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Mars Odyssey Project Manager Gaylon McSmith

Mars Odyssey Project Manager Gaylon McSmith, of NASA's Jet Propulsion Laboratory

October 15, 2010

Mars Odyssey Project Manager Gaylon McSmith, of NASA's Jet Propulsion Laboratory

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NASA/JPL-Caltech

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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.
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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
Olympica Fossae is a complex channel located on the volcanic plains between Alba Mons and Olympus Mons. The sinuosity of the large channel in the middle of this image from NASA's 2001 Mars Odyssey ...
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Olympica Fossae
Olympica Fossae
This image is near the southern edge of a low, broad volcanic feature called Syrtis Major.
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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
Interact with this 3D model of Mars Odyssey.
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3D model of Odyssey
Mars Odyssey Orbiter, 3D Model
When the Mars Exploration Rover, Opportunity, landed on Meridiani Planum in January 2004, it quickly found what it had been sent from Earth to find: evidence of liquid water in the Martian past.
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When the Mars Exploration Rover, Opportunity, landed on Meridiani Planum in January 2004, it quickly found what it had been sent from Earth to find: evidence of liquid water in the Martian past.
Meridiani Planum
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
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.
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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
This unnamed channel drains part of Margaritifer Terra.
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This unnamed channel drains part of Margaritifer Terra.
Channel in Margaritifer Terra.
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...
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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
This color-coded map indicates the depth to icy layers at a site in southern Mars. The dense, icy layer retains heat better than the looser soil above it, so where the icy layer is closer to the su...
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Depth-to-Ice Map of a Southern Mars Site Near Melea Planum
Depth-to-Ice Map of a Southern Mars Site Near Melea Planum
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
The dunes and dust devil tracks in this VIS image are located on the plains of Planum Chronium.
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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
2906_HighViewOfMidCanyonMelas.jpg
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2906_HighViewOfMidCanyonMelas.jpg
High View of Melas
A new map of Mars' gravity made with three NASA spacecraft is the most detailed to date, providing a revealing glimpse into the hidden interior of the Red Planet. Satellites always orbit a planet's...
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Mars Gravity Map
Mars Gravity Map
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)
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 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
Seen shortly after local Martian sunrise, clouds gather in the summit pit, or caldera, of Pavonis Mons, a giant volcano on Mars, in this image from the Thermal Emission Imaging System (THEMIS) on N...
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Seen shortly after local Martian sunrise, clouds gather in the summit pit, or caldera, of Arsia Mons, a giant volcano on Mars, in this image from the Thermal Emission Imaging System (THEMIS) on NASA's Mars Odyssey orbiter.
Morning Clouds Atop Martian Mountain
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
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 image of a crater in Acidalia Planitia was acquired March 8, 2003, during northern summer.
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This image of a crater in Acidalia Planitia was acquired March 8, 2003, during northern summer.
Acidalia Planitia Crater
Artist's concept of future humans on Mars.
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Artist's concept of future humans on Mars.
Artist's concept of future humans on Mars.
NASA is advancing the Journey to Mars by starting the conversation about where humans may one day land on the Red Planet.
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This image shows the different exploration zones for Mars landing sites for human missions to the surface of Mars.
Mars Exploration Zone Layout Considerations
Five decades of successful NASA missions to the Red Planet, 1965-2015.
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50 Years of Mars Exploration
50 Years of Mars Exploration
A lunar eclipse, a solar eclipse and Mars has a close encounter with a comet.
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What's Up for October?
What's Up for October?

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