I have updated the Euler page about the 3-body problem. It is nice to see three bodies with different masses.

The plot shows three bodies. It is centered in the biggest one with mass 2. The blue one has mass 1, and the orange planet has mass 0.1. The planet moves around the central star until it gets caught by the outer sun for some time. Then it returns back to an orbit around the central object. You can also see how the 0.1 mass distorts the orbit of the two suns.