Characteristics exponents of the triangular solutions in the elliptical restricted three-body problem under radiating primaries

DOI10.1007/s12591-014-0230-xzbMath1380.70034OpenAlexW2043432718MaRDI QIDQ505012

Yong-Cai Geng, Sumit K. Garg

Publication date: 18 January 2017

Published in: Differential Equations and Dynamical Systems (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s12591-014-0230-x

zbMATH Keywords

stabilitydynamical systemcharacteristic exponentsradiation pressuretriangular pointselliptical restricted three-body problem (ER3BP)

Mathematics Subject Classification ID

Three-body problems (70F07) Celestial mechanics (70F15)

Related Items (1)

Characteristics exponents of the triangular solutions in the elliptical restricted three-body problem under radiating primaries

Cites Work

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• Characteristics exponents of the triangular solutions in the elliptical restricted three-body problem under radiating primaries
• Linear stability of the triangular equilibrium points in the photogravitational elliptic restricted problem. I
• Nonlinear stability of the triangular libration points for the photo gravitational elliptic restricted problem of three bodies
• The effect of solar radiation pressure on the Lagrangian points in the elliptic restricted three-body problem
• On the stability of triangular points in the elliptic R3BP under radiating and oblate primaries
• On the non-linear stability of motions around L5 in the elliptic restricted problem of the three bodies
• Stability of the triangular points in the elliptic restricted problem of three bodies.

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