Astrochemistry & Planet Formation

Laboratory activities

Our laboratory collaborates with observational team in order to understand the physical process ongoing in protoplanetary and planetary formation phase observed in the Universe. Infrared technique and ultra-high vacuum spectroscopy are combined to investigate in depth the formation of earth-like planets and complex biomelocules.

In laboratory through the preparation of analogue samples, we can simulate different physical processes and space environments, from interstellar grains to planetary surfaces. We can also study in controlled environment the interactions between prebiotic molecules, building blocks of life, and space relevant minerals in simultated space conditions such as UV irradiation and high vacuum regime. To understand what may occur at the molecules and grains in star forming regions and disks, we use techniques such as FTIR spectroscopy and Temperature Programmed Desorption analysis.