Star and Planet Formation
Researchers
Star and Planet Formation
Area 5 has the task of studying the physics and chemistry that regulates star formation and the subsequent formation of planetary systems using multiple telescopes that allow us to see the coldest and densest places in the Universe. Its studies range from the interstellar medium and molecular clouds where stars are born in our galaxy and in nearby galaxies, to the formation and evolution of structures in protoplanetary discs where new planets form and grow.
Research Topics
Star formation
Understanding star formation plays a crucial role in understanding the evolution of galaxies and the subsequent formation of planets. Using advanced telescopes such as ALMA, we observe the birth of stars within molecular clouds and using optical telescopes we analyse the radiation emitted by young stars. Our focus is on the study of gas dynamics, radiative processes, magnetic fields and the chemistry of the interstellar medium to understand their influence on the star formation process. Through detailed observations and sophisticated physical models, we seek to unravel the complex mechanisms that govern the creation of stars, making a significant contribution to our knowledge of the universe.
Planetary formation
Studying planetary formation is essential for unravelling the mysteries of how our solar system and other systems that could harbour life formed. Through the use of powerful telescopes, such as ALMA, we observe protoplanetary discs, the cosmic nurseries where new planets are born and grow. We focus on studying the complex physical processes involved in protoplanet formation, from gravitational interactions to disc chemistry. Our main challenge is to understand how tiny particles of dust and gas clump together over relatively short periods of time to form planetary bodies. This work not only deepens our understanding of planetary formation but also seeks to resolve some of the deeper questions about the potential habitability of other planetary systems.
