infrared camera, Thermal ...
More
This movie shows three views of the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter.
Odyssey's Three Views of Phobos in Visible Light
The dune field in this polar region crater looks like a stubby arrow pointing the way west. This unnamed crater is located in Planum Chronium.
More
The dune field in this polar region crater looks like a stubby arrow pointing the way west. This unnamed crater is located in Planum Chronium.
Unnamed crater is located in Planum Chronium.
This image shows a 90-mile-wide portion of the giant Valles Marineris canyon system. Landslide debris and gullies in the canyon walls on Mars can be seen at 100 meters (330 feet) per pixel.
More
This image shows a 90-mile-wide portion of the giant Valles Marineris canyon system. Landslide debris and gullies in the canyon walls on Mars can be seen at 100 meters (330 feet) per pixel.
Close View of Valles Marineris
Colors in this image of the Martian moon Phobos indicate a range of surface temperatures detected by observing the moon on Sept. 29, 2017, with the Thermal Emission Imaging System (THEMIS) camera o...
More
Image Credit: NASA/JPL-Caltech/ASU
Martian Moon Phobos in Thermal Infrared Image
A large sandsheet with surface dune forms is shown in today's image of Aonia Terra.
More
A large sandsheet with surface dune forms is shown in today's image of Aonia Terra.
Dunes in Aonia Terra
This image is near the southern edge of a low, broad volcanic feature called Syrtis Major.
More
This image is near the southern edge of a low, broad volcanic feature called Syrtis Major. A close look at this image reveals a wrinkly texture that indicates a very rough surface that is associated with the lava flows that cover this region. On a larger scale, there are numerous bright streaks that trail topographic features such as craters. These bright streaks are in the wind shadows of the craters where dust that settles onto the surface is not as easily scoured away. It is important to note that these streaks are only bright in a relative sense to the surrounding image. Syrtis Major is one of the darkest regions on Mars and it is as dark as fresh basalt flows or dunes are on Earth.
Syrtis Major
Six views of the Martian moon Phobos captured by NASA's Odyssey orbiter as of March 2020. The orbiter's THEMIS camera is used to measure temperature variations that suggest what kind of material th...
More
Three views of the Martian moon Phobos
Odyssey's Six Views of Phobos
Download a PDF of the Mars as Art Booklet.
More
Mars as Art
Mars as Art (2013)
This view combines information from two instruments on NASA's Mars Reconnaissance Orbiter to map color-coded composition over the shape of the ground in a small portion of the Nili Fossae plains re...
More
This view combines information from two instruments on a NASA Mars orbiter to map color-coded composition over the shape of the ground within the Nili Fossae plains region of Mars. Carbonate-rich deposits in this area (coded green) hold some carbon formerly in the atmosphere's carbon dioxide.
Rocks Here Sequester Some of Mars' Early Atmosphere
A dust storm continues to envelop the Red Planet and Curiosity’s labs are back in action.
More
A dust storm continues to envelop the Red Planet and Curiosity’s labs are back in action.
Mars Report: July 2018
This is a Mars Odyssey visible color image of an unnamed crater in western Arcadia Planitia (near 39 degrees N, 179 degrees E). The crater shows a number of interesting internal and external featur...
More
This is a Mars Odyssey visible color image of an unnamed crater in western Arcadia Planitia (near 39 degrees N, 179 degrees E). The crater shows a number of interesting internal and external features that suggest that it has undergone substantial modification since it formed. These features include concentric layers and radial streaks of brighter, redder materials inside the crater, and a heavily degraded rim and ejecta blanket. The patterns inside the crater suggest that material has flowed or slumped towards the center. Other craters with features like this have been seen at both northern and southern mid latitudes The distribution of these kinds of craters suggests the possible influence of surface or subsurface ice in the formation of these enigmatic features. The image was taken on September 29, 2002 during late northern spring. This is an approximate true color image, generated from a long strip of visible red (654 nm), green (540 nm), and blue (425 nm) filter images that were calibrated using a combination of pre-flight measurements and Hubble images of Mars. The colors appear perhaps a bit darker than one might expect; this is most likely because the images were acquired in late afternoon (roughly 4:40 p.m. local solar time) and the low Sun angle results in an overall darker surface.
Western Arcadia Planitia
A small impact crater on Mars named Gratteri, 4.3 miles (6.9 km) wide, lies at the center of large dark streaks.
More
A small impact crater on Mars named Gratteri, 4.3 miles (6.9 km) wide, lies at the center of large dark streaks.
Mars Impact Crater Gratteri
The dunes and dust devil tracks in this VIS image are located on the plains of Planum Chronium.
More
The dunes and dust devil tracks in this VIS image are located on the plains of Planum Chronium.
Dunes and dust devil tracks in Planum Chronium
This mosaic image of Valles Marineris - colored to resemble the martian surface - comes from the Thermal Emission Imaging System (THEMIS), a visible-light and infrared-sensing camera on NASA's Mars...
More
This mosaic image of Valles Marineris - colored to resemble the martian surface - comes from the Thermal Emission Imaging System (THEMIS), a visible-light and infrared-sensing camera on NASA's Mars Odyssey orbiter.
The Grand Canyon of Mars-Valles Marineris
Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data from three different NASA Mars orbiters.
More
Researchers estimating the amount of carbon held in the ground at the largest known carbonate-containing deposit on Mars utilized data from five instruments on three different NASA Mars orbiters, including physical properties from THEMIS (left) and mineral information from CRISM (right).
Multiple Instruments Used for Mars Carbon Estimate
This view of an area about 140 kilometers (about 90 miles) wide in the Meridiani Planum region of Mars shows the region around NASA's Mars Exploration Rover Opportunity.
More
Orbital View of Opportunity's Region
Orbital View of Opportunity's Region

You Might Also Like

The six-wheeled scientist is heading south to explore Jezero Crater’s lakebed in search of signs of ancient microbial life.
More
NASA's Perseverance Rover Begins Its First Science Campaign on Mars
NASA's Perseverance Rover Begins Its First Science Campaign on Mars
The Red Planet rotorcraft headed south in support of furthering research into the potential use of aerial scouts on Mars in the future.
More
NASA's Ingenuity Mars Helicopter Completes First One-Way Trip
NASA's Ingenuity Mars Helicopter Completes First One-Way Trip
The Red Planet rotorcraft will shift focus from proving flight is possible on Mars to demonstrating flight operations that future aerial craft could utilize.
More
NASA's Ingenuity Helicopter to Begin New Demonstration Phase
NASA's Ingenuity Helicopter to Begin New Demonstration Phase
A livestream will begin at 3:15 a.m. PDT that morning as the helicopter team prepares to receive the data downlink at NASA’s Jet Propulsion Laboratory.
More
NASA to Attempt First Controlled Flight on Mars As Soon As Monday
NASA to Attempt First Controlled Flight on Mars As Soon As Monday
Now uncocooned from its protective carbon-fiber shield, the helicopter is being readied for its next steps.
More
NASA Ingenuity Mars Helicopter Prepares for First Flight
NASA Ingenuity Mars Helicopter Prepares for First Flight
The first trek of the agency’s largest, most advanced rover yet on the Red Planet marks a major milestone before science operations get under way.
More
NASA's Perseverance Drives on Mars' Terrain for First Time
NASA's Perseverance Drives on Mars' Terrain for First Time