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Hematite Outlier
PIA04840
Sol (our sun)
Thermal Emission Imaging Sys
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| Title |
Hematite Outlier |
| Original Caption Released with Image |
Released 30 October 2003 A stack of eroding sediments roughly 200 meters high contains the northeastern-most occurrence of the hematite layer that covers much of Meridiani Planum. The origin of the hematite layer is still a mystery, one that may be solved when the Mars Exploration Rover named Opportunity arrives in January. Image information: VIS instrument. Latitude 1.1, Longitude 0.5 East (359.5 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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Hematite Outlier
PIA04840
Sol (our sun)
Thermal Emission Imaging Sys
…
| Title |
Hematite Outlier |
| Original Caption Released with Image |
Released 30 October 2003 A stack of eroding sediments roughly 200 meters high contains the northeastern-most occurrence of the hematite layer that covers much of Meridiani Planum. The origin of the hematite layer is still a mystery, one that may be solved when the Mars Exploration Rover named Opportunity arrives in January. Image information: VIS instrument. Latitude 1.1, Longitude 0.5 East (359.5 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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Valley Floor
PIA04837
Sol (our sun)
Mars Orbiter Camera
| Title |
Valley Floor |
| Original Caption Released with Image |
MGS MOC Release No. MOC2-529, 30 October 2003 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows the floor of an ancient valley located near the Pyrrhae Chaos region of Mars. This valley might have been carved by liquid water, but today no evidence remains that a fluid ever flowed through it. Long after the valley formed, its floor was covered by large, windblown, ripple-like dunes. This picture is located near 13.0°S, 31.2°W. The image is illuminated by sunlight from the upper left and covers an area 3 km (1.9 mi) wide. |
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