Evolution of the orbital eccentricities of planetesimals during formation of the giant planets

Details Evolution of the orbital eccentricities of planetesimals during formation of the giant planets Evolution of the orbital eccentricities of planetesimals during formation of the giant planets

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989sosyr..23..119i&link_type=abstract

Solar Syst. Res., vol. 23, No. 3, p. 119-125 (1989).

Computer Science

1

Accumulation Of Planets, Disks Of Planetesimals, Eccentricities, Terrestrial Planets, Giant Planets, Computer Simulation, Ejected Bodies

Scientific paper

Changes in orbital eccentricities during the evolution of disks containing a large number (˜ 106 - 1012) of planetesimals are studied. These studies were carried out on the basis of computer simulation results obtained for the evolution of disks initially consisting of hundreds of bodies which moved around the sun. It is shown that the Safronov parameter theta can change substantially during the evolution. The mass of bodies ejected into hyperbolic orbits from the zones of the giant planets could exceed the mass of the solid material incorporated into the planets by an order of magnitude.

Affiliated with

Also associated with

No associations

Rating

Evolution of the orbital eccentricities of planetesimals during formation of the giant planets does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Evolution of the orbital eccentricities of planetesimals during formation of the giant planets, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Evolution of the orbital eccentricities of planetesimals during formation of the giant planets will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1827339