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2001 Mars Odyssey
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This region of Terra Sabaea contains areas with high densities of small craters.
Lot of Craters in Terra Sabaea
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2001 Mars Odyssey Turns 5
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"Flight Through Mariner Valley" Video Still
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Mars Canyon View
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Landslide Run-Out
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High View of Melas
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Winding Side Canyon (Louros Valles)
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Mars Canyon with Los Angeles for Scale
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'Live' Images from Mars at Camera Web Site
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Olivine-Rich Bedrock Around Nili Fossae
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This false color image shows a region with craters of different ages located at the margin of Acidalia Planitia. This image was collected during the Northern Spring season. The THEMIS VIS camera is capable of capturing color images of the Martian surface using five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from using multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation.
Cratered Acidalia Planitia
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This image of a crater in Acidalia Planitia was acquired March 8, 2003, during northern summer.
Acidalia Planitia Crater
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Mars south polar layered deposits - December 8, 2003
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Mars south polar layered deposits - December 8, 2003
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Mars south polar layered deposits - December 8, 2003
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Radiation environment at Mars and Earth - December 8, 2003
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Water mass map from neutron spectrometer - December 8, 2003
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North polar water ice by weight - December 8, 2003
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This image is located near the boundary between Syrtis Major and Isidis Planitia. The top of the image shows rough material that has eroded away from the lower portion of the image, revealing an underlying surface that has many small craters. It also reveals an ancient flow lobe that is barely discernable, crossing the southern part of the image (this flow lobe is much easier to see as a smooth region in the context image).
Erosion and what it Reveals
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NASA's Mars Odyssey spacecraft passes above Mars' south pole in this artist's concept illustration. The spacecraft has been orbiting Mars since October 24, 2001.
Odyssey over Mars' South Pole
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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
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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
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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
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Planum Boreum crater
Planum Boreum crater
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Hills abound in this portion of Mars located in the Vastitas Borealis region of the high northern plains. These hills are part of Scandia Colles. Note that some of the hills have aprons surrounding them. The northern part of Milankovic crater is visible in the lower portion of this image.
Bumpy Terrain in Vastitas Borealis
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