Upcoming Seminars

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Recent Seminars

23 Feb 2016 - 14:00
Olli Sipilä
Max Planck Institute for Extraterrestrial Physics, Garching, Germany
In the physical conditions attributed to the central areas of starless and prestellar cores - the precursors of low-...
16 Feb 2016 - 14:00
Eva Wirström
Onsala Space Observatory, Sweden
Cold, dark and quiescent molecular clouds may at a first glance seem like straightforward and, perhaps, uninteresting...
09 Feb 2016 - 14:00
Ryuki Hyodo
Institut de Physique du Globe de Paris, France & Kobe University, Japan
Saturn's F ring and Uranus’s epsilon ring are narrow rings, located just outside planet’s Roche limit. Interestingly,...
02 Feb 2016 - 14:00
Evelyn Füri
Centre de Recherches Pétrographiques et Géochimiques, CNRS, Nancy, France
"The Moon was dry, and then it wasn’t. Now we just aren’t sure how wet it is, or where the volatiles came from, or when...
02 Dec 2015 - 14:00
Susanne Pfalzner
Max Planck Institute for Radio Astronomy, Bonn, Germany
Most stars do not form in isolation but as part of a group of stars referred to as star cluster. These young star...
25 Nov 2015 - 14:00
Kathrin Altwegg
Center for Space and Habitability, University of Bern, Switzerland
Rosetta has been at comet Churyumov-Gerasimenko almost 1½ years by now and the ten instruments on board the European...
16 Nov 2015 - 11:00
René Plume
University of Calgary, Canada
Modern astronomy involves more than most people realize. While the use of physics to understand the origins of galaxies...
11 Nov 2015 - 14:00
Kjartan Kinch
Niels Bohr Institute, University of Copenhagen
NASA’s 2020 Mars Rover mission is a large rover similar to the currently active “Curiosity” rover. The mission is fully...
11 Nov 2015 - 10:30
Magnus Schneide
Hamburger Sternwarte, Univ. Hamburg, Germany
The Solar Hidden Photon Search experiment (SHIPS) just finished in summer 2015. SHIPS was designed to detect solar...
03 Nov 2015 - 14:00
John Tobin
Leiden Observatory, The Netherlands
Disks and multiple star systems are thought to form early in the star formation process. Conservation of angular...

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