Eberhard Grün

TL;DR: In this paper, the authors focus on the dust environment between the orbits of the Galilean moons of Jupiter and show that grains larger than several tenths of a micrometer in radius are likely to stay in bound orbits around Jupiter for tens or hundreds of years until they either collide with the satellites or Jupiter or are ejected to interplanetary space.

TL;DR: In-situ measurements of cosmic dust provide information on the spatial and orbital distributions, and on the physical and chemical properties of dust in interplanetary space as mentioned in this paper, and the size distribution from a few micrometer to millimeter range was also characterized by analysis of lunar micro craters and later verified by near-Earth satellites like LDEF.

TL;DR: The composition of the impact plasma produced by fast dust particles (v > 1 km/sec) hitting an Au or W target was measured both with a model of the HELIOS micrometeoroid experiment (low electric field at the target) and a high field detector.

TL;DR: In this article, the authors report on the inferred properties of the ejected dust and the surface change at the site of the outburst on comet 67P, and suggest a pressurized sub-surface gas reservoir, or the crystallization of amorphous water ice as possible causes.

TL;DR: The possibility of removing particles from Io by interactions with the Jovian magnetosphere has been investigated in this paper, where it is found that dust grains of about 0.1 micron radius will rapidly become charged if exposed to the ambient Jovians plasma.