Planetary migration changes a planet's orbital semimajor axis through torques from a disc or exchanges of energy and angular momentum with other bodies, often followed by tidal dissipation. Short-period giant planets, eccentric progenitors, resonant architectures, and stellar obliquity provide complementary constraints rather than one unique migration diagnostic.
Planetary migration refers to the process by which planets change their orbits over time, moving closer to or further away from their parent star. This phenomenon is a key concept in the field of astrophysics and planetary science, particularly in the study of the formation and evolution of planetary systems.
New to topics? Read the docs here!