Research Article

Motion of the Infinitesimal Variable Mass in the Generalized Circular Restricted Three-Body Problem under the Effect of Asteroids Belt

Table 1

All the equilibrium points depicted are unstable and determined for , , , , , , , and .

Equilibrium pointsRoots

0.400.74824671780.0000000000
1.6105
–1.4105
0.10515240500.0000000000
4.66466
–0.70991619910.0000000000
–1.08426
1.28426
–0.02743887810.000000000
  
  

0.90  
1.6105
  
  
  
  

1.40