Catalogue 3D - Inclined Trojan planets

The restricted three body problem (RTBP) is the basic model for studying the dynamics of small bodies in our Solar system and Trojan planets in Extrasolar planetary systems. For inclined orbits, the spatial or three-dimensional (3D) RTBP should be considered as the basic model. The aim of the present work is a systematic study of three dimensional (3D) orbits of the RTBP, which will as soon as possible presented on this page!

First results are shown in the poster presentation from the IAU Symposium No.249