Figure 1:

Total particle mass flux (g m⁻² s⁻¹) in each mass bin encountering Jupiter (Top left), Saturn (Top right), Uranus (Bottom left), and Neptune (Bottom right) at the planet’s exobase, for dust populations from Jupiter-family comets (orange), the Edgeworth-Kuiper belt (green), and Oort-Cloud comets (blue). Particles were grouped into bins based on mass, with 2 bins per decade of mass. The solid curves are from Poppe (2016), and the dashed curves were extrapolated as described in the text. (For interpretation of the references to color in this figure legend, the reader is referred to the web version of this article.)