Particle/Planetesimal Orbital Behavior near Proto-Jupiter

Details Particle/Planetesimal Orbital Behavior near Proto-Jupiter Particle/Planetesimal Orbital Behavior near Proto-Jupiter

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996lpi....27.1217s&link_type=abstract

Lunar and Planetary Science, volume 27, page 1217

Physics

Outer Planets: Development, Planets: Origin, Proto-Jupiter

Scientific paper

It has been suggested that the accumulation time for Mars is dependent upon both the presence as well as development of proto-Jupiter. It has also been suggested that the formation of both the inner and outer planets are directly limited by the developmental time scale of proto-Jupiter. This paper examines the affect a developing proto-Jupiter would have on the orbital trajectories of particles and planetesimals ranging in size from 0.1 m to 100 m.

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