Spin orbit resonance cascade via core shell model: application to Mercury and Ganymede
Dr. Matteo Veglianti
Forced Periodic Motion by Solar Radiation Pressure in the Polyhedral Gravity Model
Dr Anivid Pedros-Faura
Abstract
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Discussion
1. Spin orbit resonance cascade via core shell model: application to Mercury and Ganymede
Matteo Veglianti
University of Rome Tor Vergata
2. Forced Periodic Motion by Solar Radiation Pressure in the Polyhedral Gravity Model
Anivid Pedros-Faura
University of Colorado Boulder
Celestial Mechanics and Dynamical Astronomy Seminar Series
Celestial Mechanics and Dynamical AstronomyCite as
A. Pedros-Faura and M. Veglianti (2025, January 31), Spin orbit resonance cascade via core shell model: application to Mercury and Ganymede, Forced Periodic Motion by Solar Radiation Pressure in the Polyhedral Gravity Model
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Video length 1:17:45
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