Equilibrium points of the restricted three-body problem with equal prolate and radiating primaries, and their stability

DOI10.1007/s10509-010-0584-7zbMath1230.85004OpenAlexW2035762360MaRDI QIDQ659965

Christos N. Douskos

Publication date: 24 January 2012

Published in: Astrophysics and Space Science (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10509-010-0584-7

zbMATH Keywords

stabilityequilibrium pointsrestricted problemprolate-radiating primaries

Mathematics Subject Classification ID

Three-body problems (70F07) Galactic and stellar dynamics (85A05)

Related Items (2)

Analytical and semianalytical treatment of the collinear points in the photogravitational relativistic RTBP ⋮ On the stability of \(L_{4,5} \) in the photogravitational relativistic R3BP

Cites Work

• Collinear equilibrium points of Hill's problem with radiation and oblateness and their fractal basins of attraction
• The stability of inner collinear equilibrium points in the photogravitational elliptic restricted problem
• A photogravitational Hill problem and radiation effects on Hill stability of orbits
• Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids
• Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid
• The restricted 3-body problem with radiation pressure
• BURRAU'S PROBLEM OF THREE BODIES
• A Hill problem with oblate primaries and effect of oblateness on Hill stability of orbits

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