Astronomy and Astrophysics · 2011 · 46 citations · 55 references
Context. In the last few years, the so-called “Nice model” has become increasingly significant for studying the formation and evolution of the solar system. According to this model, the initial orbital configuration of the giant planets was much more compact than the one we observe today.
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Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
James B. Pollack, O. Hubickyj, Peter Bodenheimer et al. · Icarus · 1996 · 3K citations
Disk Frequencies and Lifetimes in Young Clusters
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Origin of the orbital architecture of the giant planets of the Solar System
K. Tsiganis, R. S. Gomes, Alessandro Morbidelli et al. · Nature · 2005 · 1.4K citations