Families of periodic orbits for trojan planets, with eccentricity and mutual inclination

GIUPPONE C. A.; LEIVA A. M.

Aguas de Lindoia

Congreso; XVII Coloquio Brasilero de Dinámica Orbital; 2014

Observatorio Nacional

During last years the study of 1/1 Mean Motion Resonance achieved attention in the frame of the general planetary problem. In this called coorbital resonance we have two planets orbiting a star with a period-ratio equal to one, and beyond the classical studied Trojan and Horse-Shoe kind of orbits there are another regular orbits recently discovered but not yet confirmed in the extrasolar planet population. Our aim is to extend our knowledge of these coorbital types of orbits further than circular and coplanar orbits, giving an analytical expression of the Hamiltonian coefficients and analyzing their validity.