The Dynamical Structure of the Kuiper Belt and its Primordial Origin
Astrophysics
2007-05-23 v1
Abstract
This chapter discusses the dynamical properties of the Kuiper belt population. Then, it focuses on the characteristics of the Kuiper belt that cannot be explained by its evolution in the framework of the current solar system. We review models of primordial solar system evolution that have been proposed to reproduce the Kuiper belt features, outlining advantages and problems of each of them.
Keywords
Cite
@article{arxiv.astro-ph/0703558,
title = {The Dynamical Structure of the Kuiper Belt and its Primordial Origin},
author = {A. Morbidelli and H. F. Levison and R. Gomes},
journal= {arXiv preprint arXiv:astro-ph/0703558},
year = {2007}
}
Comments
to be published in `Transneptunian Objects', Barucci et al. eds., University of Arizona Press