Heller, R.: Tidal heating in the early Earth-Moon system under a faint, young sun. General Meeting of the SPP 1833 “Building a Habitable Earth”, Göttingen (2018)
Heller, R.: Aufbruch zu den Sternen: Mit Breakthrough Starshot zu alpha Centauri und seinen Planeten. Öffentlicher Vortrag in der Reihe "Faszinierendes Weltall", Förderkreis Planetarium Göttingen e.V., Göttingen, Germany (2017)
Heller, R.; Winkler, M.: Extreme Viscoelastic Heating of Earth-like Planets in the Habitable Zones Around Low-Mass Stars. Annual Meeting of the Deutsche Astrobiologische Gesellschaft, Potsdam, Germany (2017)
Heller, R.: Die Suche nach Leben außerhalb der Erde. Public talk ("Astronomievortrag") at the Michael Adrian Observatory in Trebur, Trebur, Germany (2016)
Heller, R.: Extrasolar Planets, Astrobiology, and the PLATO Space Mission. Scientists in the Classroom, Nauset Regional High School in Cape Cod (MA), USA (2016)
Heller, R.; Barnes, R.: Benefits and Perils of Tidal Heating to Planetary Habitability. Annual Meeting of the German Astronomical Society, Splinter Session "Formation, Evolution and Astrobiology of Extrasolar Planets", Bochum, Germany (2016)
Heller, R.; Pudritz, R.; Barnes, R.: Large, Water-Rich Moons around Giant Exoplanets - Implications for Life Beyond Earth. Astrobiology, Life in the Context of Cosmic Evolution, Berlin-Adlershof, Germany (2016)
Heller, R.; Duda, J.-P.; Winkler, M.; Reitner, J.; Gizon, L.: Habitability of the Early Earth: A Faint Young Sun and Strong Tidal Heating due to a Closer Moon. ESRP Meeting, Jena, Germany (2022)
Heller, R.: Deceleration of High-Velocity Interstellar Photon Sails into Bound Orbits at α Centauri Using Photogravitational Assists. Astrobiology Science Conference, Mesa, Arizona, USA (2017)
Heller, R.: Astrophysical Simulations and Data Analyses on the Formation, Detection, and Habitability of Moons Around Extrasolar Planets. Habilitation, 433 pp., Georg-August-Universität Göttingen, Göttingen (2020)
Images from ESA’s Solar Orbiter offer the best look yet at a source region of the solar wind - and challenge our view of the continuous particle stream from the Sun.
Deciphering the magnetic origins of the Sun's hot corona: developing a framework for coronal heating by probing the elusive photosphere-corona connection
Using unique observational data and computer simulations, the MPS scientist is striving to understand the incredibly hot temperatures in the solar corona.
For the first time, images of the Sun have been taken from a distance of only 77 million kilometres enabling a completely new view of our star possible.
In his doctoral thesis, Sudip Mandal investigated how special pressure waves help maintain temperatures of several million degrees in the outermost solar atmosphere.