Mars InSight Mission
Skip Navigation
menu

INSIGHT MISSION IMAGES

Dr. Bill Boynton

Dr. Bill Boynton, Principal Investigator for the Gamma Ray Spectrometer suite of instruments

August 24, 2004

Credit

NASA/JPL-Caltech

ENLARGE

Related

Mars Odyssey Project Manager Gaylon McSmith, of NASA's Jet Propulsion Laboratory
More
Mars Odyssey Project Manager Gaylon McSmith, of NASA's Jet Propulsion Laboratory
Mars Odyssey Project Manager Gaylon McSmith
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
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...
More
Challenges of Getting to Mars: Telecommunications
Challenges of Getting to Mars: Telecommunications
NASA is advancing the Journey to Mars by starting the conversation about where humans may one day land on the Red Planet.
More
This image shows the different exploration zones for Mars landing sites for human missions to the surface of Mars.
Mars Exploration Zone Layout Considerations
Although it is 45 kilometers (28 miles) wide, countless layers of ice and dust have all but buried Udzha Crater.
More
Although it is 45 kilometers (28 miles) wide, countless layers of ice and dust have all but buried Udzha Crater.
Mars Odyssey All Stars: Udzha Crater
NASA Science missions circle Earth, the Sun, the Moon, Mars and many other destinations within our solar system, including spacecraft that look out even further into our universe. The Science Fleet...
More
NASA Science missions circle Earth, the Sun, the Moon, Mars and many other destinations within our solar system, including spacecraft that look out even further into our universe. The Science Fleet depicts the scope of NASA's activity and how our missions have traveled throughout the solar system.
SMD Spacecraft Fleet
THEMIS Support for Landing Site Selection
More
THEMIS Support for Landing Site Selection
THEMIS Support for Landing Site Selection
The Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey spacecraft has completed an unprecedented full decade of observing Mars from orbit.
More
The Thermal Emission Imaging System (THEMIS) camera on NASA's Mars Odyssey spacecraft has completed an unprecedented full decade of observing Mars from orbit.
Tenth Anniversary Image from Camera on NASA Mars Orbiter
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
Large fractures have formed 'steps' in this region of Tempe Terra.
More
Large fractures have formed 'steps' in this region of Tempe Terra.
Tempe Terra
First THEMIS Image of Mars
More
First THEMIS Image of Mars
First THEMIS Image of Mars
This image superimposes Gamma-Ray Spectrometer data from NASA's Mars Odyssey orbiter onto topographic data from the laser altimeter on NASA's Mars Global Surveyor.
More
This image superimposes Gamma-Ray Spectrometer data from NASA's Mars Odyssey orbiter onto topographic data from the laser altimeter on NASA's Mars Global Surveyor.
Potassium Concentrations on Mars
West of Valles Marineris lies a checkerboard named Noctis Labyrinthus, which formed when the Martian crust stretched and fractured.
More
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
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
On the southwest edge of the immense volcanic region of Tharsis, lava from its giant volcanoes flowed down to meet the old cratered landscape of Terra Sirenum.
More
On the southwest edge of the immense volcanic region of Tharsis, lava from its giant volcanoes flowed down to meet the old cratered landscape of Terra Sirenum.
Terra Sirenum
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
More
This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
Oblique view of Gale Crater from the North
Artist rendering of commercial Mars satellites providing communications back to Earth.
More
Artist rendering of commercial Mars satellites providing communications back to Earth.
Artist's Concept of Mars Satellites
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
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
A sea of dark dunes, sculpted by the wind into long lines, surrounds the northern polar cap covering an area as big as Texas.
More
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
Continuing our survey of non-crater dune fields brings us to this group of dunes in Aonia Terra. The daytime IR illustrates the warmth of the dune material compared to the surrounding materials.
More
Continuing our survey of non-crater dune fields brings us to this group of dunes in Aonia Terra. The daytime IR illustrates the warmth of the dune material compared to the surrounding materials.
Aonia Terra Dunes
Sand-laden jets shoot into the polar sky in this view by noted space artist Ron Miller.
More
Sand-laden jets shoot into the polar sky in this view by noted space artist Ron Miller.
Sand-Laden Jets
This image captured by NASA's 2001 Mars Odyssey spacecraft shows 'streamers' of clouds created by katabatic winds at the north polar cap.
More
Polar Winds
Polar Winds
A false-color mosaic focuses on one junction in Noctis Labyrinthus where canyons meet to form a depression 4,000 meters (13,000 feet) deep.
More
A false-color mosaic focuses on one junction in Noctis Labyrinthus where canyons meet to form a depression 4,000 meters (13,000 feet) deep.
Mars Odyssey All Stars: Noctis Canyon
Just as on Earth, volcanism and tectonism are found together on Mars. Here is an example: the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Pl...
More
Just as on Earth, volcanism and tectonism are found together on Mars. Here is an example: the ridges and fractures of Claritas Fossae are affecting or perhaps hosting the volcanic flows of Solis Planum.
Volcanism & Tectonism

You Might Also Like

Through Nov. 1, K-12 students in the U.S. are encouraged to enter an essay contest to name NASA's next Mars rover.
More
NASA Invites Students to Name Mars 2020 Rover
NASA Invites Students to Name Mars 2020 Rover
The rover recently drilled two samples, and both showed the highest levels of clay ever found during the mission.
More
NASA's Curiosity Mars Rover Finds a Clay Cache
NASA's Curiosity Mars Rover Finds a Clay Cache
For the first time, NASA's Mars Odyssey orbiter has caught the Martian moon Phobos during a full moon phase. Each color in this new image represents a temperature range detected by Odyssey's infrared camera.
More
Why This Martian Full Moon Looks Like Candy
Why This Martian Full Moon Looks Like Candy
Nominees include four JPL projects: the solar system and climate websites, InSight social media, and a 360-degree Earth video. Public voting closes April 18, 2019.
More
NASA Garners 7 Webby Award Nominations
NASA Garners 7 Webby Award Nominations
NASA's Opportunity Mars rover mission is complete after 15 years on Mars. Opportunity's record-breaking exploration laid the groundwork for future missions to the Red Planet.
More
NASA's Opportunity Rover Mission on Mars Comes to End
NASA's Opportunity Rover Mission on Mars Comes to End
In deploying its first instrument onto the surface of Mars, the lander completes a major mission milestone.
More
NASA's InSight Places First Instrument on Mars
NASA's InSight Places First Instrument on Mars