Abstract
The distribution of particle sizes in Saturn's rings is probably continuous over many orders of magnitude; there is no ‘typical particle size’. A model based on this view accounts for a number of observed properties of the rings: apparent thickness, radar and radio observations, number and size distribution of the gaps discovered by Voyager 1, and optical thickness.
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Hénon, M. A simple model of Saturn's rings. Nature 293, 33–35 (1981). https://doi.org/10.1038/293033a0
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DOI: https://doi.org/10.1038/293033a0
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