rohb.vogue
Rohb Vogue
The planetary considerations here are completely dependent on the size of the stars in question and the the distance between them. Using our own solar system is probably not the best example however though because the stellar distances are not rational; Sol and Jupiter are just too close.
The gravitational issues would not create odd orbits at all. (By odd here, I mean figure 8's and such) The system I'd use is to imagine every planet attached to its star by a string. the string represents gravity. The stronger the pull, the thicker the string. So what happens as each planet orbits its own star in the binary system: you always get a roughly circular orbit. The ellipses are produced by the temporary stronger pull as the planet passes nearer to the second star. So the deviation outside a circle depends on the strength of that 2nd gravitational tug. if the stars are too close-as in the example of sol and Jupiter, the planet gets pulled apart. i think that pretty much covers it.
The gravitational issues would not create odd orbits at all. (By odd here, I mean figure 8's and such) The system I'd use is to imagine every planet attached to its star by a string. the string represents gravity. The stronger the pull, the thicker the string. So what happens as each planet orbits its own star in the binary system: you always get a roughly circular orbit. The ellipses are produced by the temporary stronger pull as the planet passes nearer to the second star. So the deviation outside a circle depends on the strength of that 2nd gravitational tug. if the stars are too close-as in the example of sol and Jupiter, the planet gets pulled apart. i think that pretty much covers it.