Abstract
The formation of the giant planets seems to be best explained by accretion of planetesimals to form massive cores, which in the case of Jupiter and Saturn were able to capture nebular gas. However, the timescale for accretion of such cores has been a problem. Accretion in the outer solar system differs qualitatively from planetary growth in the terrestrial region, as the larger embryo masses and lower orbital velocities make bodies more subject to gravitational scattering. The planetesimal swarm in the outer nebula may be seeded by earlier-formed large bodies scattered from the region near the nebular “snow line”. Such a seed body can experience rapid runaway growth undisturbed by competitors; the style of growth is not oligarchy, but monarchy.
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Weidenschilling, S.J. Formation of the Cores of the Outer Planets. Space Sci Rev 116, 53–66 (2005). https://doi.org/10.1007/s11214-005-1947-1
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DOI: https://doi.org/10.1007/s11214-005-1947-1