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A Double Zone Dynamical Model For The Tidal Evolution Of The Obliquity
2017
Zenodo
It is debated whether close-in giants planets can form in-situ and if not, which mechanisms are responsible for their migration. One of the observable tests for migration theories is the current value of the orbital obliquity, i.e. the angle between the stellar equatorial plane and the orbital plane. But after the main migration mechanism has ended, the combined effects of tidal dissipation and the magnetic braking of the star lead to the evolution of both the obliquity and the semi-major axis.
doi:10.5281/zenodo.1066494
fatcat:r2qvqspkynhj7md6pjcb46cbcy