Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1979
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979avest..12..160r&link_type=abstract
(Astronomicheskii Vestnik, vol. 12, July-Sept. 1978, p. 160-166.) Solar System Research, vol. 12, no. 3, Jan. 1979, p. 134-140.
Astronomy and Astrophysics
Astronomy
Meteoroid Dust Clouds, Solar Activity Effects, Stellar Luminosity, Stellar Mass, Weight Reduction, Evolution (Development), Solar Radiation
Scientific paper
It is shown that the sun's effective mass is decreasing due to the repulsion of light by an amount varying from 20 times the mass of Jupiter for particle radii of order 0.001 cm to six earth masses for particles with of order 1 cm. It is determined that the nonuniform reduction in the sun's mass is the strongest mechanism for the evolution and decay of meteor swarms. It is shown that an accumulation of particles having radius greater than or equal to 0.001 cm and similar motion parameters will become stretched out along the entire orbit over a time on the order of 100 years. The effect of particle differentiation in terms of size and speed on the behavior of the luminosity function and the displacement in the radiant when the flow encounters the earth is studied.
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