Eggers, S.; Keller, H. U.; Markiewicz, W. J.: Dynamics of the Kuiper-belt during the formation of the solar system. In: Planetary Systems: the long view, S. 79 - 80 (Hg. Celniker, L. M.; Vân, J. T. T.). (1998)
Markiewicz, W. J.; Kossacki, K. J.; Keller, H. U.: Smale scale trench in the Martian soil: Conditions for condensation of atmospheric volatiles at the Mars Polar Lander site. In: First International Conference on Mars Polar Science and Exploration, S. 25 - 27 (Hg. Clifford, S.; Fisher, D.; Rice, J.). Lunar and Planetary Institute, Houston, TX (1998)
Blum, J.; Henning, T.; Cabane, M.; Fonda, M.; Giovane, F.; Gustafson, B. A. S.; Keller, H. U.; Markiewicz, W. J.; Levasseur-Regourd, A.-C.; Worms, J.-C.et al.; Nuth, J. A.; Rogers, F.: The concept of a facility for cosmic dust research on the international space station. In: Proc. ESA Symp. on Space Station Utilisation, Darmstadt, 1996, S. 303 - 308. ESA Publ. Div., Noordwjk (1996)
Markiewicz, W. J.; Keller, H. U.; Petrova, E.; Thomas, N.; Wuttke, M. W.: Water ice in the Martian atmosphere as derived from the PHOBOS/KRFM data. In: LPI Technical Report Number 96-01, Part 1, S. 32 - 33 (Hg. Jakowsky, B.; Treiman, A.). Lunar and Planetary Institute, Houston, Texas, USA (1996)
Markiewicz, W. J.; Völk, H. J.: Pre-planetary disks and planet formation. In: Formation and Evolution of Low Mass Stars, Proceedings of a NATO Advanced Study Institute, September 21 - October 2 1987, Viana do Castelo, Portugal, S. 181 (Hg. Dupree, A. K.; Lago, M. T. V. T.). Kluwer (1988)
Markiewicz, W.: Photometric Observations of Variability of Mars and Venus. Summer School Alpbach 2014, Space Missions for Geophysics of the Terrestrial Planets, Alpbach, Austria (2014)
Petrova, E. V.; Markiewicz, W. J.; Shalygina, O. S.: The latitude gradient of droplet sizes of the upper Venus clouds at 35-60S from the VMC/VEx observations. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Bertaux, J.-L.; Khatunstsev, I.; Hauchecorne, A.; Markiewicz, W.; Marcq, E.; Lebonnois, S.; Patsaeva, M.; Turin, A.: Geographic distribution of zonal wind and UV albedo at cloud top level from VMC camera on Venus Express: Influence of Venus topography through stationary gravity waves vertical propagation. European Geosciences Union General Assembly, Vienna, Austria (2015)
Bondarenko, N. V.; Basilevsky, A. T.; Shalygin, E. V.; Markiewicz, W. J.: Microwave Properties and the 1-Micron Emissivity of Crater-Related Radar-Dark Parabolas and Other Surface Features in Five Areas of Venus. 46th Lunar and Planetary Science Conference, The Woodlands, Texas, USA (2015)
Khatuntsev, I.; Limaye, S.; Ignatiev, N. I.; Markiewicz, W.; Patsaeva, M.; Turin, A.; Titov, D. V.: Upper cloud motions from the Venus Monitoring Camera imaging onboard Venus Express in period from 2006 to 2014. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Khatuntsev, I. V.; Patsaeva, M. V.; Ignatiev, N. I.; Titov, D. V.; Markiewicz, W. J.; Limaye, S. S.; Turin, A. V.: Variations of the zonal flow at Venus cloud tops from VMC/VEX UV images in period from 2006 to 2014. European Planetary Science Congress, Cascais, Portugal (2014)
Markiewicz, W. J.; Krauss, R. J.; Limaye, S. S.: Temporal variations observed in the clouds of Venus from Venus Monitoring Camera. European Planetary Science Congress 2014, Cascais, Portugal (2014)
Patsaeva, M.; Ignatiev, N. I.; Markiewicz, W. J.; Khatuntsev, I.; Titov, D. V.; Patsaev, D.: Mesoscale circulation at the upper cloud level at middle latitudes from the imaging by Venus Monitoring Camera onboard Venus Express. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Patsaeva, M.; Khatuntsev, I.; Patsaev, D.; Titov, D.; Ignatiev, N. I.; Markiewicz, W. J.; Rodin, A.: Correlation of the cloud top wind pattern with cloud morphology at the upper cloud level of Venus at 25S-75S from VMC/Venus Express. European Planetary Science Congress, Cascais, Portugal (2014)
Stenzel, O. J.; Hoekzema, N. M.; Markiewicz, W. J.: Mars' Atmospheric Optical Depth from Mars Express HRSC and Mars Exploration Rovers A Comparison. 45th Lunar and Planetary Science Conference, The Woodlands, Texas (2014)
Die ESA-Mission JUICE soll ab 2030 das Jupitersystem erkunden. Nach Vorbeiflügen an Europa und Callisto wird die Raumsonde erstmals in der Geschichte der Raumfahrt in eine Umlaufbahn um den Mond Ganymed einschwenken.
Das Submillimetre Wave Instrument (SWI) wird die Galileischen Monde, die Chemie, die Meteorologie und die Struktur der mittleren Jupiter-Atmosphäre, sowie atmosphärische und magnetosphärische Kopplungsprozesse untersuchen.
Mars Express ist eine ESA Mission zum Mars. Sie hat eine Nutzlast an Bord, die in der Lage ist, die bisher gründlichste Suche nach flüssigem Wasser, das unerlässlich ist für Leben wie wir es kennen, auf dem roten Planeten durchzuführen.
Ein Überblick über alle Arbeits- und Forschungsgruppen der Abteilung für Planetenwissenschaften: Atmosphären der Planeten, Inneres der Planeten, Kleine Körper und Kometen, Oberflächen der Planeten, Plasmaumgebung der Planeten.