Motion about equilibrium points in the Jupiter-Europa system with oblateness

Abstract The study of motion a test mass in the vicinity an equilibrium point under frame restricted three body problem (RTBP) plays important role trajectory design for different space missions. In this paper, infinitesimal has been described Jupiter-Europa system with oblateness. At first, we have determined points and then performed linear stability tests influence oblateness both primaries. We found that due to oblateness, considerable deviation existing results occurred. Next, computed tadpole horseshoe orbits neighbourhood triangular effect is recorded on these orbits. Finally, evolution about estimated by using Poincaré surface section technique it noticed presence quasi-periodic orbit dominates over chaotic zones. These will help further more generalised models perturbations.