Planetary orbits in the elliptic restricted problem. I - The Alpha Centauri system

Details Planetary orbits in the elliptic restricted problem. I - The Alpha Centauri system Planetary orbits in the elliptic restricted problem. I - The Alpha Centauri system

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...206..143b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 206, no. 1, Nov. 1988, p. 143-146.

Astronomy and Astrophysics

Astrophysics

26

Binary Stars, Orbit Perturbation, Orbital Mechanics, Planetary Orbits, Three Body Problem, Centaurus Constellation, Elliptical Orbits

Scientific paper

Numerical simulations are made within the frame of the elliptic plane restricted three-body problem, in order to search if stable orbits exist for planets around one of the two components in double stars. The α Cen system is investigated here. Large stable planetary orbits, already known to exist through a systematic exploration of the circular model and for the Sun-Jupiter elliptic case, are found to exist around α Cen A and α Cen B up to distances from each star of the order of more than half the binary's periastron separation.

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