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ReportsCassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring evi ,5
During Cassini's close flyby of Enceladus on 14 July 2005, the High Rate Detector of the Cosmic Dust Analyzer registered micron-sized dust particles enveloping this satellite. The dust impact rate peaked about 1 minute before the closest approach of the spacecraft to the moon. This asymmetric signature is consistent with a locally enhanced dust production in the south polar region of Enceladus. Other Cassini experiments revealed evidence for geophysical activities near Enceladus' south pole: a high surface temperature and a release of water gas. Production or release of dust particles related to these processes may provide the dominant source of Saturn's E ring.
1 Institut für Physik, Universität Potsdam, Am Neuen Palais 10, Haus 19, D-14469 Potsdam, Germany.
2 Max Planck Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany. 3 Astrophysikalisches Institut, Friedrich Schiller Universität, 07745 Jena, Germany. 4 Hawaii Institute of Geophysics and Planetology, University of Hawaii, Honolulu, HI 96822, USA. 5 Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, CO 80303, USA. 6 Laboratory for Astrophysics and Space Research, University of Chicago, Chicago, IL 60637, USA. * Corresponding author: jschmidt{at}agnld.uni-potsdam.de
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Science. ISSN 0036-8075 (print), 1095-9203 (online)