Research on the early history of the solar system

Details Research on the early history of the solar system Research on the early history of the solar system

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pggp.rept..146c&link_type=abstract

In NASA, Washington Rept. of Planetary Geol. and Geophys. Program, 1984 p 146-148 (SEE N85-23474 13-91)

Other

Galactic Evolution, Solar Corona, Stellar Evolution, Stellar Mass Accretion, Stellar Structure, Baroclinic Instability, Celestial Mechanics, Disk Galaxies, Protoplanets, Roche Limit, Stellar Mass

Scientific paper

The evolution of a dissipating turbulently viscous disk of gas and dust formed during the collapse of an interstellar cloud fragment and how it relates to the early history of the solar system is discussed. Results from calculations on modelling the inner parts of the primitive solar nebula subject to the assumption of a steady inward flow are given. Other calculations are reviewed which simulate the accretion of a star from an accretion disk. Scenarios for the evolution of the primitive solar nebula and the formation of the Moon as a result of a major collision with the protoearth are described.

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