Bergner performs laboratory rotational spectroscopy and astrochemical kinetics measurements to identify and characterize prebiotic molecules relevant to star- and planet-forming regions, complementing observational spectroscopy of protoplanetary disks. The lab is actively recruiting postdocs.
Rimmer's Planetary Astrochemistry Lab experimentally simulates planetary atmospheric, aqueous and surface chemistry to measure reaction rate constants relevant to prebiotic chemistry, using the custom-built StarLab UV photochemistry simulator to reproduce the light of young stars, in order to constrain which planets and moons are most likely to host the chemical pathways to life.