Possible discrete annular dust formations around Mars and Venus

Computer Science

Scientific paper

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Mars (Planet), Micrometeoroids, Planetary Rings, Standing Waves, Venus (Planet), Gravitational Effects, Mars Satellites, Solar Planetary Interactions, Terrestrial Dust Belt

Scientific paper

The positions of possible annular dust belts around Mars and Venus are
calculated on the basis of the statistical theory of quasi-isoenergetic
complexes in the form of radial standing waves. A comparison of the
theoretically calculated and observed semimajor axes of the orbits of
the Mars satellites is presented.

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