Radiative braking and resonance phenomena in the motion of interplanetary dust

Details Radiative braking and resonance phenomena in the motion of interplanetary dust Radiative braking and resonance phenomena in the motion of interplanetary dust

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13.1080k&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, Dec. 1987, p. 1080-1085. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Interplanetary Dust, Particle Motion, Poynting-Robertson Effect, Braking, Jupiter (Planet), Radiation Pressure, Resonance, Solar System

Scientific paper

Dissipation due to the Robertson-Poynting effect generates a resonance structure in the plane model of the sun-Jupiter-dust system with noninteracting dust particles. Each value for the period of rotation radially commensurate with Jupiter's period and exceeding the latter corresponds to a single-parameter set of asymptotically stable orbits. The particles captured in the fixed resonance are aligned along a synodical orbit with Jupiter enclosed in one of its loops. The motion of the particles is synchronized such a way that the pattern formed by them is constantly reproducing itself while rotating around the sun following Jupiter.

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