2018
DOI: 10.1007/s11214-018-0539-9
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Dust Emission by Active Moons

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Cited by 5 publications
(4 citation statements)
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“…Nanodust from Io's volcanoes or dust originating from the depths of Enceladus' oceans can escape the systems of Jupiter [742] and Saturn [743], [744]. Their compositions can be measured by in situ time-of-flight mass spectrometry [745].…”
Section: A Interplanetary Dust Cloudmentioning
confidence: 99%
“…Nanodust from Io's volcanoes or dust originating from the depths of Enceladus' oceans can escape the systems of Jupiter [742] and Saturn [743], [744]. Their compositions can be measured by in situ time-of-flight mass spectrometry [745].…”
Section: A Interplanetary Dust Cloudmentioning
confidence: 99%
“…Cosmic dust in the form of nanometer- to micrometer-sized ice grains originates from comets, plumes from icy satellites of the giant planets, or ejecta from hypervelocity impacts of micrometeoroids on the icy surfaces of atmosphereless bodies. The plume of Enceladus ejects material from the subsurface ocean so that it may be sampled and analyzed from spacecraft on a fly-by or in orbit around the moon . The Cosmic Dust Analyzer (CDA) instrument on the Cassini spacecraft sampled Enceladus plume grains during flythroughs at 7–17 km/s relative velocity and returned fascinating findings about the grains’ molecular composition, , including the presence of large organic macromolecules with masses of over 200 amu .…”
Section: Introductionmentioning
confidence: 99%
“…13). conclude that a salt-water reservoir is the source of a compositionally stratified plume on Enceladus (see also Hsu et al, 2015, Hillier et al, 2019. CDA also identified particles above the main rings (Hsu et al, 2018), dust from the Kuiper belt and interstellar dust grains (Altobelli et al 2016).…”
Section: Composition Measurements By Dust Analyzersmentioning
confidence: 99%
“…Among the significant discoveries by the Galileo and Ulysses dust instruments were: the detection of streams of nanometer sized dust particles from the volcanoes of Jupiter's moon Io , Horanyi et al, 1993, Zook et al, 1996, Graps et al, 2000, Krüger et al, 2006, Hillier et al, 2019, impactgenerated dust clouds surrounding the Galilean moons and the formation of a tenuous dust ring (Krüger et al, 2003, Krivov et al, 2002, and dust in and beyond Jupiter's gossamer rings (Krüger et al, 2009). By a Jupiter flyby, the Ulysses spacecraft was brought on to an orbit almost perpendicular to the ecliptic plane (Fig.…”
Section: Dust Detections By In Situ Detectors Throughout the Planetar...mentioning
confidence: 99%