Linear stability and resonance of triangular equilibrium points in elliptic restricted three body problem with radiating primary and triaxial secondary
-
2016-09-17 https://doi.org/10.14419/ijaa.v4i2.6536 -
Celestial Mechanics, Elliptical Restricted Three Body Problem, Stability, Oblateness, Rigid Body, Resonance. -
Abstract
The present paper studies the linear stability of the triangular equilibrium points of the system. The system comprises of a radiating primary and a triaxial secondary in elliptic restricted three body problem. The existence of third order resonances has been shown and the linear stability has been analyzed for these resonance cases. For the resonance case,  and  , the conditions of the linear stability are satisfied and the system is stable. But, for the resonance cases and  the system is unstable.
-
References
[1] Arnold, V. I.; Stability of equilibrium position of a Hamiltonian system of ordinary differential equations I general elliptic case; Doklady Akademii Nauk SSR; 137(2), 255, 1961.
[2] Ammar, M. K.; The effect of solar radiation pressure on the Lagrangian points in the elliptic restricted three-body problem; Astrophysics and Space Science; 313(4):393–408, 2008. http://dx.doi.org/10.1007/s10509-007-9709-z.
[3] Baoyin, Hexi. McInnes, Colin, R.; Solar sail equilibria in the elliptical restricted three-body problem. Journal of Guidance, Control, and Dynamics, 29(3):538–543, 2006. http://dx.doi.org/10.2514/1.15596.
[4] Bennet, A.; Characteristic exponents of the five equilibrium solutions in the elliptically restricted problem; ICARUS; 4(2), 177-187, 1965. http://dx.doi.org/10.1016/0019-1035(65)90060-6.
[5] C Beaug´e., S Ferraz-Mello., Michtchenko, T., A.,; Extrasolar planets in mean-motion resonance: apses alignment and asymmetric stationary solutions. The Astrophysical Journal, 593(2):1124, 2003. http://dx.doi.org/10.1086/376568.
[6] Broucke, R.; Stability of periodic orbits in the elliptic, restricted three-body problem; AIAA journal; 7(6):1003–1009, 1969. http://dx.doi.org/10.2514/3.5267.
[7] Biggs, James, D., Colin, R., McInnes., Thomas, Waters., ; Control of solar sail periodic orbits in the elliptic three-body problem. Journal of Guidance, Control, and Dynamics, 32(1):318–320, 2009a. http://dx.doi.org/10.2514/1.38362.
[8] Biggs, James, D., Colin, R., McInnes., Thomas, Waters., ; Solar sail formation flying for deep-space remote sensing; Journal of Guidance, Control, and Dynamics,; 46(3):670–678, 2009b.
[9] Chandra, Navin., Kumar, Ranjeet.,; Effect of oblateness on the non-linear stability of the triangular liberation points of the restricted three-bo dy problem in the presence of resonances. Astrophysics and Space Science, 291(1):1–19, 2004. http://dx.doi.org/10.1023/B:ASTR.0000029925.13391.7d.
[10] Choudhry, Manju., Choudhry, R , K. , ; On the stability of triangular libration points taking into account the light pressure for the circular restricted problem of three bodies. Celestial mechanics, 36(2):165–190, 1985. http://dx.doi.org/10.1007/BF01230650.
[11] Danby, J, M, A.; Stability of the triangular points in the elliptic restricted problem of three bodies; the Astronomical Journal, 69:165, 1964.
[12] S Ferraz-Mello. Averaging the elliptic asteroidal problem near a first-order resonance. The Astronomical Journal, 94:208–212, 1987. http://dx.doi.org/10.1086/114465.
[13] Hadjidemetriou, John, D., The elliptic restricted problem at the 3: 1 resonance. Celestial Mechanics and Dynamical Astronomy; 53(2):151–183, 1992. http://dx.doi.org/10.1007/BF00049463.
[14] Hadjidemetriou, John, D., Resonant motion in the restricted three body problem. In Qualitative and Quantitative Behaviour of Planetary Systems, pages 201–219. Springer, 1993. http://dx.doi.org/10.1007/978-94-011-2030-2_19.
[15] Henrard, Jacques, Caranicolas, N, D., A perturbative treatment of the 2:1 Jovian resonance; ICARUS; 69(2):266–279, 1987. http://dx.doi.org/10.1016/0019-1035(87)90105-9.
[16] Henrard, Jacques, Caranicolas, N, D., Motion near the 3/1 resonance of the planar elliptic restricted three body problem; Celestial Mechanics and Dynamical Astronomy; 47(2):99–121, 1989. http://dx.doi.org/10.1007/BF00051201.
[17] Henrard, Jacques; A semi-numerical perturbation method for separable Hamiltonian systems; Celestial Mechanics and Dynamical Astronomy, 49(1):43–67, 1990. http://dx.doi.org/10.1007/BF00048581.
[18] Kamel, A, A., Nayfeh, A, H.,; Stability of the triangular points in the elliptic restricted problem of three bo dies. AIAA Journal, 8(2):221–223, 1970. http://dx.doi.org/10.2514/3.5646.
[19] Katsiaris, G.; The three-dimensional elliptic problem; In Recent Advances in Dynamical Astronomy, pages 118–134; Springer; 1973. http://dx.doi.org/10.1007/978-94-010-2611-6_12.
[20] 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 Mechanics and Dynamical Astronomy, 46(1):59–77, 1989. http://dx.doi.org/10.1007/BF02426713.
[21] McCuskey, Sidney, Wilcox. ; Introduction to Celestial Mechanics; Reading; Mass.; Addison-Wesley Pub. Co. [1963], 1, 1963.
[22] Narayan, A., Shrivastava, Amit. , 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, 2014, 2014a.
[23] Narayan, A., Usha, T.; Stability of triangular equilibrium points in the elliptic restricted problem of three bodies with radiating and triaxial primaries. Astrophysics and Space Science, 351(1):135–142, 2014b. http://dx.doi.org/10.1007/s10509-014-1818-x.
[24] Subba Rao, P, V., Sharma, Ram Krishan.; Effect of oblateness on the non-linear stability of L4 in the restricted three-body problem. Celestial Mechanics and Dynamical Astronomy, 65(3):291–312,
[25] Szebehely, V., Theory of orbits: The restricted three body problem, 1967.
[26] Thakur, A, P. Singh, R, B.; Stability of the triangular libration points of the circular restricted problem in the presence of resonances. Celestial Mechanics and Dynamical Astronomy, 66(2):191–202, 1996. http://dx.doi.org/10.1007/BF00054964.
[27] Usha, T., Narayan, A., Ishwar, B.; Effects of radiation and triaxiality of primaries on triangular equilibrium points in elliptic restricted three body problem; Astrophysics and Space Science; 349(1):151–164, 2014 http://dx.doi.org/10.1007/s10509-013-1655-3.
-
Downloads
Additional Files
-
How to Cite
Usha, T., & Narayan, A. (2016). Linear stability and resonance of triangular equilibrium points in elliptic restricted three body problem with radiating primary and triaxial secondary. International Journal of Advanced Astronomy, 4(2), 82-89. https://doi.org/10.14419/ijaa.v4i2.6536Received date: 2016-07-28
Accepted date: 2016-08-24
Published date: 2016-09-17