Khatuntsev, I. V.; Patsaeva, M. V.; Titov, D. V.; Ignatieva, N. I.; Turina, A. V.; Limaye, S. S.; Markiewicz, W. J.; Almeida, M.; Roatsch, T.; Moissl, R.: Cloud level winds from the Venus Express Monitoring Camera imaging. Icarus 226, pp. 140 - 158 (2013)
Krüger, H.; Bindschadler, D.; Dermott, S. F.; Graps, A. L.; Grün, E.; Gustafson, B. A.; Hamilton, D. P.; Hanner, M. S.; Horány, M.; Kissel, J.et al.; Linkert, D.; Linkert, G.; Mann, I.; McDonnell, J. A. M.; Moissl, R.; Morfill, G. E.; Polanskey, C.; Roy, M.; G., S.; Srama, R.: Galileo dust data from the jovian system: 2000 to 2003. Planetary and Space Science 58, pp. 965 - 993 (2010)
Moissl, R.: Morphology and dynamics of the Venus atmosphere at the cloud top level as observed by the Venus Monitoring Camera. Dissertation, Technische Universität Braunschweig (2008)
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.