On possible circumbinary configurations of the planetary systems of α Centauri and EZ Aquarii
Abstract
Possible configurations of the planetary systems of the binary stars α Cen ABandEZAqr AC are analyzed. The Ptype orbits—circumbinary ones, i.e., the orbits around both stars of the binary, are studied. The choice of these systems is dictated by the fact that α Cen is closest to us in the Galaxy, while EZ Aqr is the closest system whose circumbinary planets, as it turns out, may reside in the "habitability zone." The analysis has been performed within the framework of the planar restricted threebody problem. The stability diagrams of circumbinary motion have been constructed: on representative sets of initial data (in the pericentric distanceeccentricity plane), we have computed the Lyapunov spectra of planetary motion and identified the domains of regular and chaotic motion through their statistical analysis. Based on present views of the dynamics and architecture of circumbinary planetary systems, we have determined the most probable planetary orbits to be at the centers of the main resonance cells, at the boundary of the dynamical chaos domain around the parent binary star, which allows the semimajor axes of the orbits to be predicted. In the case of EZ Aqr, the orbit of the circumbinary planet is near the habitability zone and, given that the boundary of this zone is uncertain, may belong to it.
 Publication:

Astronomy Letters
 Pub Date:
 April 2016
 DOI:
 10.1134/S106377371604006X
 Bibcode:
 2016AstL...42..260P
 Keywords:

 celestial mechanics;
 planetary systems;
 binary stars;
 α Centauri;
 EZ Aquarii;
 methods;
 numerical