Yes, and if you model the force on the planet when it travels between them it has a small tidal effect. Depending on the relative orbital planes of the planet and the second binary star system, that may occur any time from once per orbital period to once every 10,000 years. But now try to see how the planet stays in a stable orbit over a billion years. At least in the models I've been able to come up with the tidal effect is assymetric, which is to say the tweak to orbit of the planet is not counter acted by a symmetric tweak on the far side. Even starting with the 'suns' being effectively two point sources 1000AU apart in a bilaterally stable orbit. Trying to find a way to reliably orbit a planet around one of them stably is eluding me. If you can come up with some orbital parameters that work I'd love to see them.
Apologies for my skepticism, my estimate is that the distant binary star system would impart a force on a planet less than 5% that of Jupiter on Earth. Could you provide more details on your n-body simulations? Such as what code base you are using, etc.
Wow that´s great, I have always wondered how astronomers come to calculate the orbits of objects like asteroids or comets just knowing a small part of their movement. Modeling a system as complex as this double double, is just awesome (even if it´s not holding water yet).
What programs are you using? is there a book or web that explains to a layman how this is done?
