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Cited by 332

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Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring

Spahn, Frank, Schmidt, Jürgen, Albers, Nicole, Hörning, Marcel, Makuch, Martin, Seiß, Martin, Kempf, Sascha, Srama, Ralf, Dikarev, Valeri, Helfert, Stefan, Moragas-Klostermeyer, Georg, Krivov, Alexander V., Sremčević, Miodrag, Tuzzolino, Anthony J., Economou, Thanasis, Grün, Eberhard·2006·Science

Abstract

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.

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Metadata

Authors
Spahn, F., Schmidt, J., Albers, N., Hörning, M., Makuch, M., Seiß, M., Kempf, S., Srama, R., Dikarev, V., Helfert, S., Moragas-Klostermeyer, G., Krivov, A. V., Sremčević, M., Tuzzolino, A. J., Economou, T., & Grün, E.
Venue
Science
Published
2006-03-10
Volume
311
Issue
5766
Pages
1416-1418
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2168197767
Cited by
332
References
0
FWCI
16.39
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring. https://app.cochat.ai/papers/10.1126/science.1121375
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Spahn, F., Schmidt, J., Albers, N., Hörning, M., Makuch, M., Seiß, M., Kempf, S., Srama, R., Dikarev, V., Helfert, S., Moragas-Klostermeyer, G., Krivov, A. V., Sremčević, M., Tuzzolino, A. J., Economou, T., & Grün, E. (2006). Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring. Science. https://doi.org/10.1126/science.1121375

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