Triaxial gravitational fields of small solar system bodies stabilize narrow rings against solar radiation pressure loss, allowing sub-mm particles to persist.
L., Sicardy, B., Morgado, B
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Rings Around Non-Spherical Worlds: Sub-mm Dust Retention Around Triaxial Small Bodies in the Solar System
Triaxial gravitational fields of small solar system bodies stabilize narrow rings against solar radiation pressure loss, allowing sub-mm particles to persist.