The dispersal of the solar nebula by the solar wind

Details The dispersal of the solar nebula by the solar wind The dispersal of the solar nebula by the solar wind

Aug 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976obs....96..140h&link_type=abstract

The Observatory, vol. 96, Aug. 1976, p. 140-142.

Mathematics

10

Plasma-Particle Interactions, Solar System, Solar Wind, Escape Velocity, Kinetic Energy, Mass Transfer, Mathematical Models, Particle Motion

Scientific paper

The effect of a continuous spherically symmetric solar wind on a solar
nebula assumed to be in equilibrium about the sun before the onset of
the wind is analyzed to test the hypothesis that the solar nebula would
be swept away by the onset of the T Tauri-stage mass loss. The results
show that the T Tauri solar wind would not disperse the solar nebula.

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