The supernova fragmentation model of solar system formation

Details The supernova fragmentation model of solar system formation The supernova fragmentation model of solar system formation

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123..161b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 1, June 1986, p. 161-181.

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Astronomical Models, Computational Astrophysics, Galactic Evolution, Solar System, Stellar Evolution, Supernova Remnants, Computer Programs, Mass Distribution, Nebulae, Planetary Evolution, Reversed Flow, Stellar Envelopes

Scientific paper

The authors have further developed Brown's model of solar system formation. In this model, each fragment of an ejected supernova shell evolves into a separate solar system. Specifically, the authors have formulated the reverse-flow hypothesis that may be responsible for the inner, earthlike planets. They have written a computer program with which it is possible to calculate mass distributions within a solar nebula. They have found mass distributions similar to our solar system over a wide range of the model parameters.

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