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Layers Near South Crater
PIA05245
Sol (our sun)
Mars Orbiter Camera
| Title |
Layers Near South Crater |
| Original Caption Released with Image |
20 January 2004 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows layer outcrops near the rim of South Crater, in the south polar region of Mars. These ancient layered materials surround an even older knob--the rounded feature at right/center. This picture is located near 78.0°S, 336.0°W, and covers an area 3 km (1.9 mi) wide. Sunlight illuminates the scene from the upper left. |
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Dark Polar Dunes
PIA07282
Sol (our sun)
Mars Orbiter Camera
| Title |
Dark Polar Dunes |
| Original Caption Released with Image |
20 January 2004 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image, acquired during northern summer in December 2004, shows dark, windblown sand dunes in the north polar region of Mars. A vast sea of sand dunes nearly surrounds the north polar cap. These landforms are located near 80.3°N, 144.1°W. Light-toned features in the image are exposures of the substrate that underlies the dune field. The image covers an area about 3 km (1.9 mi) wide and is illuminated by sunlight from the lower left. |
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Meridiani Planum
PIA05356
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
Meridiani Planum |
| Original Caption Released with Image |
Released 20 January 2004 Long before the MER landers were named or launched, the two orbiters at Mars were asked to examine landing sites. Both the Odyssey and Mars Global Surveyor spacecraft have been collecting landing site data for the past two years. The MGS and ODY data were used as part of the decision making process in the final selection of the two landing sites. The types of data collected by the two orbiters included not only images of the surface but also thermal data about the surface composition, atmospheric data about the climate at each location, and the tracking of major dust storms in the region prior to landing. The presence of, and data collected by, the MGS and ODY orbiters have proven invaluable in MER mission planning. This image, captured on 13 April 2003, shows an area to the west of Opportunity's projected landing spot on Meridiani Planum. Image information: VIS instrument. Latitude -4.8, Longitude 355.8 East (4.2 West). 19 meter/pixel resolution. Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time. NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena. |
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Meridiani Planum
PIA05356
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
Meridiani Planum |
| Original Caption Released with Image |
Released 20 January 2004 Long before the MER landers were named or launched, the two orbiters at Mars were asked to examine landing sites. Both the Odyssey and Mars Global Surveyor spacecraft have been collecting landing site data for the past two years. The MGS and ODY data were used as part of the decision making process in the final selection of the two landing sites. The types of data collected by the two orbiters included not only images of the surface but also thermal data about the surface composition, atmospheric data about the climate at each location, and the tracking of major dust storms in the region prior to landing. The presence of, and data collected by, the MGS and ODY orbiters have proven invaluable in MER mission planning. This image, captured on 13 April 2003, shows an area to the west of Opportunity's projected landing spot on Meridiani Planum. Image information: VIS instrument. Latitude -4.8, Longitude 355.8 East (4.2 West). 19 meter/pixel resolution. Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time. NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena. |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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