On the Model of Motion of Giant Planets Rings Arcs

Details On the Model of Motion of Giant Planets Rings Arcs On the Model of Motion of Giant Planets Rings Arcs

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1685p&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1685

Physics

Scientific paper

Perturbed four body (a planets, two satellites of equal mass and a
particle) central configuration is under consideration. For ratio of
mass of planets M and satellites m M/m>1150 the stable arcs of rings
are formed near the planets.

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