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Models of dust around Europa and Ganymede

Miljkovic, K.; Hillier, J. K.; Mason, N.J. and Zarnecki, J. C. (2012). Models of dust around Europa and Ganymede. Planetary and Space Science, 70(1) pp. 20–27.

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DOI (Digital Object Identifier) Link: http://dx.doi.org/10.1016/j.pss.2012.06.006
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Abstract

We use numerical models, supported by our laboratory data, to predict the dust densities of ejecta outflux at any altitude within the Hill spheres of Europa and Ganymede. The ejecta are created by micrometeoroid bombardment and five different dust populations are investigated as sources of dust around the moons. The impacting dust flux (influx) causes the ejection of a certain amount of surface material (outflux). The outflux populates the space around the moons, where a part of the ejecta escapes and the rest falls back to the surface. These models were validated against existing Galileo DDS (Dust Detector System) data collected during Europa and Ganymede flybys. Uncertainties of the input parameters and their effects on the model outcome are also included. The results of this model are important for future missions to Europa and Ganymede, such as JUICE (JUpiter ICy moon Explorer), recently selected as ESA’s next large space mission to be launched in 2022.

Item Type: Journal Article
Copyright Holders: 2012 Elsevier Ltd.
ISSN: 0032-0633
Keywords: dust; cloud; detection; Europa; Ganymede; Galileo; JUICE
Academic Unit/Department: Science > Physical Sciences
Interdisciplinary Research Centre: Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)
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Item ID: 33950
Depositing User: Astrid Peterkin
Date Deposited: 04 Jul 2012 12:49
Last Modified: 27 Nov 2014 17:19
URI: http://oro.open.ac.uk/id/eprint/33950
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