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Composition of Saturnian Stream Particles

Kempf, Sascha; Srama, Ralf; Postberg, Frank; Burton, Marcia; Green, Simon F.; Helfert, Stefan; Hillier, Jon K.; McBride, Neil; McDonnell, J. Anthony M.; Moragas-Klostermeyer, Georg; Roy, Mou and Grun, Eberhard (2005). Composition of Saturnian Stream Particles. Science, 307(5713) pp. 1274–1276.

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During Cassini's approach to Saturn, the Cosmic Dust Analyser (CDA) discovered streams of tiny (less than 20 nanometers) high-velocity (100 kilometers per second) dust particles escaping from the saturnian system. A fraction of these impactors originated from the outskirts of Saturn's dense A ring. The CDA time-of-flight mass spectrometer recorded 584 mass spectra from the stream particles. The particles consist predominantly of oxygen, silicon, and iron, with some evidence of water ice, ammonium, and perhaps carbon. The stream particles primarily consist of silicate materials, and this implies that the particles are impurities from the icy ring material rather than the ice particles themselves.

Item Type: Journal Item
ISSN: 1095-9203
Extra Information: Some of the symbols may not have transferred correctly into this bibliographic record and/or abstract.
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
Item ID: 5696
Depositing User: Users 6872 not found.
Date Deposited: 30 Oct 2006
Last Modified: 01 May 2019 13:23
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