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Status: Unchecked ×Keyword: disk aspect ratio ×Clear all

2 claims from 1 paper

1. Physics and Astronomy › Astro and Planetary Science

   OUTWARD MIGRATION OF JUPITER AND SATURN IN 3:2 OR 2:1 RESONANCE IN RADIATIVE DISKS: IMPLICATIONS FOR THE GRAND TACK AND NICE MODELS

   Pierens, Raymond, Nesvorny and Morbidelli · The Astrophysical Journal Letters · 2014

   Simulations of Jupiter and Saturn in disks with viscous heating and radiative cooling find outward migration in 3:2 or 2:1 resonance, with implications for the Grand Tack and Nice models.

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   1. UncheckedIn simulated low-mass disks, Jupiter and Saturn get captured in 2:1 resonance and can migrate outward when viscosity is very low (α ≤ 10^-4).“In disks with relatively low-mass ($M_{disk} \lesssim M_{MMSN}$) , Jupiter and Saturn get captured in 2:1 resonance and can even migrate outward in low-viscosity disks ($α\le 10^{-4}$).”
   2. UncheckedIn N-body runs, a Nice model instability starting from Jupiter and Saturn in 2:1 resonance, after the gas disk disperses, gives good Solar System analogs.“After dispersal of the gaseous disk, a Nice model instability starting with Jupiter and Saturn in 2:1 resonance results in good Solar Systems analogs.”