On the Lagrange stability of motion in the planar restricted three-body problem

2017 ◽  
Vol 59 (10) ◽  
pp. 2459-2465 ◽  
Author(s):  
S.P. Sosnitskii
Author(s):  
M. N. Ismail ◽  
A. H. Ibrahim ◽  
G. H. F. Mohamadin ◽  
W. A. Okasha

In this work, the canonical Hamiltonian form of the restricted three- body problem including the effects of primaries oblateness is presented. Moreover, the collinear libration points are obtained. In addition to this, the relation between position of libration points and variation in (mass ration , oblateness coefficients A1 and A2) is studied. The results obtained are a good agreement with Perdios [1] & Singh [2].  The Poincare surface section PSS is used to illustrate the stability of motion around each of the collinear libration points. A numerical application on the real system Earth-Moon is presented.


New Astronomy ◽  
2021 ◽  
Vol 84 ◽  
pp. 101510
Author(s):  
Md Sanam Suraj ◽  
Rajiv Aggarwal ◽  
Md Chand Asique ◽  
Amit Mittal

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