Migration of a Jupiter in a protoplanetary disk

Details Migration of a Jupiter in a protoplanetary disk Migration of a Jupiter in a protoplanetary disk

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..34..119m&link_type=abstract

IV Reunión sobre Astronomía Dinámica en Latino América (Eds. C. Allen, A. Ruelas, & R. Teixeira) Revista Mexicana de Astronomía

Astronomy and Astrophysics

Astronomy

Accretion, Planets And Satellites: Formation, Solar System: Formation

Scientific paper

We study the formation of planets in a simple model of planetary accretion (Laskar 2000), which includes additionally physical restrictions in the accretion processes and a proto-Jupiter immersed in the protoplanetary disk. Short-time local effects increase the migration of Jupiter and yield wider distributions for the eccentricity. Such three-body processes could explain the large eccentricities observed in exosolar planets.

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