An optimum opportunity for interstellar dust measurements by the JUICE mission

The JUpiter ICy moons Explorer (JUICE) is an ESA L-class mission concept designed to explore the Galilean satellites of the Jovian system. Although the current mission science goals do not include any astrophysical observations, we find that the planned period of the JUICE mission is optimal for in...

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Bibliographic Details
Main Authors: Sterken, Veerle Jasmin (Author) , Postberg, Frank (Author) , Grün, Eberhard (Author)
Format: Article (Journal)
Language:English
Published: 8 July 2012
In: Planetary and space science
Year: 2012, Volume: 71, Issue: 1, Pages: 142-146
ISSN:1873-5088
DOI:10.1016/j.pss.2012.06.020
Online Access:Verlag, Volltext: http://dx.doi.org/10.1016/j.pss.2012.06.020
Verlag, Volltext: http://www.sciencedirect.com/science/article/pii/S0032063312001912
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Author Notes:V.J. Sterken, N. Altobelli, S. Kempf, H. Krüger, F. Postberg, R.H. Soja, R. Srama, E. Grün
Description
Summary:The JUpiter ICy moons Explorer (JUICE) is an ESA L-class mission concept designed to explore the Galilean satellites of the Jovian system. Although the current mission science goals do not include any astrophysical observations, we find that the planned period of the JUICE mission is optimal for in situ measurements of Interstellar Dust (ISD), due to highly increased flux levels at that time. In case that JUICE carries a dust detector, this could lead to in situ high-resolution mass spectra of ISD grains. Such compositional information on the ISD grains is important for understanding the origins of solar/planetary systems, and therefore could represent a valuable addition to the core JUICE mission science.
Item Description:Gesehen am 02.09.2020
Physical Description:Online Resource
ISSN:1873-5088
DOI:10.1016/j.pss.2012.06.020