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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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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
Sand-laden jets shoot into the polar sky in this view by noted space artist Ron Miller.
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Sand-laden jets shoot into the polar sky in this view by noted space artist Ron Miller.
Sand-Laden Jets
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 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 artist's animation shows how NASA's Curiosity rover will communicate with Earth via two of NASA's Mars orbiters, Mars Reconnaissance Orbiter and Odyssey. As the rover descends to the surface o...
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Communicating with Curiosity
Communicating with Curiosity
Artist’s concept of Comet Siding Spring approaching Mars, shown with NASA’s orbiters preparing to make science observations of this unique encounter.
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Artist's concept of Comet Siding Spring approaching Mars, shown with NASA's orbiters preparing to make science observations of this unique encounter.
NASA's Mars Orbiters Maneuvers as Comet Siding Spring Approaching Mars
This is a Mars Odyssey visible color image of an unnamed crater in western Arcadia Planitia (near 39 degrees N, 179 degrees E). The crater shows a number of interesting internal and external featur...
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This is a Mars Odyssey visible color image of an unnamed crater in western Arcadia Planitia (near 39 degrees N, 179 degrees E). The crater shows a number of interesting internal and external features that suggest that it has undergone substantial modification since it formed. These features include concentric layers and radial streaks of brighter, redder materials inside the crater, and a heavily degraded rim and ejecta blanket. The patterns inside the crater suggest that material has flowed or slumped towards the center. Other craters with features like this have been seen at both northern and southern mid latitudes The distribution of these kinds of craters suggests the possible influence of surface or subsurface ice in the formation of these enigmatic features. The image was taken on September 29, 2002 during late northern spring. This is an approximate true color image, generated from a long strip of visible red (654 nm), green (540 nm), and blue (425 nm) filter images that were calibrated using a combination of pre-flight measurements and Hubble images of Mars. The colors appear perhaps a bit darker than one might expect; this is most likely because the images were acquired in late afternoon (roughly 4:40 p.m. local solar time) and the low Sun angle results in an overall darker surface.
Western Arcadia Planitia
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
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 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
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
THEMIS Support for Landing Site Selection
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THEMIS Support for Landing Site Selection
THEMIS Support for Landing Site Selection
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
This mosaic of day and night infrared THEMIS images shows landslides flowed over 100 kilometers (62 miles) across the floor of Melas Chasma.
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This mosaic of day and night infrared THEMIS images shows landslides flowed over 100 kilometers (62 miles) across the floor of Melas Chasma.
mosaic of day and night infrared THEMIS
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
This image shows the context for orbital observations of exposed rocks that had been buried an estimated 5 kilometers (3 miles) deep on Mars.
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This image shows the context for orbital observations of exposed rocks that had been buried an estimated 5 kilometers (3 miles) deep on Mars.
Nature's Drilling Exposes Deeply Buried Minerals
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
Around 200 kilometers long, Ravi Vallis was born in a flood of water from Aromatum Chaos.
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Around 200 kilometers long, Ravi Vallis was born in a flood of water from Aromatum Chaos (left). The racing waters sliced a pathway across Xanthe Terra, spawned at least two small chaos regions in the channel (center), and then hurtled over the plateau edge to disappear into another chaos region (right foreground). In the distance at left lies Orson Welles Crater and the meandering path of Shalbatana Vallis, a much longer outflow channel perhaps related hydrologically to Ravi.
Ravi Vallis
This image from NASA's 2001 Mars Odyssey spacecraft shows part of the caldera floor of Arsia Mons. Arsia Mons is the southernmost of the Tharsis volcanoes. It is 270 miles in diameter, almost 12 mi...
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Investigating Mars: Arsia Mons
Investigating Mars: Arsia Mons
2021_WindingTributary.jpg
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2021_WindingTributary.jpg
Winding Side Canyon (Louros Valles)
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. The frame is about 14 kilometers (9 miles) wide.
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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. The frame is about 14 kilometers (9 miles) wide.
Bunge Crater Dunes
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
Part of a multispectral THEMIS infrared image of Nili Patera caldera on Syrtis Major has been superimposed on a high-resolution THEMIS visual image.
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Part of a multispectral THEMIS infrared image of Nili Patera caldera on Syrtis Major has been superimposed on a high-resolution THEMIS visual image.
Nili Patera and Dacite Lava Flow
Spider Web Pattern
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Spider Web Pattern
Spider Web Pattern
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

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