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Sremcevic, M.; Krivov, A. V.; Krüger, H.; Spahn, F.: Impact-generated dust clouds around planetary satellites: model versus Galileo data. Planetary and Space Science 53, pp. 625 - 641 (2005)
Willis, M.; Burchell, M. J.; Ahrens, T. J.; Krüger, H.; Grün, E.: Decreased values of cosmic dust number density estimates in the solar system. Icarus 176, pp. 440 - 452 (2005)
Altobelli, N.; Krüger, H.; Moissl, R.; Landgraf, M.; Grün, E.: Influence of wall impacts on the Ulysses dust detector in modelling the interstellar dust flux. Planetary and Space Science 52, pp. 1287 - 1295 (2004)
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The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.
The Planetary Plasma Environments group (PPE) has a strong heritage in the exploration of planetary magnetospheres and space plasma interactions throughout the solar system. It has contributed instruments to several past missions that flew-by or orbited Jupiter (Galileo, Cassini, Ulysses). The PPE participates in the JUICE mission by contributing hardware and scientific expertise to the Particle Environment Package (PEP).