Speaker
Ewa Szuszkiewicz
(University of Szczecin)
Description
Multi-planet systems are important for understanding how the planets form and evolve. The information about the planetary system evolutionary scenarios is encrypted in one of the robust observational features, namely mean-motion resonances. We present a new method in which the resonance structure can be used to characterise the planetary architectures during different phases of planetary system evolution and in the different stellar environments. This method has a potential to help in the interpretation of PLATO findings.
Primary author
Ewa Szuszkiewicz
(University of Szczecin)
