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Habitable Planet Formation in Binary Star Systems

✍ Scribed by Daniel P Whitmire; John J Matese; Lee Criswell; Seppo Mikkola

Publisher
Elsevier Science
Year
1998
Tongue
English
Weight
287 KB
Volume
132
Category
Article
ISSN
0019-1035

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✦ Synopsis

AU), or when the secondary has a very low mass and near

The accretion of planetesimals from a turbulent gas and circular orbit as in the Sun-Jupiter system. The discrepancy dust nebula is not well understood theoretically even in with the present numerical study is due in part to the different the case of our own Solar System. Nonetheless, dust grains runaway accretion time scales assumed and the neglect in the managed to collect into planetesimals even in the parent earlier study of an exact criterion for crossing orbits.

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✍ Vittorio Banfi πŸ“‚ Article πŸ“… 1991 πŸ› Springer Netherlands 🌐 English βš– 595 KB

A theoretical model, based on particular type of the restricted three-body problem, is here presented in order to demonstrate the existence of a possible planetary motion near the center of mass in a binary star system. The superposition principle is used, with the introduction of two fictitious neg