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The problem of densities and composition of terrestrial planets in the light of modern ideas on the origin of meteorites

✍ Scribed by B.J. Levin


Publisher
Elsevier Science
Year
1964
Tongue
English
Weight
164 KB
Volume
3
Category
Article
ISSN
0019-1035

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We perform three-dimensional N-body integrations of the final stages of terrestrial planet formation. We report the results of 10 simulations beginning with 22-50 initial planetary embryos spanning the range 0.5-1.5 AU, each with an initial mass of 0.04-0.13M βŠ• . Collisions are treated as inelastic