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Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure
J. Hunter Waite, Jr.,1Michael R. Combi,1Wing-Huen Ip,2Thomas E. Cravens,3Ralph L. McNutt, Jr.,4Wayne Kasprzak,5Roger Yelle,6Janet Luhmann,7Hasso Niemann,5David Gell,1Brian Magee,1Greg Fletcher,1Jonathan Lunine,6,8Wei-Ling Tseng2
The Cassini spacecraft passed within 168.2 kilometers of thesurface above the southern hemisphere at 19:55:22 universaltime coordinated on 14 July 2005 during its closest approachto Enceladus. Before and after this time, a substantial atmosphericplume and coma were observed, detectable in the Ion and NeutralMass Spectrometer (INMS) data set out to a distance of over4000 kilometers from Enceladus. INMS data indicate that theatmospheric plume and coma are dominated by water, with significantamounts of carbon dioxide, an unidentified species with a mass-to-chargeratio of 28 daltons (either carbon monoxide or molecular nitrogen),and methane. Trace quantities (<1%) of acetylene and propanealso appear to be present. Ammonia is present at a level thatdoes not exceed 0.5%. The radial and angular distributions ofthe gas density near the closest approach, as well as otherindependent evidence, suggest a significant contribution tothe plume from a source centered near the south polar cap, asdistinct from a separately measured more uniform and possiblyglobal source observed on the outbound leg of the flyby.
1 Department of Atmospheric, Oceanic, and Space Sciences, University of Michigan, Ann Arbor, MI 48109, USA. 2 Institutes of Astronomy and Space Science, National Central University, Chung Li 32054, Taiwan. 3 Department of Physics and Astronomy, University of Kansas, Lawrence, KS 66045, USA. 4 Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA. 5 NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA. 6 Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA. 7 Space Science Laboratory, University of California, Berkeley, CA 94720, USA. 8 Istituto di Fisica dello Spazio Interplanetario, Via del Fosso del Cavaliere 100, 00133 Rome, Italy.
From the Cover: Unified model of tectonics and heat transport in a frigid Enceladus.
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PNAS
104, 13578-13581
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The Variable Rotation Period of the Inner Region of Saturn's Plasma Disk.
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316, 442-445
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314, 1764-1766
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311, 1393-1401
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311, 1401-1405
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311, 1409-1412
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311, 1422-1425
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