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Dust spectrometry in the Jovian System

Abstract : The Galileo spacecraft characterised the dust environment in the jovian system. The discoveries included an extended dusty ring system, the nano-metre sized stream particles originating from the moon Io, and the dust exospheres around the Galilean satellites Ganymed, Europa and Callisto [2]. The study of the nanodust-magnetosphere interaction and the compositional analysis of dust particles ejected by the surfaces of Ganymed or Europa offer unique future opportunities. New dust instrumentation is a factor of 10 more sensitive then the former Galileo detector and adds compositional analysis for moon surface studies complementary to neutral gas or ion particle investigations. A dust spectrometer performs complementary measurements with respect to neutral gas or ion investigations and is highly sensitive for organic, salty water ice and mineral particles.
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Submitted on : Thursday, February 23, 2012 - 5:03:31 PM
Last modification on : Tuesday, September 22, 2020 - 3:24:02 PM

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R. Srama, S. Kempf, F. Postberg, Julien Schmidt, H. Krüger, et al.. Dust spectrometry in the Jovian System. EPSC-DPS Joint Meeting 2011, Oct 2011, Nantes, pp.1502. ⟨in2p3-00673512⟩

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