The Solar System could have formed in a low-viscosity disc: A dynamical study from giant planet migration to the Nice model

Open Access

Fig. 3

Same as Fig. 2, but with Neptune’s introduction time T_N_,0 = 238 000 yr, namely simulation N_bis4. Here Uranus is ejected from the system at 355 000 yr. We add another Uranus-mass ice giant later in the simulation and obtain the final resonance chain (2:1, 2:1, 4:3).

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