Abstract
In the present paper we have found the range of values of µ ande for the linear stability of the triangular points for the doubly photogravitational elliptic restricted problem of three bodies. It has been shown that some resonances of the third and the fourth order exist which will need special investigation for the determination of complete stability of the libration points under our terms of reference.
Similar content being viewed by others
References
Bennet, A.: 1965,Icarus,4 (2).
Birkhoff, G. D.: 1927,Dynamical Systems, New York.
Duboshin, G. N.: 1964,Celestial Mechanics, Analytical and Qualitative Methods (Russian), Nauka, Moscow.
Kumar, V. and Choudhry, R. K.: 1987,Celest. Mech. 40 (2).
Kumar, V. and Choudhry, R. K.:Celest. Mech. (Accepted for publication, 1988.)
Lanzano, P.: 1967,Icarus,6 (1).
Lukyanov, L. G.: 1969,Bulletin of the Theoretical Institute of Astronomy (Russian),11, 10(133), p. 693.
Manju and Choudhry, R. K.: 1985,Celest. Mech.,36, 165–190.
Markeev, A. P.: 1970,PMM,34 (2), p. 227.
Markeev, A.P.: 1978,Libration Points in Celestial Mechanics and Astrodynamics (Russian), Nauka, Moscow.
Moser, J.: 1958, ‘New aspects in the theory of stability of Hamiltonian system’,Comm. Pure Appl. Math.,11 (1), pp. 81–114.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kumar, V., Choudhry, R.K. Linear stability and the resonance cases for the triangular libration points for the doubly photo-gravitational elliptic restricted problem of three bodies. Celestial Mech Dyn Astr 46, 59–77 (1989). https://doi.org/10.1007/BF02426713
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1007/BF02426713