On the extension of the Laplace-Lagrange secular theory to order two in the masses for extrasolar systems

DOI10.1007/s10569-013-9501-zzbMath1293.70057arXiv1306.5624OpenAlexW2068340802MaRDI QIDQ399966

Anne-Sophie Libert, Marco Sansottera

Publication date: 20 August 2014

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

Full work available at URL: https://arxiv.org/abs/1306.5624

zbMATH Keywords

secular dynamicsextrasolar systemsn-body problemnormal forms methodproximity to mean-motion resonancesupsilon andromedae

Mathematics Subject Classification ID

Perturbations of finite-dimensional Hamiltonian systems, normal forms, small divisors, KAM theory, Arnol'd diffusion (37J40) Celestial mechanics (70F15) Dynamical systems in classical and celestial mechanics (37N05) Perturbation theories for problems in Hamiltonian and Lagrangian mechanics (70H09)

Related Items (9)

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