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Evidence from the asteroid belt for a violent past evolution of Jupiter's orbit

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Academic year: 2021

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Fig. 1.— Current orbital distribution (inclination vs. semi major axis) of the asteroid belt
Fig. 2.— Orbital distribution of the asteroid belt at the end of the three step-wise simulations described in the main text
Fig. 3.— Example of an asteroid jumping across the 3:1 resonance with Jupiter. The top panel depicts the semi major axis of the asteroid (bullets) and the location of the 3:1 resonance with Jupiter (solid line) as a function of time
Fig. 4.— Orbital distribution of the asteroid belt after smooth migration of Jupiter and Saturn with τ = 5 My, assuming the belt had an original uniform inclination distribution up to 10 ◦ .
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