Formation Of The Terrestrial Planets From A Narrow Annulus

Details Formation Of The Terrestrial Planets From A Narrow Annulus Formation Of The Terrestrial Planets From A Narrow Annulus

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21534404h&link_type=abstract

American Astronomical Society, AAS Meeting #215, #344.04; Bulletin of the American Astronomical Society, Vol. 42, p.451

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Current models of the assembly of the terrestrial planets succeed in reproducing several features of the solar system configuration, but continue to suffer from several long-standing quantitative shortcomings. These include overpredicting the masses of Mercury and Mars, as well as the planetary eccentricities and spatial extent of the planetary grouping. I will discuss how starting from a radically different initial condition may alleviate some of these problems, and may connect the Solar System to the dynamically active planetary systems around other stars.

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