Long-term orbital stability of exosolar planetary systems with highly eccentric orbits

Nowadays, many extrasolar planetary systems possessing at least one planet on a highly eccentric orbit have been discovered. In this work, we study the possible long-term stability of such systems. We consider the general three body problem as our model. Highly eccentric orbits are out of the Hill s...

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Veröffentlicht in:	Proceedings of the International Astronomical Union 2015-08, Vol.11 (A29A), p.38-39
Hauptverfasser:	Antoniadou, Kyriaki I., Voyatzis, George
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Contributed Papers Dynamic stability Eccentric orbits Extrasolar planets Motion stability Orbital elements Orbital resonances (celestial mechanics) Orbital stability Orbits Planetary systems Three body problem
Online-Zugang:	Volltext
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