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- W313321860 abstract "The implications and limitations of program ACRETE were tested. The program is a scheme based on Newtonian physics and accretion with unit sticking efficiency, devised to simulate the origin of the planets. The dependence of the results on a variety of radial and vertical density distribution laws, the ratio of gas to dust in the solar nebula, the total nebular mass, and the orbital eccentricity of the accreting grains was explored. Only for a small subset of conceivable cases are planetary systems closely like our own generated. Many models have tendencies towards one of two preferred configurations: multiple star systems, or planetary systems in which Jovian planets either have substantially smaller masses than in our system or are absent altogether. But for a wide range of cases recognizable planetary systems are generated-anging from multiple star systems with accompanying planets, to systems with Jovian planets at several hundred AU, to single stars surrounded only by asteroids." @default.
- W313321860 created "2016-06-24" @default.
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- W313321860 date "1976-10-01" @default.
- W313321860 modified "2023-09-27" @default.
- W313321860 title "Computer simulations of planetary accretion dynamics: sensitivity to initial conditions. [Implications and limitations of ACRETE]" @default.
- W313321860 hasPublicationYear "1976" @default.
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