Orbital dynamics in the post-Newtonian planar circular restricted Sun–Jupiter system

DOI10.1142/S0218271818500360zbMath1430.70095arXiv1803.07437MaRDI QIDQ5203780

Euaggelos E. Zotos, F. L. Dubeibe

Publication date: 9 December 2019

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1803.07437

zbMATH Keywords

chaoscelestial mechanicsmethodsnumerical

Mathematics Subject Classification ID

Celestial mechanics (70F15) Galactic and stellar dynamics (85A05) Orbital mechanics (70M20)

Related Items (6)

Orbital dynamics in the photogravitational restricted four-body problem: Lagrange configuration ⋮ On Robe’s restricted problem with a modified Newtonian potential ⋮ Poynting-Robertson and oblateness effects on the equilibrium points of the perturbed R3BP: application on Cen X-4 binary system ⋮ Long-term evaluation of orbital dynamics in the Sun-planet system considering axial-tilt ⋮ Equilibrium Points and Basins of Convergence in the Triangular Restricted Four-Body Problem with a Radiating Body ⋮ Existence and stability of equilibrium points under the influence of Poynting-Robertson and Stokes drags in the restricted three-body problem

Uses Software

• Mathematica

Cites Work

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• Gravity
• ON MOULTON'S ORBITS IN THE RESTRICTED PROBLEM OF THREE BODIES

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