Image:Huygens landing01 L.jpg
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Huygens_landing01_L.jpg (13KB, MIME type: image/jpeg)
This raw image was returned by the Descent Imager/Spectral Radiometer camera onboard the European Space Agency's Huygens probe after the probe descended through the atmosphere of Titan. It shows the surface of Titan with ice blocks strewn around. The size and distance of the blocks will be determined when the image is properly processed.
The Descent Imager/Spectral Radiometer is one of two NASA instruments on the probe.
The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, California, manages the Cassini-Huygens mission for NASA's Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The Descent Imager/Spectral team is based at the University of Arizona, Tucson, Arizona.
For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov.
Credit: ESA/NASA/University of Arizona
| This image page contains items that originally came from a European Space Agency (ESA) website or publication. This image is not licensed under the GFDL. It is under a non-commercial-use only licence. See the ESA copyright policy [1], [2], [3] for more information. | |
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If this image was uploaded after May 19, 2005, it will soon be deleted without further warning.[4]
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Copyright info: http://www.esa.int/export/esaCP/SEMK95VZJND_index_0.html#O4
[edit] Sources
- http://www.esa.int/SPECIALS/Cassini-Huygens/index.html
- http://www.esa.int/images/landing01_L.jpg
- http://www.nasa.gov/images/content/105738main_Crop0-H1-300-215.jpg
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