Planetary orbits in the elliptic restricted problem. II - The Sirius system

Details Planetary orbits in the elliptic restricted problem. II - The Sirius system Planetary orbits in the elliptic restricted problem. II - The Sirius system

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...223..361b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 223, no. 1-2, Oct. 1989, p. 361-364.

Astronomy and Astrophysics

Astrophysics

19

Celestial Mechanics, Extrasolar Planets, Orbital Elements, Solar Orbits, Three Body Problem, Astronomical Models, Binary Stars, Orbit Calculation

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 Sirius 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 and the Alpha-Centauri elliptic cases, are found to exist around Sirius A and Sirius B up to distances from each star of the order of more than half the binary's periastron separation.

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