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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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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 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).
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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).
Downslope of the Fan
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
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
These three views of the Martian moon Phobos were taken by NASA's 2001 Mars Odyssey orbiter using its infrared camera, THEMIS. Each color represents a different temperature range.
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Three views of the Martian moon Phobos taken by NASA's 2001 Mars Odyssey orbiter using its infrared camera.
Odyssey's Three Views of Phobos
This image combines two products from the first pointing at the Martian moon Phobos by the THEMIS camera on NASA's Mars Odyssey orbiter, on Sept. 29, 2017. Surface-temperature information from obse...
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Temperature Gradient on Martian Moon Phobos
Temperature Gradient on Martian Moon Phobos
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 ...
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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
Interact with this 3D model of Mars Odyssey.
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3D model of Odyssey
Mars Odyssey Orbiter, 3D Model
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
The annotated area of Mars in this illustration holds near-surface water ice that would be easily accessible for astronauts to dig up. The water ice was identified as part of a map using data from ...
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The annotated area of Mars in this illustration holds near-surface water ice that would be easily accessible for astronauts to dig up. The water ice was identified as part of a map using data from NASA orbiters.
Water Ice Marked on Mars Globe
This artist's animation shows how orbiters over Mars will monitor the landing of NASA's Curiosity rover. (No audio)
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Great Convergence of Spacecraft around Mars
Great Convergence of Spacecraft around Mars
How can you communicate with Mars spacecraft when the Sun is in the way? Learn more about 'solar conjunction' in this 60-second video.
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Mars in a Minute: What Happens When the Sun Blocks our Signal?
Mars in a Minute: What Happens When the Sun Blocks our Signal?
Phobos and Deimos, the moons of Mars, are seen in this image from NASA's 2001 Mars Odyssey orbiter. The distance to Deimos from Odyssey during the observation was about 12,222 miles (19,670 kilomet...
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Mars Odyssey Observes Martian Moons
Mars Odyssey Observes Martian Moons
In Ares Vallis, teardrop mesas extend like pennants behind impact craters, where the raised rocky rims diverted the floods and protected the ground from erosion.
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In Ares Vallis, teardrop mesas extend like pennants behind impact craters, where the raised rocky rims diverted the floods and protected the ground from erosion.
Mars Odyssey All Stars: Ares Vallis
Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike.
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Geological faulting has opened cracks in the Cerberus region that slice through flat plains and mesas alike.
Mars Odyssey All Stars: Cerberus Crack
Mars program Chief Engineer Robert Shotwell describes Mars Odyssey's unprecedented view of comet Siding Spring as the comet sweeps by the Red Planet on Oct. 19 and how it will maneuver to take images.
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NASA's Mars Odyssey Maneuvers to Image Comet Siding Spring
NASA's Mars Odyssey Maneuvers to Image Comet Siding Spring
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
This unnamed channel drains part of Margaritifer Terra.
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This unnamed channel drains part of Margaritifer Terra.
Channel in Margaritifer Terra.
The floor of this crater in Terra Sirenum contains layered material. The layered sedimentary material on Mars is arguably the most interesting and compelling material on the planet. These layers mo...
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The floor of this crater in Terra Sirenum contains layered material. The layered sedimentary material on Mars is arguably the most interesting and compelling material on the planet. These layers most likely contain the answers to fundamental questions about Martian geology, climate, and possibly even biology.
Terra Sirenum Crater
Download a PDF of the 2001 Mars Odyssey Launch Press Kit.
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Odyssey launch press kit
2001 Mars Odyssey Launch Press Kit
Valles Marineris, the "Grand Canyon of Mars," sprawls wide enough to reach from Los Angeles to nearly New York City, if it were located on Earth. The red outline box shows the location of a second,...
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Valles Marineris, the "Grand Canyon of Mars," sprawls wide enough to reach from Los Angeles to nearly New York City, if it were located on Earth. The red outline box shows the location of a second, full-resolution image.
Valles Marineris, the "Grand Canyon of Mars"
Ius Chasma is unique from the other chasmata of Valles Marineris in possessing mega gullies on both sides of the chasma. This image was captured by NASA's 2001 Mars Odyssey spacecraft.
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Investigating Mars: Ius Chasma
Investigating Mars: Ius Chasma
This series of images was taken in visible-wavelength light as the THEMIS camera on NASA's Mars Odyssey scanned across the Martian moon Phobos on Sept. 29, 2017. The apparent motion is due to progr...
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Series of Images from THEMIS Scanning Phobos
Series of Images from THEMIS Scanning Phobos
This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.
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This crater, located in Chryse Planitia, is relatively unmodified, meaning it appears very much like it did when it first formed.
Lismore Crater
The artist's animation depicts how NASA's Curiosity rover will communicate with Earth during landing. As the rover descends to Mars, it will send out basic radio-frequency tones that go directly to...
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Curiosity Speaks
Curiosity Speaks

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