Physics
Scientific paper
Apr 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981m%26p....24..231l&link_type=abstract
Moon and the Planets, vol. 24, Apr. 1981, p. 231-243.
Physics
Particle Motion, Poynting-Robertson Effect, Protostars, Solar Radiation, Stellar Luminosity, Sun, Gravitational Effects, Radiation Effects, Solar Physics
Scientific paper
The motion of particles in the vicinity of the protosun at the Hayashi stage is analyzed in terms of an idealized model assuming that uncharged particles move around the protosun of quasi-circular orbits in a transparent space. Consideration is given to the zone of predominance of the effect of variable luminosity and Poynting-Robertson effect during the increase of luminosity, character of drift for linear increase of luminosity with time, drift pattern for some variants of increase of luminosity, and drift pattern during the decrease of luminosity.
Levin Iu. B.
Simonenko A. N.
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