Astronomy and Astrophysics – Astrophysics – Earth and Planetary Astrophysics
Scientific paper
2011-01-28
Astrophysics and Space Science, Volume 333, Number 1, 49-59(2011)
Astronomy and Astrophysics
Astrophysics
Earth and Planetary Astrophysics
Accepted for publication in Astrophysics & Space Science
Scientific paper
10.1007/s10509-011-0632-y
The dynamical behaviour of near by trajectories is being estimated by Lyapunov Characteristic Exponents(LCEs) in the Generalized Photogravitational Chermnykh-Like problem. It is found that the trajectories of the Lagrangian point $L_4$ move along the epicycloid path, and spirally depart from the vicinity of the point. The LCEs remain positive for all the cases and depend on the initial deviation vector as well as renormalization time step. It is noticed that the trajectories are chaotic in nature and the $L_4$ is asymptotically stable. The effects of radiation pressure, oblateness and mass of the belt are also examined in the present model.
No associations
LandOfFree
Trajectories of $L_4$ and Lyapunov Characteristic Exponents in the Generalized Photogravitational Chermnykh-Like Problem does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Trajectories of $L_4$ and Lyapunov Characteristic Exponents in the Generalized Photogravitational Chermnykh-Like Problem, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Trajectories of $L_4$ and Lyapunov Characteristic Exponents in the Generalized Photogravitational Chermnykh-Like Problem will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-551425