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Tides in Planetary Systems

  • Stéphane MathisEmail author
  • Christophe Le Poncin-Lafitte
  • Françoise Remus
Part of the Lecture Notes in Physics book series (LNP, volume 861)

Abstract

The Solar system is the seat of many interactions between the Sun, the planets and their natural satellites. Moreover, since 1995, a large number of extrasolar planetary systems has been discovered where planets orbit around other stars, sometimes very close to them. Therefore, in such systems, tidal interactions are one of the key mechanisms that must be studied to understand the celestial bodies’ dynamics and evolution. Indeed, tides generate displacements and flows in planetary (and in the host star) interiors. The associated kinetic energy is then dissipated into heat because of internal friction processes. This leads to secular evolution of orbits and of spins with characteristic time-scales that are intrinsically related to the properties of dissipative mechanisms, those latters depending both on the internal structure of the studied bodies and on the tidal frequency. This lecture is aimed to review the must advanced theories to study tidal dynamics in planetary systems and the different tidal flows or displacements that can be excited by a perturber, the conversion of their kinetic energy into heat, the related exchanges of angular momentum, and the consequences for systems evolution.

Keywords

Giant Planet Multipole Moment Natural Satellite Love Number Extrasolar Planet 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

Acknowledgements

We thank the CNRS/INSU for the support given to this Thematic School. This work was supported in part by the Programme National de Planétologie (CNRS/INSU), the Programme National de Physique Stellaire (CNRS/INSU), the EMERGENCE-UPMC project EME0911, and the CNRS Physique théorique et ses interfaces program.

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Authors and Affiliations

  • Stéphane Mathis
    • 1
    • 2
    Email author
  • Christophe Le Poncin-Lafitte
    • 3
  • Françoise Remus
    • 1
    • 4
    • 5
  1. 1.Laboratoire AIM Paris-Saclay, CEA/DSM-CNRS-Université Paris DiderotCEAGif-sur-YvetteFrance
  2. 2.LESIA, Observatoire de Paris-CNRS-Université Paris Diderot-Université Pierre et Marie CurieObservatoire de ParisMeudonFrance
  3. 3.Syrte, Observatoire de Paris, CNRS UMR8630, Université Pierre et Marie CurieObservatoire de ParisParisFrance
  4. 4.LUTH, Observatoire de Paris-CNRS-Université Paris DiderotObservatoire de ParisMeudon CedexFrance
  5. 5.IMCCE, Observatoire de Paris-UMR 8028 du CNRS-Université Pierre et Marie CurieObservatoire de ParisParisFrance

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