Electrostatic forces in planetary rings

Details Electrostatic forces in planetary rings Electrostatic forces in planetary rings

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988georl..15...84g&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 15, Jan. 1988, p. 84-87.

Physics

47

Celestial Mechanics, Electrostatics, Jupiter Rings, Planetary Rings, Uranus Rings, Collisionless Plasmas, Gravitational Collapse, Interplanetary Dust, Plasma Clouds, Planets, Rings, Electrostatic Forces, Calculations, Charged Particles, Plasma, Clouds, Density, Temperature, Size, Thickness, Saturn, E Ring, G Ring, F Ring, Uranus, Jupiter, Comparisons, Dust, Grains, Spokes, Perturbations, Collisions

Scientific paper

The average charge on a particle in a particle-plasma cloud, the plasma potential inside the cloud, and the Coulomb force acting on the particle are calculated. The net repulsive electrostatic force on a particle depends on the plasma density, temperature, density of particles, particle size, and the gradient of the particle density. In a uniformly dense ring the electrostatic repulsion is zero. It is also shown that the electrostatic force acts like a pressure force, that even a collisionless ring can be stable against gravitational collapse, and that a finite ring thickness does not necessarily imply a finite velocity dispersion. A simple criterion for the importance of electrostatic forces in planetary rings is derived which involves the calculation of the vertical ring thickness which would result if only electrostatic repulsion were responsible for the finite ring thickness. Electrostatic forces are entirely negligible in the main rings of Saturn and the E and G rings. They may also be negligible in the F ring. However, the Uranian rings and Jupiter's ring seem to be very much influenced by electrostatic repulsion. In fact, electrostatic forces could support a Jovian ring which is an order of magnitude more dense than observed.

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