The origin of the angular momentum distribution in the solar nebula

Details The origin of the angular momentum distribution in the solar nebula The origin of the angular momentum distribution in the solar nebula

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.186..159c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 186, no. 1, Dec. 1991, p. 159, 160.

Astronomy and Astrophysics

Astrophysics

3

Angular Distribution, Angular Momentum, Interstellar Matter, Solar Corona, Computerized Simulation, Inelastic Scattering, Solar System

Scientific paper

The present study proposes supersonic noncentral collision and coalescence of interstellar matter as a physical process that could lead to the formation of a solar nebula with an appropriate distribution of the spin angular momentum. An idealized chain of events is outlined which may make possible a relevant distribution of the angular momentum due to the very process of the nebula formation, but not internal distribution of it.

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