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Old Arabian Crater
PIA04549
Sol (our sun)
Mars Orbiter Camera
| Title |
Old Arabian Crater |
| Original Caption Released with Image |
MGS MOC Release No. MOC2-376, 30 May 2003 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows an old meteor impact crater that was once buried and was then partially-exhumed from within the layered rocks on the floor of a much larger crater in eastern Arabia Terra. The erosion processes that began to exhume the crater, however, stopped some time ago, because today the entire area is covered by a blanket of dust. Avalanches of this dust have created dark streaks on the walls of the partly exhumed crater. This April 2003 image covers an area 3 km (1.9 mi) wide and is located near 20.9°N, 320.8°W. Sunlight illuminates the scene from the lower left. |
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Lava Flows
PIA04553
Sol (our sun)
Thermal Emission Imaging Sys
| Title |
Lava Flows |
| Original Caption Released with Image |
Released 30 May 2003 Lava flows and channels are visible here on the eastern flanks of Ascraeus Mons. One of the channels is bordered by levees, which form as lava overflows the channel banks, cools and solidifies. The other prominent channel to the north lacks levees, suggesting it may be a collapsed lava tube, or may have an aqueous origin. Image information: VIS instrument. Latitude 13.9, Longitude 262.2 East (97.8 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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Lava Flows
PIA04553
Sol (our sun)
Thermal Emission Imaging Sys
| Title |
Lava Flows |
| Original Caption Released with Image |
Released 30 May 2003 Lava flows and channels are visible here on the eastern flanks of Ascraeus Mons. One of the channels is bordered by levees, which form as lava overflows the channel banks, cools and solidifies. The other prominent channel to the north lacks levees, suggesting it may be a collapsed lava tube, or may have an aqueous origin. Image information: VIS instrument. Latitude 13.9, Longitude 262.2 East (97.8 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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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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| General Description |
International Space Station Imagery |
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