About the Hill stability of extrasolar planets in stellar binary systems

DOI10.1007/s10569-008-9144-7zbMath1254.70033OpenAlexW2032103725MaRDI QIDQ1931793

Zoltán Makó, Ferenc Szenkovits

Publication date: 16 January 2013

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

Full work available at URL: https://doi.org/10.1007/s10569-008-9144-7

zbMATH Keywords

Hill stabilityelliptic restricted three-body problemextrasolar planetsplanets in stellar binary systems

Mathematics Subject Classification ID

Three-body problems (70F07) Stability for nonlinear problems in mechanics (70K20) Celestial mechanics (70F15)

Related Items

A parametric study of stability and resonances around \(L_4\) in the elliptic restricted three-body problem ⋮ Stable and unstable orbits around Mercury ⋮ Stabilization of Lagrange points in circular restricted three-body problem: a port-Hamiltonian approach ⋮ Connection between Hill stability and weak stability in the elliptic restricted three-body problem ⋮ Limits on the orbits of possible eccentric and inclined moons of extrasolar planets orbiting single stars

Cites Work

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• Hill stability of the planar three-body problem: General and restricted cases
• Capture in the circular and elliptic restricted three-body problem
• Hill stability and distance curves for the general three-body problem
• Stability criteria in many-body systems