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Seasonal Variation of Micrometeoroid Impacts and Dust Clouds around Saturn’s Rings

  • Authors: Ian-Lin Lai, Wei-Ling Tseng, Hsiang-Wen Hsu, Hua-Shan Shih, Wing-Huen Ip

Ian-Lin Lai et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 4.

Impact flux distribution of micrometeoroid on Saturn’s rings at different orbital phases based on Cassini’s measurement. The X–Y plane represents Saturn’s orbital plane, with the −X-direction pointing toward the Sun and the +Y-direction aligned with Saturn’s orbital motion. Panels (a)−(d) show the mass flux distribution on the northern ring plane at orbital phases of 0° (vernal equinox), 90° (summer solstice), 180° (fall equinox), and 270° (winter solstice), respectively. Panels (e)−(h) are the corresponding mass flux on the southern ring plane.

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