Origin and ability of planetary systems

Statistics – Computation

Scientific paper

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Angular Momentum, Binary Stars, Origins, Planetary Systems, Solar Radiation, Brown Dwarf Stars, Computational Astrophysics, Interstellar Magnetic Fields

Scientific paper

The formation of a planetary system from the collapse of a cloud is discussed. The cloud's angular momentum J must be small enough to form a starlike core with a mass of at least 0.01 solar, but to form planets the cloud's J must exceed the minimum necessary to form a single star. The disk from which planets form originates from the equatorial layer of the core of the cloud, and spreads out due to magnetic and turbulent torques. This model can explain the lack of brown dwarf companions to solar type stars.

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