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Student Teams Work As Real Scientists

Ninth-grade, high-school students from Peoria, AZ analyze images of Mars.

February 21, 2013

Ninth-grade, high-school students from Peoria, AZ analyze images of Mars.

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NASA/JPL-Caltech/ASU

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This computer-generated view based on multiple orbital observations shows Mars' Gale crater as if seen from an aircraft north of the crater.
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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 (Unannotated)
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.
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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.
Canyon Junction
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
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.
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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 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
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...
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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
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
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)
A small impact crater on Mars named Gratteri, 4.3 miles (6.9 km) wide, lies at the center of large dark streaks.
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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
Sixteen seventh-graders at Evergreen Middle School in Cottonwood, Calif., found the Martian pit feature at the center of the superimposed red square in this image while participating in a program t...
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Martian Pit Feature Found by Seventh Graders
Martian Pit Feature Found by Seventh Graders
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 ...
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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
Odyssey launched on Boeing's Delta II 7925 that uses nine strap-on solid rocket motors.
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Odyssey launched on Boeing's Delta II 7925 that uses nine strap-on solid rocket motors.
Odyssey Launches Boeing's Delta II 7925
2906_HighViewOfMidCanyonMelas.jpg
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2906_HighViewOfMidCanyonMelas.jpg
High View of Melas
This image from NASA's Mars Odyssey shows ice-rich clouds over the summit of Arsia Mons.
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This is an image of ice-rich clouds in false color, taken by the Odyssey satellite orbiting Mars.
Ice-Rich Clouds - False Color
The channels in this VIS image are part of Tyrrhena Fossae on the northern flank of Tyrrhenus Mons.
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The channels in this VIS image are part of Tyrrhena Fossae on the northern flank of Tyrrhenus Mons.
Tyrrhena Fossae
This image from NASAs Mars Odyssey shows lava flows from Alba Mons, and a tectonic graben called Cyane Fossae.
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This image from NASAs Mars Odyssey shows lava flows from Alba Mons, and a tectonic graben called Cyane Fossae.
Alba Mons
This mosaic of infrared images shows the abundance and location of hematite at Opportunity's landing site, Meridiani Planum. On Earth, hematite is a mineral that typically forms in water.
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This mosaic of infrared images shows the abundance and location of hematite at Opportunity's landing site, Meridiani Planum. On Earth, hematite is a mineral that typically forms in water.
Meridiani Planum
This lava channel is part of the Elysium Mons flows.
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This lava channel is part of the Elysium Mons flows.
Lava Channel
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 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...
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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
At 11:02 a.m. EDT on April 7, 2001, crowds watch a Boeing Delta II rocket lift off from Cape Canaveral Air Force Station, Florida, carrying NASA's 2001 Mars Odyssey spacecraft into space on its sev...
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At 11:02 a.m. EDT on April 7, 2001, crowds watch a Boeing Delta II rocket lift off from Cape Canaveral Air Force Station, Florida, carrying NASA's 2001 Mars Odyssey spacecraft into space on its seven-month journey to Mars.
Odyssey's Launch to Mars on April 7, 2001
At the time this video was released, the Odyssey team had successfully completed the third trajectory correction maneuver to adjust the spacecraft's flightpath toward its final aimpoint for entry i...
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Challenges of Getting to Mars: Interplanetary Cruise
Challenges of Getting to Mars: Interplanetary Cruise
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.
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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
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...
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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

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