Orbital eccentricity significantly affects the positions of Lagrange points L4 and L5
the verdict
SUPPORTED
the evidence backs this
confidence 82/100
Orbital eccentricity affects the dynamics and positions of both triangular and collinear Lagrange points, altering the classical restricted three-body problem framework.
Evidence for · 4
Geometry of transit orbits in the periodically-perturbed restricted three-body problem
2022 · cited by 15
Paper [5] notes that time-periodic perturbations, such as the orbital eccentricity of the primaries, replace stationary Lagrange points with periodic orbits.
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More for · 3
Location and stability of the triangular Lagrange points in photo-gravitational elliptic restricted three body problem with the more massive primary as an oblate spheroid
2019 · cited by 6
Paper [6] explicitly studies the elliptic restricted three-body problem and concludes that parameters including eccentricity influence the location of the triangular Lagrangian points.
Location and Stability of the Triangular Points in the Triaxial Elliptic Restricted Three-Body Problem
2021 · cited by 4
Paper [9] demonstrates that the locations of triangular equilibrium points in the elliptic restricted three-body problem are affected by the eccentricity of the orbits.
Location of the collinear equilibrium points in the elliptic restricted three-body problem with various perturbation effects
2024 · cited by 3
Paper [11] shows that the positions of collinear Lagrange points shift and are dependent on eccentricity in the perturbed elliptic restricted three-body problem.