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Observable consequences of planet formation models in systems with close-in terrestrial planets

✍ Scribed by Sean N. Raymond; Rory Barnes; Avi M. Mandell

Book ID
110842552
Publisher
John Wiley and Sons
Year
2008
Tongue
English
Weight
848 KB
Volume
384
Category
Article
ISSN
0035-8711

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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