Mass loss from the proto-sun - Formation and evolution of the solar nebula

Details Mass loss from the proto-sun - Formation and evolution of the solar nebula Mass loss from the proto-sun - Formation and evolution of the solar nebula

Jun 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984apj...281..375t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 281, June 1, 1984, p. 375-380.

Astronomy and Astrophysics

Astrophysics

2

Interplanetary Medium, Protostars, Solar System, Stellar Evolution, Stellar Mass Ejection, Sun, Angular Momentum, Chemical Evolution, Equations Of Motion, Mass Distribution, Planets, T Tauri Stars

Scientific paper

The author considers the formation and evolution of the solar nebula in the light of observations of T Tauri stars, oxygen-isotopic anomalies in meteorites, and the mass and angular momentum distribution in the present solar system. He argues that the solar nebula and hence the planetary system were formed from the mass ejected by the proto-Sun, whose strong magnetic field controlled the azimuthal and radial flow of the ejected material.

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