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On the Stability of the Triangular Equilibrium Points in the Photogravitational R3BP with an Oblate Infinitesimal and Triaxial Primaries for the Binary Lalande 21258 System

In: Approximation and Computation in Science and Engineering

Author

Listed:
  • Jessica Mrumun Gyegwe

    (Federal University Lokoja)

  • Aguda Ekele Vincent

    (Nigeria Maritime University)

  • Angela E. Perdiou

    (University of Patras)

Abstract

In the framework of the planar circular restricted three-body problem (R3BP), we explore the effects of oblateness of the infinitesimal mass body as well as radiation pressure and triaxiality of the two primaries on the position and stability of the triangular equilibrium points (TEPs). It is found that all the involved parameters affect the positions and stability of these points. Specifically, it has been shown that TEPs are stable for 0

Suggested Citation

  • Jessica Mrumun Gyegwe & Aguda Ekele Vincent & Angela E. Perdiou, 2022. "On the Stability of the Triangular Equilibrium Points in the Photogravitational R3BP with an Oblate Infinitesimal and Triaxial Primaries for the Binary Lalande 21258 System," Springer Optimization and Its Applications, in: Nicholas J. Daras & Themistocles M. Rassias (ed.), Approximation and Computation in Science and Engineering, pages 397-415, Springer.
    • Handle: RePEc:spr:spochp:978-3-030-84122-5_21
    DOI: 10.1007/978-3-030-84122-5_21
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