Exoplanets in binary star systems: on the switch from prograde to retrograde orbits

DOI10.1007/S10569-015-9650-3zbMath1332.70012OpenAlexW2219711520WikidataQ114842688 ScholiaQ114842688MaRDI QIDQ259517

F. Blanchet-Sadri, M. Dambrine

Publication date: 11 March 2016

Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)

Full work available at URL: http://hdl.handle.net/11449/177723

zbMATH Keywords

three-body problemexoplanetsflip of inclinationLidov-Kozai mechanismorbital perturbation

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15) Orbital mechanics (70M20)

Related Items (2)

Analysis of the orbital evolution of exoplanets ⋮ Mutual potential between two rigid bodies with arbitrary shapes and mass distributions

Uses Software

• Mercury

Cites Work

• Unnamed Item
• Tidal evolution of hierarchical and inclined systems
• On the evection resonance and its connection to the stability of outer satellites
• Introduction to celestial mechanics
• The Three-Body Problem
• Explicit expansion of the three-body disturbing function for arbitrary eccentricities and inclinations
• The stellar three-body problem

This page was built for publication: Exoplanets in binary star systems: on the switch from prograde to retrograde orbits