Image Credit: NASA/JPL-Caltech/Space Science Institute/Kevin M. The imaging operations center is based at the Space Science Institute in Boulder, Colorado.įor more information about the Cassini-Huygens mission visit and. Images from NASA, JPL-Caltech, Space Science Institute and the University of Arizona. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. NASA’s Cassini spacecraft burned up in Saturn’s atmosphere in September 2017, after 20 years in space. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The view was made using images taken by Cassini’s wide-angle camera on July 20, 2016, using a combination of spectral filters sensitive to infrared light at 750, 727 and 619 nanometers.įilters like these, which are sensitive to absorption and scattering of sunlight by methane in Saturn’s atmosphere, have been useful throughout Cassini’s mission for determining the structure and depth of cloud features in the atmosphere. Gill, who also happens to be an engineer at NASA’s Jet Propulsion Laboratory. The view was made using images taken by Cassini's wide-angle camera on July 20, 2016, using a combination of spectral filters sensitive to infrared light at 750, 727 and 619 nanometers. The view was produced by space imaging enthusiast Kevin M. This false-color view from NASA's Cassini spacecraft shows clouds in Saturn's northern hemisphere. This false-color view from NASA’s Cassini spacecraft shows clouds in Saturn’s northern hemisphere. This image was taken as part of Webb Guaranteed Time Observation. However, the icy rings stay relatively bright, leading to the unusual appearance of Saturn in the Webb image. This false-color view from NASA's Cassini spacecraft shows clouds in Saturn's northern hemisphere. Saturn itself appears extremely dark at this infrared wavelength observed by the telescope, as methane gas absorbs almost all of the sunlight falling on the atmosphere.
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