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Dust grain orbital behavior around ceres

✍ Scribed by R. Nazzario; T.W. Hyde; L. Barge


Book ID
108426782
Publisher
Elsevier Science
Year
2003
Tongue
English
Weight
715 KB
Volume
31
Category
Article
ISSN
0273-1177

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We analyze the data of the Galileo dust detector system (DDS) with respect to micrometer-sized dust grains in the inner jovian system. The analysis of these data requires an in-depth modeling because an exact determination of the orbits of individual particles directly from the data is not possible.