ISSN: 2375-3870
International Journal of Modern Physics and Application  
Manuscript Information
 
 
Effect of Perturbations on the Stability of Triangular Libration Points of the Robes Restricted Three-Body Problem when the Primaries are Oblate Spheroid
International Journal of Modern Physics and Application
Vol.1 , No. 3, Publication Date: Aug. 8, 2014, Page: 32-37
1375 Views Since August 8, 2014, 455 Downloads Since Apr. 14, 2015
 
 
Authors
 
[1]    

AbdulRazaq AbdulRaheem, Department of Mathematics and Statistics, Kwara State University, Malete, Nigeria.

[2]    

Faluyi Oludotun Omoniyi, Department of Physics and Material Science, Kwara State University, Malete, Nigeria.

 
Abstract
 

The effect of small changes in the Coriolis and centrifugal forces on the stability of equilibrium points in the Robe restricted three body problem was studied. In this problem we considered both primaries as oblate spheroid. The critical mass obtained depends on the small changes in the Coriolis and centrifugal forces, oblateness of the rigid shell and the second the second primary as well as the density parameter k. The stability of the triangular points depends largely on the values of k. The destabilizing tendencies of the centrifugal force and oblateness factors were enhanced when k>0 and weakened for k<0.


Keywords
 

Stability, Triangular Points, Robes Problem, Density Parameter, Perturbations


Reference
 
[01]    

V. V. Szebehely, Theory of Orbits (The Restricted Problem of Three-Body) Academic Press, New York (1967).

[02]    

K. B. Bhatnagar and P. P. Hallan, Celest. Mech. and Dyn. Astr.20 (1978): 95-103.

[03]    

M. Khanna and K. B. Bhatnagar, Indian Journal of Pure and Applied Mathematics, 30(7) (1999): 721-733.

[04]    

J. Singh and B. Ishwar, Bulletin of Astronomical Society of India, (27)(3)(1999): 415-424.

[05]    

R. K. Sharma, Z. A. Taqvi and K. B. Bhatnagar, Celest. Mech. and dyn. Astr. 79 (2001): 119-233.

[06]    

A. AbdulRaheem and J.Singh, Astronomical Journal, 131(2006), 1880-1885.

[07]    

H. A. G. Robe, Celestial Mechanics, 16(1997), 345-351.

[08]    

A. K. Shrivastava and D. Garain , Celest. Mech. and Dyn. Astr., 51(1991), 67-73.

[09]    

A. R. Plastino and A. Plastino , Celest. Mech. and Dyn. Astr., 61(1995), 197-206.

[10]    

C.M. Giordano, A.R.Plastino and A.Plastino, Celest. Mech. and Dyn. Astr., 66(1997), 229-242.

[11]    

P.P. Hallan and K.B.Mangang 2007. Planetary and Space Science, 55(2007), 512-516.

[12]    

P.P .Hallan and N. Rana, Indian J. of Pure and Appl. Math., 35(3) (2004), 401-413.

[13]    

S.W. McCuskey, Introduction to Celestial Mechanics, Addison-Wesley, New York(1963).

[14]    

S.A. Berger, Fluid Mechanics in Mechanical Engineering Handbook, Boca Raton: CRC Press LCC (1999).

[15]    

E.A.Abouelmagd, Earth, Moon and Planets, 110(3-4) (2013), 143-155.

[16]    

A. Narayan and C. R. Kumar, International Journal of Pure and Applied Mathematics, 68(2)(2011),201-224.

[17]    

R.K.Sharma and P.V.Subba Rao, Celest. Mech and Dyna. Astr.,13(1976),137-149.

[18]    

R.K.Sharma and P.V.Subba Rao, Astrophysics and Space Science,60(1979),347-250

[19]    

J.Singh and A.Umar, The stronomical Journal, 13,(2012), 109-131.

[20]    

O.P.Raman and R.Sharma, International Journal of Innovative Research in Science, Engineering and Technology, 2(10)(2013), 5682-5686.





 
  Join Us
 
  Join as Reviewer
 
  Join Editorial Board
 
share:
 
 
Submission
 
 
Membership