Tidal dynamics of extended bodies in planetary systems and multiple stars

TL;DR

This paper develops a comprehensive analytical framework for modeling tidal interactions between extended celestial bodies, improving accuracy over point-mass approximations and enabling detailed numerical simulations of planetary and stellar systems.

Contribution

It introduces a method using Cartesian STF tensors and Kaula's transform to derive tidal and mutual interaction potentials for extended bodies, advancing beyond traditional point-mass models.

Findings

Derived analytical expressions for tidal and mutual interaction potentials.

Formulated general dynamical evolution equations for extended body systems.

Provided a basis for accurate numerical simulations of tidal evolution.

Abstract

With the discovery during the past decade of a large number of extrasolar planets orbiting their parent stars at a distance lower than 0.1 astronomical unit (and the launch and the preparation of dedicated space missions such as CoRoT and KEPLER), with the position of inner natural satellites around giant planets in our Solar System and with the existence of very closed but separated binary stars, tidal interaction has to be carefully studied. In particular, a question arises about the validity of usual approximations used in the modelling of this interaction. The purpose of this paper is to examine the step beyond the ponctual approximation for the tidal perturber. To achieve this aim, the gravitational interaction between two extended bodies and more precisely the interaction between mass multipole moments of their gravitational fields and the associated tidal phenomena are studied. Use of Cartesian Symmetric Trace Free (STF) tensors, of their relation with spherical harmonics and of the Kaula's transform enables to derive analytically the tidal and mutual interaction potentials as well as the associated disturbing functions in extended bodies systems. The tidal and mutual interaction potentials of two extended bodies are derived. Next, the external gravitational potential of such tidally disturbed extended body is obtained, using the Love's number theory, as well as the associated disturbing function. Finally, the dynamical evolution equations for such systems are given in their more general form without any linearization. The dynamical equations for the gravitational and tidal interactions between extended bodies and associated dynamics are derived in a form where they could be directly implemented to perform coherent numerical simulations of planetary systems or multiple stars tidal evolution.