Computer Science
Scientific paper
Nov 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106..210i&link_type=abstract
Icarus, vol. 106, p. 210
Computer Science
151
Protoplanets, Mass Distribution, Planetary Evolution, Many Body Problem, Computerized Simulation, Scattering, Spatial Distribution, Mass Ratios
Scientific paper
N-body simulations are conducted to study the evolution of random velocities of planetesimals due to scattering by a protoplanet; if the protoplanet's mass is sufficiently great, the inclinations and eccentricities of planetesimals in the protoplanet's vicinity are enhanced by perturbations of the protoplanet, rather than those of the planetesimals. On the basis of the results thus obtained, a two-step growth scenario for a protoplanet is proposed in whose second stage growth gradually decreases due to eccentricity and inclination increases due to perturbations.
Ida Shigeru
Makino Junichiro
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