New numerical models on giant planet formation

Details New numerical models on giant planet formation New numerical models on giant planet formation

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006rmxac..26....3f&link_type=abstract

XI IAU Regional Latin American Meeting of Astronomy (Eds. L. Infante & M. Rubio) Revista Mexicana de Astronomía y Astrofísica (S

Astronomy and Astrophysics

Astronomy

Planets And Satellites: Formation

Scientific paper

We present our results on giant planet formation in the frame of the
nucleated instability mechanism. We consider the oligarchic growth
regime for the solid core and a reduction in the grain opacity. Under
these assumptions, in situ giant planet formation is achievable in a
timescale shorter than the lifetime of protoplanetary disks.

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