Computer Science
Scientific paper
Jun 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981sciam.244..163w&link_type=abstract
Scientific American, vol. 244, June 1981, p. 163-170, 173, 174.
Computer Science
1
Earth (Planet), Planetary Evolution, Protoplanets, Collisions, Computerized Simulation, Solar System
Scientific paper
A state-of-the-art review is given of the current understanding of planet formation by the accumulation of planetesimals. Emphasis is placed on recent computer simulation studies of this process, and illustrations depict the orbital and mass distribution patterns obtained by simulation at various phases of accretion. Simulations show that the formation was virtually complete about 100 million years after it began, and that the newly 2ormed planet was so hot that much of its interior was molten.
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