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. 11

Evolution of the orbital parameters of the planets in one simulation of the chain (2:1, 2:1, 4:3) and M_D = 30 M_⊕, to illustrate the smooth planetesimal-driven migration of the planets. The dashed grey line in the background shows the number of planetesimals in the simulation.

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