Dynamics of the β Pictoris planetary system and its falling evaporating bodies

Open Access

Fig. 1

Secular evolution over 10⁸ yr of the β Pic b+c two-planet system corresponding to solution #2 from Table 1. From left to right: semi-major axes, eccentricities, and mutual inclination. The logarithmic time axes highlight the short-term as well as the long-term behaviour. Red always stands for β Pic c and green for β Pic b.

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