Fig. 5
Semimajor axes, eccentricities, resonant angles, and period-ratio evolution of one of the stable fits for 10 Myr. Planet b is shown in green, while planet c is in red. The left panel shows a 100 yr zoomed region of the complete 10 Myr simulation, shown in the right panel (we note the logarithmic scale in the X-axis). The system suffers from strong gravitational interactions on very short timescales, but it can preserve stability for 10 Myr.
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