Galileo In-Situ Dust Measurements in Jupiter's Gossamer Rings
Harald Krueger, Douglas P. Hamilton, Richard Moissl, Eberhard Gruen

TL;DR
The Galileo spacecraft's in-situ dust measurements in Jupiter's gossamer rings revealed a detailed size distribution of tiny particles, extending previous optical findings and showing variations in particle flux and orbital inclinations.
Contribution
First in-situ measurements of dust in Jupiter's gossamer rings, extending size distribution data to smaller particles and comparing results with optical imaging.
Findings
Size distribution increases towards smaller particles.
Detected particles on highly-tilted orbits up to 20 degrees.
Large particles (~5 micron) dominate optical cross-section.
Abstract
During its late orbital mission at Jupiter the Galileo spacecraft made two passages through the giant planet's gossamer ring system. The impact-ionization dust detector on board successfully recorded dust impacts during both ring passages and provided the first in-situ measurements from a dusty planetary ring. In all, a few thousand dust impacts were counted with the instrument accumulators during both ring passages, but only a total of 110 complete data sets of dust impacts were transmitted to Earth. Detected particle sizes range from about 0.2 to 5 micron, extending the known size distribution by an order of magnitude towards smaller particles than previously derived from optical imaging (Showalter et al. 2008). The grain size distribution increases towards smaller particles and shows an excess of these tiny motes in the Amalthea gossamer ring compared to the Thebe ring. The size…
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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Space Exploration and Technology
