%0 Journal Article %1 Spahn1416 %A Spahn, Frank %A Schmidt, Jürgen %A Albers, Nicole %A Hörning, Marcel %A Makuch, Martin %A Seiß, Martin %A Kempf, Sascha %A Srama, Ralf %A Dikarev, Valeri %A Helfert, Stefan %A Moragas-Klostermeyer, Georg %A Krivov, Alexander V. %A Sremcević, Miodrag %A Tuzzolino, Anthony J. %A Economou, Thanasis %A Grün, Eberhard %D 2006 %I American Association for the Advancement of Science %J Science %K ibbs_biomat myown %N 5766 %P 1416--1418 %R 10.1126/science.1121375 %T Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring %U http://science.sciencemag.org/content/311/5766/1416 %V 311 %X 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.

@article{Spahn1416, abstract = {During Cassini{\textquoteright}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{\textquoteright} 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{\textquoteright}s E ring.}, added-at = {2018-05-08T15:36:50.000+0200}, author = {Spahn, Frank and Schmidt, J{\"u}rgen and Albers, Nicole and H{\"o}rning, Marcel and Makuch, Martin and Sei{\ss}, Martin and Kempf, Sascha and Srama, Ralf and Dikarev, Valeri and Helfert, Stefan and Moragas-Klostermeyer, Georg and Krivov, Alexander V. and Srem{\v c}evi{\'c}, Miodrag and Tuzzolino, Anthony J. and Economou, Thanasis and Gr{\"u}n, Eberhard}, biburl = {https://puma.ub.uni-stuttgart.de/bibtex/227e85315f520849927c9bb5c71634456/marcelhoerning}, doi = {10.1126/science.1121375}, eprint = {http://science.sciencemag.org/content/311/5766/1416.full.pdf}, interhash = {397d805aa0f40165c684aede5b9ef000}, intrahash = {27e85315f520849927c9bb5c71634456}, issn = {0036-8075}, journal = {Science}, keywords = {ibbs_biomat myown}, number = 5766, pages = {1416--1418}, publisher = {American Association for the Advancement of Science}, timestamp = {2019-04-23T07:28:36.000+0200}, title = {Cassini Dust Measurements at Enceladus and Implications for the Origin of the E Ring}, url = {http://science.sciencemag.org/content/311/5766/1416}, volume = 311, year = 2006 }