Author(s)

Preeti Jain¹, Rajiv Aggarwal², Amit Mittal¹,   Abdullah³

¹Department of Mathematics, A.R.S.D. College, University of Delhi, New Delhi, India.
²Department of Mathematics, Sri Aurobindo College, University of Delhi, New Delhi, India.
³Department of Mathematics, College of Science in Zulfi, Majmaah University, Riyadh, KSA.

We have studied periodic orbits generated by Lagrangian solutions of the restricted three-body problem when both the primaries are triaxial rigid bodies and source of radiation pressure. We have determined periodic orbits for different values of  (h is energy constant; μ is mass ratio of the two primaries; are parameters of triaxial rigid bodies and are radiation parameters). These orbits have been determined by giving displacements along the tangent and normal at the mobile co-ordinates as defined in our papers (Mittal et al. [1]-[3]). These orbits have been drawn by using the predictor-corrector method. We have also studied the effect of triaxial bodies and source of radiation pressure on the periodic orbits by taking fixed value of μ.

Restricted Three-Body Problem, Periodic Orbits, Triaxial Rigid Body, Radiation Pressure

Jain, P. , Aggarwal, R. , Mittal, A. and Abdullah,  . (2016) Periodic Orbits in the Photogravitational Restricted Problem When the Primaries Are Triaxial Rigid Bodies. International Journal of Astronomy and Astrophysics, 6, 111-121. doi: 10.4236/ijaa.2016.61009.