Abstract:Planetary systems in mean motion resonances hold a special place among the planetary population. They allow us to study planet formation in great detail as dissipative processes are thought to have played an important role in their existence. Additionally, planetary masses in bright resonant systems can be independently measured via both radial velocities and transit timing variations.
In principle, they also allow us to quickly determine the inclination of all planets in the system since, for the s… Show more
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