Models of the formation of the solar nebula

Details Models of the formation of the solar nebula Models of the formation of the solar nebula

Jan 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icar...53...26c&link_type=abstract

Icarus, vol. 53, Jan. 1983, p. 26-40.

Astronomy and Astrophysics

Astronomy

57

Gravitational Collapse, Interplanetary Medium, Protoplanets, Protostars, Solar Corona, Solar System, Angular Momentum, Astronomical Models, Cosmology, Evolution (Development), Photosphere, Solar Temperature

Scientific paper

Protostellar cloud collapse and solar nebula formation models indicate that the size of the nebula produced will be larger in terms of both gas centrifugal balance R(CF) and collapse time diffusion length R(V). From this, it can be deduced that low mass nebulas are produced if (R(V)/R(CF))-squared is much greater than unity, while nebulas result for values lower than approximately unity. The total angular momentum value distinguishes most current models of the solar nebula. Analytic expressions for the surface density, nebular mass flux and photospheric temperature distributions during the formation stage are presented for simple modes illustrating and general properties of growing protostellar disks.

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