Statistics – Computation
Scientific paper
Oct 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987brig.iafcs....r&link_type=abstract
IAF, International Astronautical Congress, 38th, Brighton, England, Oct. 10-17, 1987. 5 p.
Statistics
Computation
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.
No associations
LandOfFree
Origin and ability of planetary systems does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Origin and ability of planetary systems, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Origin and ability of planetary systems will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1774066