Stable planetary orbits around one component in nearby binary stars. II

Details Stable planetary orbits around one component in nearby binary stars. II Stable planetary orbits around one component in nearby binary stars. II

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993cemda..56...45b&link_type=abstract

Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 56, no. 1-2, p. 45-50.

Astronomy and Astrophysics

Astronomy

17

Binary Stars, Digital Simulation, Planetary Orbits, Three Body Problem, Variable Stars, Cool Stars, Stellar Gravitation

Scientific paper

Numerical simulations were performed within the framework of the plane restricted three-body problem to determine the possibility of existence of stable orbits for planets around one of the two components in double stars. The mass ratio of the two stars and the eccentricity of their orbit around each other as well as the phase-space of initial positions and velocities were systematically examined. Data obtained confirm that stable potential planetary orbits around one component of double stars exist up to distance if their parent star of the order or more of half the periastron separation of the binary.

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