Non- linear stability of triangular librations points in circular restricted three body under radiating and oblate primaries in presence of resonance
-
2015-06-23 https://doi.org/10.14419/ijaa.v3i2.4772 -
ER3BP, Hamiltonian Functions, Triangular Libration Points, Resonance. -
Abstract
The nonlinear stability of the triangular librations points is studied in the presence resonance considering both the primaries as radiating and oblate. The study is carried out for various values of radiation pressure and oblateness parameter in general and binary systems in particular. It is found that the normal forms of the Hamiltonian contains both the resonance cases; ω1= 2ω2 and ω1= 3ω2. The case ω1= ω2 corresponds to the boundary region of the stability for the system.It is investigated that for the motion is unstable for third order resonance but stable for fourth order resonance.
-
References
[1] Ammar MK (2008), the effect of solar radiation pressure on the Lagrangian points in the elliptical restricted three body problem, Astrophysics & Space Science, 313, 393-408.http://dx.doi.org/10.1007/s10509-007-9709-z.
[2] Arnold VI (1963a), Proof of A. N. Kolmogorov’s theorem on the preservation of quasiperiodic motions under small perturbations of the Hamiltonian, Russian Math. Surveys, 18, 5, 9–36.
[3] Arnold VI (1963b), Small divisor problems in classical and celestial mechanics, Russian Mathematical Surveys 18(6), 85–192. http://dx.doi.org/10.1070/RM1963v018n06ABEH001143.
[4] Bennet A (1965), Characteristics exponents of the five equilibrium solutions in the elliptically restricted problem, Icarus 4, 177-187. http://dx.doi.org/10.1016/0019-1035(65)90060-6.
[5] Bhatnagar KB, Gupta U &Bhadrawaj R (1994), Celestial Mechanics and Dynamical Astronomy, 59, 345-374. http://dx.doi.org/10.1007/BF00692102.
[6] Conxita P (1995), Ejection collision orbits with the more massive primary in the planar elliptic restricted three body problem, Celestial Mechanics and Dynamical Astronomy, 61, 315-331.http://dx.doi.org/10.1007/BF00049513.
[7] Danby, JMA (1964), Stability of the triangular points in the elliptic restricted problem of three bodies, Astronomical Journal, 69, 165-172. http://dx.doi.org/10.1086/109254.
[8] Erdi B (2009), A parametric study of stability and resonance around L4 in the elliptical restricted three body problem, Celestial Mechanics and Dynamical Astronomy, 104,145- 158.http://dx.doi.org/10.1007/s10569-009-9197-2.
[9] Grebenikov EA (1964), On the stability of the Lagrangian Triangular Solutions of the Restricted Elliptic Three Body problem, Soviet Astronomy, 8(3), 451-459.
[10] Gyorgyey J (1985), on the nonlinear stability of motions around the elliptical restricted problem of three bodies, Celestial Mechanics and Dynamical Astronomy, 36(3), 281-285.http://dx.doi.org/10.1007/BF01230741.
[11] Halan PP & Rana N (2001), The Existence and stability of equilibrium points in the Robe's restricted three body problem, Celestial Mechanics and Dynamical Astronomy, 79, 145-155. http://dx.doi.org/10.1023/A:1011173320720.
[12] Kumar S &Ishwar B (2011) Location of collinear equilibrium points in the generalized photogravitational elliptical restricted three body problem, Int. Journal of Sciience& Technology, 3(2), 157-162.
[13] Kumar V & Choudhary RK (1986), On the stability of the triangular libration points for the photogravitational circular restricted problem of three bodies when both of the attracting bodies are radiating as well, Celestial Mechanics, 40(2), 155-170.http://dx.doi.org/10.1007/BF01230257.
[14] Liapnuov AM (1956), the general problem of stability of Motion, Acad. Science USSR.
[15] Manju. & Choudhary RK (1985), On the stability of triangular libration points taking into account the light pressure for the circular restricted problem of three bodies, Celestial Mechanics, 36, 165
[16] Markeev AP (1978), Libration points in celestial Mechanics and Cosmodynamics, nauka, Moscow, Russia.
[17] Markellos VV, Perdios E &Labropoulou P (1992), Linear stability of the triangular equilibrium points in the phptogravitational elliptical restricted three body problem, Astrophysics & Space Science, 194, 207- 213. http://dx.doi.org/10.1007/BF00643991.
[18] Markellos VV (1996), Nonlinear stability zones around triangular equilibria in the plane circular restricted three-body problem , Astrophysics & Space Science, 245 157.http://dx.doi.org/10.1007/BF00637811.
[19] Narayan A., and Shrivastava.A., (2014), Existence of Resonance Stability of Triangular Equilibrium Points in Circular Case of the Planar Elliptical Restricted Three-Body Problem under the Oblate and Radiating Primaries around the Binary System, Advances in Astronomy; http://dx.doi.org/10.1155/2014/287174.
[20] Narayan, A &Singh.N (2014a), Motion and stability of triangular equilibrium points in elliptical restricted three body problem under the radiating primaries , Astrophysics & Space Science, 352 (1) , 57-70. http://dx.doi.org/10.1007/s10509-014-1903-1.
[21] Narayan, A., Singh.N. (2014c), Resonance stability of triangular equilibrium points in elliptical restricted three body problem under the radiating primaries, Astrophysics & Space Science, 353 (2) 441-455. http://dx.doi.org/10.1007/s10509-014-2085-6.
[22] Narayan, A & Singh N (2014b), Stability of triangular lagrangian points in elliptical restricted three body problem under the radiating binary systems, Astrophysics & Space Science, 353 (2) 457-464. http://dx.doi.org/10.1007/s10509-014-2014-8.
[23] Roberts G (2002), linear stability of the elliptic Lagrangian triangle solution in the three body problem, Differential equation, 182, 191-218. http://dx.doi.org/10.1006/jdeq.2001.4089.
[24] Sahoo SK &Ishwar B (2000), Stability of collinear equilibrium points in the generalized photo gravitational elliptic restricted three-body problem, Bulletin Astronomical Society India, 28, 579-586.
[25] Selaru D &Cucu-Dumitrescu C (1995), Infinitesimal orbit around Lagrange points in the elliptic restricted three body problem , Celestial Mechanics and Dynamical Astronomy, 61(4), 333- 346. http://dx.doi.org/10.1007/BF00049514.
[26] Singh J & Umar A (2012a), Motion in the photogravitational elliptic restricted three-body problem under an oblate primary, Astronomical Journal, 143, 109.http://dx.doi.org/10.1088/0004-6256/143/5/109.
[27] Singh J & Umar A, (2012b), on the stability of triangular equilibrium points in the elliptic R3BP under radiating and oblate primaries, Astrophysics & Space Science, 341, 349.http://dx.doi.org/10.1007/s10509-012-1109-3.
[28] Szebebely V (1967), Stability of the points of equilibrium in the restricted problem, Astronomical Journal, 72, 7-9.http://dx.doi.org/10.1086/110195.
[29] Usha T, Narayan A &Ishwar B (2014), Effects of Radiation and Triaxiality of primaries on triangular equilibrium points in elliptic restricted three body problem, Astrophysics & Space Science, 349, 151-164. http://dx.doi.org/10.1007/s10509-013-1655-3.
[30] Zimvoschikov AS &Thakai VN (2004), Instability of libration points and resonance phenomena in the photogravitational in the elliptical restricted three body problem, Solar System Research, 38 (2), 155-163.http://dx.doi.org/10.1023/B:SOLS.0000022826.31475.a7.
-
Downloads
-
How to Cite
Narayan, A., & Singh, N. (2015). Non- linear stability of triangular librations points in circular restricted three body under radiating and oblate primaries in presence of resonance. International Journal of Advanced Astronomy, 3(2), 58-68. https://doi.org/10.14419/ijaa.v3i2.4772Received date: 2015-05-14
Accepted date: 2015-06-08
Published date: 2015-06-23