Non-collinear libration points in CR3BP when less massive primary is an heterogeneous oblate body with N-layers

 
 
 
  • Abstract
  • Keywords
  • References
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  • Abstract


    In the present paper, the existence of non-collinear libration points has been shown in circular restricted three-body problem when less massive primary is a heterogeneous oblate body with N-layers. Further, the stability of non-collinear libration points is investigated in linear sense and found that the non-collinear libration points are stable for the critical value of mass parameter µµcrit= µo – 3.32792 k1 – 1.16808 k2.


  • Keywords


    Celestial Mechanics; Restricted Three-Body Problem; Libration Points; Stability; Heterogeneous Oblate Spheroid.

  • References


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Article ID: 5928
 
DOI: 10.14419/ijaa.v4i1.5928




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