An overview of important topics in modern astronomy: planets, sun, stars, milky way, galaxies, and cosmology

Astrophysics III is a course in Galactic Astrophysics. It introduces the concepts of stellar populations, stellar dynamics, interstellar medium (ISM), and star formation for understanding the physics and phenomenology of the different components of the Milky Way galaxy.

While thousands of extrasolar planets are known to orbit stars other than the Sun, Earth is - until now - the only planet known to be habitable. This lecture takes an interdisciplinary view on Earth as a habitable planet, how it formed, evolved, allowed life to flourish, and how its future might look like. Would we be able to identify another Earth-like planet amongst the population of exoplanets?

The course introduces in detail some of the main observational methods for the detection and characterization of extra-solar planetary systems. It covers the physics of planets (in the solar system and in extra-solar systems) and provides some overview of the current state of this dynamic research field.

Lecture Series about selected topics of space research and exploration consisting of individual talks given by different leading experts from academia and industry.

Introduction to the concepts and tools in physics with the help of demonstration experiments: mechanics of point-like and ridged bodies, periodic motion and mechanical waves.

Introduction to the concepts and tools in physics with the help of demonstration experiments: electromagnetism, optics, introduction to modern physics.

The physics of solar flares, coronal mass ejections and the solar wind will be described. A discussion of the similarities and differences to stellar flares and coronal mass ejections will follow. An introduction to the detection and characterization of extrasolar planets, the impact of stellar phenomena on exoplanets and in particular on their potential habitability will be given.