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Observations of Saturn in the 5- to 8-μm spectral region
Authors:FC Witteborn  JB Pollack  JD Bregman  JH Goebel  BT Soifer  RC Puetter  RJ Rudy  SP Willner
Institution:Ames Research Center, NASA, Moffett Field, California 94035, USA;California Institute of Technology, Pasadena, California 91109, USA;University of California, San Diego, La Jolla, California 92037, USA
Abstract:A spectrum of Saturn obtained from the Kuiper Airborne Observatory exhibits an emission peak at 6.8 μm attributed to ethane, but is otherwise dominated by absorption from 5.3 to 7.2 μm. While the large absorption in this spectral region is consistent with the presence of ammonia gas or ammonia ice, or both, such an explanation is inconsistent with the lack of a major absorption near 3.0 μm.
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