The orbital evolution of resonant chains of exoplanets incorporating circularisation produced by tidal interaction with the central star with application to the HD 158259 and EPIC 245950175 systems

DOI10.1007/S10569-021-10027-7zbMath1472.70051arXiv2105.03652OpenAlexW3170343159WikidataQ114092002 ScholiaQ114092002MaRDI QIDQ2049218

J. C. B. Papaloizou

Publication date: 24 August 2021

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

Full work available at URL: https://arxiv.org/abs/2105.03652

zbMATH Keywords

resonancesplanetary systemsplanet formationtidal interactions

Mathematics Subject Classification ID

Galactic and stellar structure (85A15) Orbital mechanics (70M20) Parametric resonances for nonlinear problems in mechanics (70K28)

Related Items (1)

The role of tidal forces in the long-term evolution of the Galilean system

Cites Work

• Consequences of tidal interaction between disks and orbiting protoplanets for the evolution of multi-planet systems with architecture resembling that of Kepler 444
• Tidal interactions in multi-planet systems
• The Orbital Resonance Amongst the Galilean Satellites of Jupiter
• Tidal torques on accretion discs in binary systems with extreme mass ratios
• Solar System Dynamics

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