Cassini Ion and Neutral Mass Spectrometer: Enceladus Plume Composition and Structure

The Cassini spacecraft passed within 168.2 kilometers of the surface above the southern hemisphere at 19:55:22 universal time coordinated on 14 July 2005 during its closest approach to Enceladus. Before and after this time, a substantial atmospheric plume and coma were observed, detectable in the Io...

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Published in:Science (American Association for the Advancement of Science) Vol. 311; no. 5766; pp. 1419 - 1422
Main Authors: Waite, J. Hunter, Combi, Michael R, Ip, Wing-Huen, Cravens, Thomas E, McNutt, Ralph L, Kasprzak, Wayne, Yelle, Roger, Luhmann, Janet, Niemann, Hasso, Gell, David, Magee, Brian, Fletcher, Greg, Lunine, Jonathan, Tseng, Wei-Ling
Format: Journal Article
Language:English
Published: United States American Association for the Advancement of Science 10-03-2006
The American Association for the Advancement of Science
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Summary:The Cassini spacecraft passed within 168.2 kilometers of the surface above the southern hemisphere at 19:55:22 universal time coordinated on 14 July 2005 during its closest approach to Enceladus. Before and after this time, a substantial atmospheric plume and coma were observed, detectable in the Ion and Neutral Mass Spectrometer (INMS) data set out to a distance of over 4000 kilometers from Enceladus. INMS data indicate that the atmospheric plume and coma are dominated by water, with significant amounts of carbon dioxide, an unidentified species with a mass-to-charge ratio of 28 daltons (either carbon monoxide or molecular nitrogen), and methane. Trace quantities (<1%) of acetylene and propane also appear to be present. Ammonia is present at a level that does not exceed 0.5%. The radial and angular distributions of the gas density near the closest approach, as well as other independent evidence, suggest a significant contribution to the plume from a source centered near the south polar cap, as distinct from a separately measured more uniform and possibly global source observed on the outbound leg of the flyby.
Bibliography:http://www.scienceonline.org/
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ISSN:0036-8075
1095-9203
DOI:10.1126/science.1121290