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- W2766068051 abstract "The origin of the orbital structure of the cold component of the Kuiper belt is still a hot subject of investigation. Several features of the solar system suggest that the giant planets underwent a phase of global dynamical instability, but the actual dynamical evolution of the planets during the instability is still debated. To explain the structure of the cold Kuiper belt, Nesvorny (2015, AJ 150,68) argued for a ”soft” instability, during which Neptune never achieved a very eccentric orbit. Here we investigate the possibility of a more violent instability, from an initially more compact fully resonant configuration of 5 giant planets. We show that the orbital structure of the cold Kuiper belt can be reproduced quite well provided that the cold population formed in situ, with an outer edge between 44−45 au and never had a large mass." @default.
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- W2766068051 date "2018-05-01" @default.
- W2766068051 modified "2023-10-18" @default.
- W2766068051 title "Checking the compatibility of the cold Kuiper belt with a planetary instability migration model" @default.
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- W2766068051 doi "https://doi.org/10.1016/j.icarus.2017.10.018" @default.
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