Satellite-type planetary orbits in double stars - A numerical approach

Details Satellite-type planetary orbits in double stars - A numerical approach Satellite-type planetary orbits in double stars - A numerical approach

Feb 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...191..385r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 191, no. 2, Feb. 1988, p. 385-391.

Astronomy and Astrophysics

Astrophysics

46

Double Stars, Planetary Orbits, Planetary Systems, Eccentricity, Numerical Integration

Scientific paper

The problem of planets in double stars is discussed in this study from the celestial mechanics point of view. One type of planet is the P-type surrounding both primaries in a direct orbit, the other interesting one is the S-type, orbiting only one of the primaries in the double star. The P-types were examined in a detailed numerical study by Dvorak (1986); the direct S-types in binaries with equal masses are examined in this paper. The aim is to establish stability zones for S-types. The model chosen for this analysis is the elliptic restricted three-body problem, the primaries are assumed to have equal masses.

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