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Science 10 March 2006:
Vol. 311. no. 5766, pp. 1406 - 1409
DOI: 10.1126/science.1120985

Reports

Identification of a Dynamic Atmosphere at Enceladus with the Cassini Magnetometer

M. K. Dougherty,1* K. K. Khurana,2 F. M. Neubauer,3 C. T. Russell,2 J. Saur,3 J. S. Leisner,2 M. E. Burton4

The Cassini magnetometer has detected the interaction of the magnetospheric plasma of Saturn with an atmospheric plume at the icy moon Enceladus. This unanticipated finding, made on a distant flyby, was subsequently confirmed during two follow-on flybys, one very close to Enceladus. The magnetometer data are consistent with local outgassing activity via a plume from the surface of the moon near its south pole, as confirmed by other Cassini instruments.

1 Blackett Laboratory, Imperial College London, London SW7 2AZ, UK.
2 Institute of Geophysics and Planetary Physics, University of California, Los Angeles, CA 90025, USA.
3 Institute for Geophysics and Meteorology, Köln University, 50923 Köln, Germany.
4 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

* To whom correspondence should be addressed. E-mail: m.dougherty{at}imperial.ac.uk

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