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

  • Authors

    • A. Arantza Jency Department of Aerospace EngineeringKarunya UniversityCoimbatore-641114Tamilnadu, India
    • Ram Krishan Sharma
    2019-11-05
    https://doi.org/10.14419/ijaa.v7i2.29814
  • Mean Motion, Planar ERTBP, Oblateness, Radiation Pressure, Critical Mass Ratio, Triangular Lagrangian Points, Transition Curves.

  • Abstract

    The triangular Lagrangian points of the elliptic restricted three-body problem (ERTBP) with oblate and radiating more massive primary are studied. The mean motion equation used here is different from the ones employed in many studies on the perturbed ERTBP. The effect of oblateness on the mean motion equation varies. This change influences the location and stability of the triangular Lagrangian points. The points tend to shift in the y-direction. The influence of the oblateness on the critical mass ratio is also altered. But the eccentricity limit  for stability remains the same.

     

     

     

    Author Biography

    • A. Arantza Jency, Department of Aerospace EngineeringKarunya UniversityCoimbatore-641114Tamilnadu, India
      Professor

  • References

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  • How to Cite

    Arantza Jency, A., & Krishan Sharma, R. (2019). 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. International Journal of Advanced Astronomy, 7(2), 57-62. https://doi.org/10.14419/ijaa.v7i2.29814

    Received date: 2019-09-04

    Accepted date: 2019-10-24

    Published date: 2019-11-05