2015/04/23 by F. A. Abd El-Salam, El-Salam, F. A. Abd, F. A. El-Salam
Engineering · Physics and Astronomy · #70E50 #70M20 #Earth and Planetary Astrophysics (astro-ph.EP) #FOS: Physical sciences #Nonlinear Waves and Solitons #Spacecraft Dynamics and Control #astro-ph.EP #msc:70E50 #msc:70M20
paper · pdf · doi:10.48550/arxiv.1506.02687
26 pages
arxiv created 2015/04/23 · openalex publication_date 2015/04/23 · arxiv updated 2015/06/10 · openalex created_date 2022/09/30 · openalex updated_date 2026/07/28
The multi-dissipative photogravitational triaxial elliptic restricted three body problem is treated. The perturbed locations of triangular points are computed. The stability of the triangular points under changing one or more perturbing parameter is investigated. The results revealed that at certain values of the considered perturbing parameters, we haven't triangular equilibrium points, or at least there exists but very far from the origin. The change in the stability/instability regions with eccentricity seems to be nonlinear. It seems that increasing the eccentricity the enlarge the stability regions and vice versa. It is revealed that we have two disjoint stability regions. The stability/instability regions for a new set of eccentricities are merged to one region. Consider a very high eccentricity stability region for the whole domain of the mass ratio except in the neighborhood of 0.3 is obtained. stability/asymptotic stability/instability regions due to certain photogravitational effects correspond are revealed.