Saturn's G ring: insights from the dynamical evolution of dust particles from the G-ring arc
Zhenghan Chen, Xiaodong Liu, Kun Yang

TL;DR
This study models the dynamical evolution of dust particles in Saturn's G ring to explain observed properties and estimate its age, particle distribution, and lifetime.
Contribution
It introduces a detailed numerical simulation of dust dynamics that explains the G ring's observed brightness and estimates its physical and temporal characteristics.
Findings
Dust particles follow a power-law size distribution with an exponent of 2.8.
Dominant dust particle sizes are between 5 and 10 micrometers.
Estimated age of the G ring is between 1 million and 10 million years.
Abstract
To explore the formation and properties of Saturn's G ring, we study the dynamics of micron-sized dust particles originating from the arc of debris near the inner edge of the ring. The dynamical evolution of particles due to various perturbation forces and the plasma sputtering that erodes the particles is simulated by a well-tested numerical code. Based on the simulation results, the normal of the G ring observed by the Cassini spacecraft can be explained by dust particles originating from the arc. Other properties of the G ring are also estimated, including the steady-state size distribution and the number density of ring particles, the geometric optical depth, the apparent edge-on thickness, the age and the remaining lifetime of the G ring. We find that the particle size distribution of the G ring follows a power law with an exponent of 2.8, and dust particles in the size range…
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