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Planum Boreum crater

Planum Boreum crater

March 03, 2003

Planum Boreum crater

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NASA/JPL-Caltech/ASU

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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...
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Image Credit: NASA/JPL-Caltech/ASU
Martian Moon Phobos in Thermal Infrared Image
Mars radiation levels are two to three times higher than around Earth.
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Mars radiation levels are two to three times higher than around Earth.
Mars radiation levels
How do you converse with a robot nearly one hundred million miles away? In this video, Odyssey team members describe communications with the 2001 Mars Odyssey spacecraft using the antennas of the D...
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Challenges of Getting to Mars: Telecommunications
Challenges of Getting to Mars: Telecommunications
Fly Through Mariner Valley
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Fly Through Mariner Valley
Fly Through Mariner Valley
This movie shows the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter on April 24, 2019. The apparent motion is due to movement by Odyssey's infrared camera, Therm...
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This movie shows the Martian moon Phobos as viewed in visible light by NASA's 2001 Mars Odyssey orbiter.
Odyssey Views Phobos in Visible Light: April 24, 2019
Newly detailed mapping of local variations in Mars' gravitational pull on orbiters (center), combined with topographical mapping of the planet's mountains and valleys (left), yields the best-yet ma...
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Newly detailed mapping of local variations in Mars' gravitational pull on orbiters (center), combined with topographical mapping of the planet's mountains and valleys (left), yields the best-yet mapping of Mars' crustal thickness (right).
Using Gravity and Topography to Map Mars' Crustal Thickness
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.
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Orbital View of Opportunity's Region
Orbital View of Opportunity's Region
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 ...
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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)
NASA's Mars Odyssey spacecraft passes above Mars' south pole in this artist's concept illustration. The spacecraft has been orbiting Mars since October 24, 2001.
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NASA's Mars Odyssey spacecraft passes above Mars' south pole in this artist's concept illustration. The spacecraft has been orbiting Mars since October 24, 2001.
Odyssey over Mars' South Pole
This map of Mars indicates locations of new craters that have excavated ice (blue) and those that have not (red). The underlying map is based on the brightness, or albedo, of the Martian surface.
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This map of Mars indicates locations of new craters that have excavated ice (blue) and those that have not (red). The underlying map is based on the brightness, or albedo, of the Martian surface.
Locations of Ice-Exposing Fresh Craters on Mars
Taken on April 24, 2019, this rainbow-colored image shows the Martian moon Phobos, as viewed by NASA's 2001 Mars Odyssey orbiter using its infrared camera, THEMIS. Each color represents a different...
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Martian moon Phobos viewed by Mars Odyssey orbiter using its infrared camera.
Odyssey Views Phobos: April 24, 2019
Dr. Bill Boynton, Principal Investigator for the Gamma Ray Spectrometer suite of instruments Image credit: NASA/JPL
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Dr. Bill Boynton, Principal Investigator for the Gamma Ray Spectrometer suite of instruments
Dr. Bill Boynton
A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 meters (3,300 feet) wide.
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A vast dune field lies near the northern polar cap of Mars. Seen here in summer, the dunes have partially buried an impact crater about 1,000 meters (3,300 feet) wide.
Mars Odyssey All Stars: Dunes Engulf Crater
Gale Crater, home to NASA's Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA's Mars Odyssey orbiter.
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Gale Crater, home to NASA's Curiosity Mars rover, shows a new face in this image made using data from the THEMIS camera on NASA's Mars Odyssey orbiter.
Gale Crater's Surface Materials
This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT) and the location where Curiosity collected its first drill...
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This false-color map shows the area within Gale Crater on Mars, where NASA's Curiosity rover landed on Aug. 5, 2012 PDT (Aug. 6, 2012 EDT) and the location where Curiosity collected its first drilled sample at the "John Klein" rock.
Location of John Klein Drill Site
A sea of dark dunes, sculpted by the wind into long lines, surrounds the northern polar cap covering an area as big as Texas.
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A sea of dark dunes, sculpted by the wind into long lines, surrounds the northern polar cap covering an area as big as Texas.
Mars Odyssey All Stars: Polar Dunes
This image captured by NASA's 2001 Mars Odyssey spacecraft shows a section of Nanedi Valles, located in Xanthe Terra.
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Nanedi Valles
Nanedi Valles
Chasma Boreale is a long, flat-floored valley that cuts deep into Mars' north polar icecap
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Chasma Boreale is a long, flat-floored valley that cuts deep into Mars' north polar icecap
Mars Odyssey All Stars: Chasma Boreale
This animation shows how NASA's Curiosity rover communicates with Earth via two of NASA's Mars orbiters, Mars Reconnaissance Orbiter (MRO) and Odyssey, and the European Space Agency's Mars Express....
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Curiosity Communicates with Help From Its 'Friends'
Curiosity Communicates with Help From Its 'Friends'
Although this may look like a hostile alien life form, it's actually a complex line of sand dunes near the northern ice cap of Mars.
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Although this may look like a hostile alien life form, it's actually a complex line of sand dunes near the northern ice cap of Mars.
Mars Odyssey All Stars: Reptilian Dunes
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.
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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
West of Valles Marineris lies a checkerboard named Noctis Labyrinthus, which formed when the Martian crust stretched and fractured.
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West of Valles Marineris lies a checkerboard named Noctis Labyrinthus, which formed when the Martian crust stretched and fractured.
Mars Odyssey All Stars: Noctis Vista
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...
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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
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the margin of the north polar cap and the surrounding plains. The layering of the ice is easily visible due to the dust that is dep...
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This image from NASA's 2001 Mars Odyssey spacecraft shows part of the margin of the north polar cap and the surrounding plains. The layering of the ice is easily visible due to the dust that is deposited on the top of the ice every year, creating layering over millions of years.
Polar Layers
This pair of maps indicates locations of confirmed sites of recurrent slope linea on Mars, with respect to elevation (upper map) and surface brightness, or albedo (lower map).
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This pair of maps indicates locations of confirmed sites of recurrent slope linea on Mars, with respect to elevation (upper map) and surface brightness, or albedo (lower map).
Maps of Recurrent Slope Linea Markings on Mars

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